Issue 
A&A
Volume 513, April 2010



Article Number  A47  
Number of page(s)  16  
Section  Astrophysical processes  
DOI  https://doi.org/10.1051/00046361/200913169  
Published online  23 April 2010 
Low magneticPrandtl number flow configurations for cold astrophysical disk models: speculation and analysis
O. M. Umurhan^{1,2}
1  Astronomy Unit, School of Mathematical Sciences, Queen Mary
University of London, London E1 4NS, UK
2 
Astronomy Department, City College of San Francisco,
San Francisco, CA 94112, USA
Received 24 August 2009 / Accepted 28 January 2010
Abstract
Context. Simulations of astrophysical disks in the shearing
box that are subject to the magnetorotational instability (MRI) show
that activity appears to be reduced as the magnetic Prandtl
number
is
lowered. It is therefore important to understand the reasons for
this trend, especially if this trend is shown to continue when higher
resolution calculations are performed in the near future. Calculations
for laboratory experiments show that saturation is achieved through
modification of the background shear for
.
Aims. Guided by the results of calculations appropriate for laboratory experiments when
is very low, the stability of inviscid disturbances in a shearing box
model immersed in a constant vertical background magnetic field is
considered under a variety of shear profiles and boundary conditions in
order to evaluate the hypothesis that modifications of the shear bring
about saturation of the instability. Shear profiles q are given by the local background Keplerian mean, q_{0}, plus timeindependent departures, Q(x), with zero average on a given scale.
Methods. The axisymmetric linear stability of inviscid magnetohydrodynamic normal modes in the shearing box is analyzed.
Results. (i) The stability/instability of modes subject to
modified shear profiles may be interpreted by a generalized Velikhov
criterion given by an effective shear and radial wavenumber that are
defined by the radial structure of the mode and the form of Q. (ii) Where channel modes occur, comparisons against marginally unstable disturbance in the classical case, Q=0,
shows that all modifications of the shear examined here enhance mode
instability. (iii) For models with boundary conditions mimicing
laboratory experiments, modified shear profiles exist that stabilize a
marginally unstable MRI for Q=0. (iv) Localized normal
modes on domains of infinite radial extent characterized by either
single defects or symmetric tophat profiles for Q are also
investigated. If the regions of modified shear are less (greater)
than the local Keplerian background, then there are (are no)
normal modes leading to the MRI.
Conclusions. The emergence and stability of the MRI is sensitive
to the boundary conditions adopted. Channel modes do not appear to be
stabilized through modifications of the background shear whose average
remains Keplerian. However, systems that have nonpenetrative
boundaries can saturate the MRI through modification of the background
shear. Conceptually equating the qualitative results from laboratory
experiments to the conditions in a disk may therefore be misleading.
Key words: accretion, accretion disks  magnetohydrodynamics (MHD)  instabilities  protoplanetary disks
1 Introduction
After almost 40 years of investigation the source of the anomalous transport in accretion disks still remains an open question. As it is mostly assumed that the transport is a reflection of some underlying turbulent state, identification of its source mechanism and process has been the focus of much research activity. A leading candidate mechanism is the magnetorotational instability (Balbus & Hawley 1991).
The magnetic Prandtl number (), i.e. the ratio of a fluid's viscosity to its magnetic diffusivity, appears to play an important role in the ability of the MRI to drive a fullydeveloped turbulent state. Recently resolved simulations of the MRI in a shearing box environment (e.g. Lesur & Longaretti 2007; Fromang et al. 2008) show the appearance of a turbulent state for moderately high Reynolds numbers (Re) when is an order 1 quantity or higher. However, the amount of transport delivered by the MRI appears to depend on : as this quantity decreases the vigor of the turbulent state decreases and if drops below some critical value, then the turbulence appears to vanish altogether.
Estimates of the properties of cold astrophysical disks, like protoplanetary disks, show that their characteristic 's are on the order of 10^{6} at best and that the MRI may be operating only in the disk's corona as its ionization fraction is sufficient to merit an MHD description there rather than near the disk midplane (see Balbus & Henri 2008, and references therein). Thus, the fate of the MRI in disk environments, in which the magnetic Prandtl number is characteristically small, remains to be settled.
It is not clear why turbulent transport appears to vanish in numerical experiments when weakens. One possibility may be that under those conditions the MRI cannot grow sufficiently to excite a secondary transition that would, in turn, open the way to a turbulent cascade. Theoretical considerations of the MRI for restrictive configurations like laboratory experiments with cylindrical geometry predict that a low sheared fluid undergoing the MRI settles onto a pattern state whose momentum transport scales as () where  in other words, saturation of the instability is sensitive to the microscopic viscosity of the fluid. This counterintuitive result is rationalized by noting that a weak fluid viscosity means that it takes very little effort to readjust the underlying flow profile and establish a new shear in which the instability cannot operate. The stronger the viscosity, then, it becomes more difficult for the fluid to shut off the shear and the instability may operate unabatedly during the fluid's nonlinear development and eventual cascade to turbulence via secondary instabilities (e.g. parasitic instabilities, Xu & Goodman 1994).
In the idealized quasilinear study of Knobloch & Julien (2006) it was shown that in the limit of very large hydrodynamic and magnetic Reynolds numbers (i.e. Re 1 and Re 1 respectively) the azimuthal velocity profile tips over to shut off the instability by establishing a new velocity profile which reduces the shear throughout the domain. Their analysis shows that in the limits where Re and Re the resulting net velocity profile tends toward zero shear. Examinations of the thingap TaylorCouette system in the low limit (Umurhan et al. 2007a,b) show that once the system reaches saturation, the resulting velocity field within large midportions of the experimental domain is characterized by weakened shear. However these regions, where the tendency toward instability is reduced, are sandwiched by regions of strengthened shear, where the tendency toward instability is enhanced. Nonetheless, the aggregate configuration results in a profile that is stable against the MRI or any secondary instability and the system settles onto nonturbulent pattern state. Equally relevant is that in this pattern state the amplitudes of all fluid quantities, except the modified shear, scale as some power of . By comparison the modification of the shear is an order 1 quantity. Thus, in the limit where becomes very small only the modification to the background shear appears as a noticeable response in the idealized studies of the laboratory setup.
Because resolved shearing box numerical experiments of high Re and low flows appropriate for cold astrophysical disks is currently out of reach, speculation at this stage is justifiable. In particular, what may be the effective azimuthal velocity profile of high Re and low disks (or their sections)? As Ebrahimi et al. (2009) recently note, quasilinear saturation of the shear profile might be an unreasonable expectation given that the strong gravity tends to restore the shear profile within disks. However, the theoretical results of the thingap TaylorCouette system and the quasilinear studies, together with the objection of Ebrahimi et al., point to a possible hybrid scenario: what if the velocity profile of a low disk is on average Keplerian but locally exhibits alternating zones of very weak (or no) shear and very strong shear? This hypothetical configuration of the azimuthal velocity profile, an example of which is depicted in Fig. 1, might very well be driven into place by the MRI under very low situations. The recent studies of Julien & Knobloch (2006) and Jamroz et al. (2008) argue for the relevance of this scenario.
This study is an examination of the axisymmetric linear stability of incompressible ideal magnetohydrodynamic disturbances in a shearing box threaded by a constant vertical magnetic field and characterized by a variety of mean velocity profiles, including an extreme instance of the one appearing in Fig. 1^{}. Such configurations might be representative of real astrophysical disks characterized by very small values of .
Guided by the low results of Knobloch & Julien (2005) and Umurhan et al. (2007a,b), the analysis undertaken in this study is inviscid. The only low effect that is included here is the possibility that the fundamental shear profile is significantly modified. This altered shear profile may be easily included into the equations of motion as any radially dependent barotropic steady shear profile is a permitted equilibrium flow solution of the small shearingbox equations.
The range of questions that figure prominently are: (i) what happens to the unstable mode leading to the MRI when there are departures of the steady shear from the background Keplerian state? (iii) How does the nature or existence of unstable modes depend upon the radial boundary conditions of the shearing box (e.g. whether it is open or periodic in the radial direction)? (ii) Can one infer a possible reason or explanation for why turbulence seems to vanish in numerical experiments of the shearing box when is small?
This work is organized as follows: in Sect. 2 the equations of motion are laid out and the framework within which the stability analysis is discussed. Section 3 develops the profiles for the steady state for given modifications of the background shear while in Section 4 the normal mode stability analysis is developed and the governing ODE is derived including a statement of the generalized Velikhov criterion (Velikhov 1959). Section 5 presents the results of the stability analysis for a variety of boundary conditions and shear profiles and their forms. The implications of the results are discussed in the final section.
Figure 1: Qualitative depiction of a hypothesized mean rotational velocity profile for a low magnetic Prandtl number disk suggested by Jamroz et al. (2008). The dashed line shows the usual Keplerian velocity profile describing a rotationally supported disk. The mean velocity profile resulting from the saturation of the MRI in the low limit is speculated to consist of alternating regions of low and high shear (black lines). The mean shear over the extent of the disk follows the general Keplerian profile. 

Open with DEXTER 
2 Equations of Motion
The small shearing box equations (SSB, Lesur & Longaretti 2007; Regev & Umurhan 2008) are adopted which are the incompressible incarnation of the usual shearing box equations (Goldreich & LyndenBell 1965).
Their usage is justified as compressibility is an inessential feature
for the MRI. The box is moving in a rotating frame moving with the
local Keplerian velocity
^{}. The length scales of the box are measured by a size
which is much smaller than the radial scale of the disk .
On these scales, the background Keplerian shear appears as a linear
Couette flow profile. Time units are scaled by the local rotation time
of the disk
,
as measured at the fiducial radius ,
implying that the velocities of interest are scaled by
.
Given this, the disparity of the ratio of the
local disk soundspeed to the Keplerian speed (since the gas is relatively cold), and the assumption that the scale
is much less than the vertical scale height of the disk, the flow dynamics
have the character of incompressible rotating magnetic Couette flow. Magnetic fields are
scaled by a reference field scale
and the density is .
These quantities form a velocity defined to be the Alfven speed via
.
Furthermore the Cowling number is defined
which may be considered as related to the inversesquare of the ``parameter'' of plasma physics. This is not to be confused with the parameter used later on in this work to designate radial wavenumbers. The nondimensionalized SSB equations of motion are
in which is the velocity vector, p is the pressure, is the constant density (which is 1 in these units). is the local rotation rate but in the units used here it is also 1. The parameter q_{0} defines the amplitude of the local Keplerian shear and is formally given by
which is equal to 3/2 for rotationally supported Keplerian disks. This is the value assumed for q_{0} throughout the remainder of this work. The magnetic field is given by the vector and the current and is governed by Ampere's Law^{}.
3 Steady state
It is assumed that the fluid is of constant density
and the fluid is threaded uniformly throughout by a constant vertical magnetic field, i.e.
.
The current source of this background field is taken to be external to
the domain. As stated in the Introduction the steady velocity
field that represent departures to the Keplerian shear are taken as
given and represented by U(x). The total mean velocity is written as V(x) which is the sum of the Keplerian portion
and the departures U. Thus the steady state configuration requires satisfying the radial momentum balance which becomes
(5) 
in which the total mechanical and magnetic pressure is given by
where p_{0} is the steady state mechanical pressure field. For the model analyzed here where B_{z} is constant, the steady pressure field p_{0} is related to the azimuthal velocity departures by
The above expression represents a radially geostrophic state. Note that the solutions to p_{0} are smooth and well behaved so long as is continuous across the domain. In the axisymmetric linear stability analysis that follows only the steady state total vorticity field, denoted by q, plays a role and it is defined as
q = q_{0} + Q,  (7) 
where . A variety of functional forms for Q will be examined. The only restriction on Q will be that its domain integral is bounded, i.e.,
where symbolizes the domain under consideration. In many cases this integral will be zero.
4 Linear theory
Axisymmetric infinitesimal disturbances about the steady state shaped by q(x) are introduced into the governing equations of motion (14) revealing,
in which u',v' w' and p' denote perturbations in the radial, azimuthal vertical velocities and pressures, respectively, while b'_{x,y,z} represent perturbations in the magnetic field components. It should be recalled that q(x) is unspecified at this stage. However the existence of a steady state is assumed for a given reasonable q(x) profile. Normal mode perturbations are assumed which are periodic in the vertical direction. A perturbation variable f'(x,z,t) is thus expressed via the ansatz where is the temporal response while k is the vertical wavenumber. The incompressibility condition (11) means that a streamfunction may be defined such that,
Similarly the expression (12) and (14) allow for the definition of a flux function in which the radial and vertical components of the perturbed magnetic field are expressed via and .
Utilizing these definitions, the linearized perturbation equations are
reduced to a single one for the streamfunction (wherein and henceforth
the primes are dropped),
in which
where is the Alfven frequency and the spatially dependent epicyclic frequency is defined by . For later usage is rewritten in the alternate form,
The solutions to this system is governed by several parameters including the vertical wavenumber k, the Cowling number, , the radial size of the domain (appearing below) L and the form and amplitude of the deviation shear profile Q. Taken as a representation of a small disk section it is assumed that there exists a minimum vertical wavenumber k_{0} for disturbances since it is not reasonable to consider fundamental disturbances whose vertical extent is much larger than the disk height itself (Curry et al. 1994, and see discussion).
Before proceeding to these results it is important to keep in mind a number of matters. First, Knobloch (1992) showed that for vertical field configurations like that considered here, together with boundary conditions in which individual disturbances or their combinations are zero on the boundaries, the character of the normal mode response of the MRI is that is either real (growing/decaying exponential modes) or imaginary (oscillating modes), but never complex^{}. A version of the argument leading to this conclusion is given in Appendix A. Thus when the character of the fluid response is analyzed, will be taken as Reals. The relevance of this observation is that as a function of the system's parameters, a mode becomes unstable by passing through , sometimes known as exchange of stabilities (Chandrasekhar 1961). As such, in some instances the stability analysis of this system will focus on identifying which mode becomes marginal (i.e. ) and under which parameter conditions.
Secondly, the very same integral argument developed in Appendix A
also leads to a general statement about the relationship between the
temporal response and the structure of the modes in the domain,
is like an average radial wavenumber of the disturbance,
and, evidentally, is always greater than zero. represents the mode weighted average shear over the domain
One immediate consequence of this is that if (i.e. the mode weighted average shear over the domain is zero), then there is no possibility of instability. This follows from evaluating the criterion for marginality in (18), setting to zero and revealing
(21) 
The above expression cannot be satisfied if is zero. In general this relationship is not useful for direct calculations as the quantities therein depend implicitly upon the eigenvalue . However, it will be called upon to aid in interpreting the results that are obtained from specific direct calculations in Sect. 6.
5 Results
5.1 Classical MRI modes and channel solutions: a review
The classical system is recovered for Q=0. This means that
is independent of x and
Solutions of (15) are sought on a periodic domain L and are given in general by
(23) 
where A and are constants set by the boundary conditions of the system. The periodicity condition that = then means that
(24) 
which has the solution where n is any integer including zero. This condition recovers the incompressible limit of the classical dispersion relationship of the ideal case (e.g. Acheson & Hide 1973; Balbus & Hawley 1991) where specifically,
in which is the epicyclic frequency and where the radial wavenumber is
The solutions for the temporal response, written in terms of respected pairs, is given by
The solutions associated with the ``'' branch are termed the hydrodynamic inertial (HI) modes while those associated with the ``+'' are the hydromagnetic inertial (HMI) modes (viz. Acheson & Hide 1973). For a given mode n, the magnetorotational instability occurs for the latter of these provided that and
The background field must be sufficiently weak for the HMImodes to be unstable.
For given values of
the absolute minimum criterion required for instability to set in (i.e. for the mere possibility of
)
is when n=0, i.e.
,
and the condition in (27) predicts this to happen if,
(Velikhov 1959; Acheson & Hide 1973). This particular special mode, in which its radial structure is uniform, is generally referred to in the literature as the channel mode which describes purely 2D flow with no vertical velocity. The temporal response in this case is given by in which,
When unstable (for the HMImode branch) this radially uniform mode plays the central role in the development of MRI induced turbulence in numerical experiments. If 2q_{0} > 0, then the expression for is
The combination expression (which shall appear on a number of occasions in the following discussion) is always positive for HMI modes and is always negative for the HM modes since the expression inside the squareroot operation is always positive.
It should be noted that for Q=0 there are no localized normal modes possible for a domain which is infinite in extent. Put in another way, there is no solution of (15) for modes on an infinite domain with both (a) all quantities going to zero as and (b) is constant as given in (22).
5.2 Weak shear variations on a finite domain: 0 < Q 1
In this section weak shear variations are considered whose average are zero on the domain L. Before proceeding a caveat ought to be stated. Despite the spatially periodic nature of the shear Q, the analysis necessary to determine the temporal response uses a multiple timescale analysis. When periodic boundary conditions are imposed, as they are in Sect. 5.2.3, the multiple timescale analysis is akin to a Floquet analysis. In this instance a longtime scale behavior (in the form of correspondingly weak corrections to the temporal response ) must be invoked in order to ensure that the resulting perturbation solutions remain periodic on the length scale L. For boundary conditions other than periodic ones (Sects. 5.2.1 and 5.2.2), the multipletime scale analysis employed is a generic procedure involving perturbation series expansions and imposition of solvability conditions at successive perturbation orders (Bender & Orszag 1999). The role of the solvability conditions is to make sure that higher order perturbation solutions satisfy the boundary conditions of the system.
The shear with zero average on the domain of length L may be decomposed into the Fourier series expansion
where the parameter measures the overall severity of the shear. q_{n} measures the Fourier amplitude of the shear component n and is treated hereafter as a tunable parameter. Reference to (6) indicates that this form for Q ensures that the deviation steady velocity U and, hence, the radial pressure gradients are zero at the boundaries . The governing equation, with Q as given above, is expressed as
(32) 
Solutions of this are developed in a singular perturbation series expansion in powers of . Thus the ansatz,
(33) 
Given the definition of given in (22) it follows that and
(34) 
wherein
(35) 
The possibility that must be allowed (see below) This is why the next order term is also included in the expansion. With these expansions in mind (15) is written out for each power of . To lowest order
and to order
The order form is relegated until later. Solutions to (36, 37) are developed in the following subsections for various boundary conditions and restrictions at .
5.2.1 Channel conditions
Channel conditions require that the perturbed radial velocity is zero at the boundaries .
This, in turn, amounts to requiring that
at these positions, or in terms of the perturbation variables
The lowest order solution is given by
and where . The general solution for is written out as a sum of the linearly independent solutions . The index m ought not be confused with the index n which refers to the Fourier component of the shear profile Q appearing in (31). Stability, on the other hand, is evaluated by examining each individual eigenmode m. Thus all eigenvalues (and their perturbative corrections) will be identified according to which eigenmode under examination, e.g. etc. Note also that here the index m does not include m=0 as this would correspond to the trivial state .
Given the functional form of
found in (22), these relationships imply that
is equal to the functional form
found in (26) except with
replaced by ,
i.e.
.
The stability of these modes is now a function of the mode number m and, henceforth, the summation sign in (38) will be dropped and it shall be henceforth understood that when reference is made to ,
a particular eigenmode mode m
will be analyzed. At the next order it can be seen that in order
to have solutions that satisfy the boundary condition that
at the two endpoints, the terms on the RHS of (37)
must satisfy a particular solvability condition which will relate the correction
to the variation Q_{1}. This is seen by multiplying (37) by
given in (38) and integrating the result across the domain from L/2 to L/2^{}. In a general sense, then, one finds,
(39) 
in which the bracket notation is
(40) 
It follows that
in which
The denominator term of never crosses zero for physically relevant values of the parameters so that .
For illustration consider the m=1 mode (which is also the most unstable one) near marginality in the limit where kL is very large. In order for
to be nearly zero it must be that
,
cf. (28). It follows that the correction for this mode,
, is given approximately by the solution to
(42) 
where the last equality is established because the marginal mode, is under examination. The introduction of this profile pattern stabilizes this otherwise marginal mode if q_{1} < 0 and destabilizes it when q_{1} > 0. The corresponding shear profile for this example is depicted in Fig. 2. It can be seen that the modified shear is stabilizing when the shear is positive near the boundaries and negative in the interior.
Figure 2: The n=1 component of the shear profile (31). The solid line q_{1} = 1 and the dashed line q_{1} = 1. For problems in which channel wall conditions are imposed the solid line corresponds to a stable deviation profile while the dashed line corresponds to an unstable profile. The situation is reversed when fixedpressure boundary conditions are imposed. 

Open with DEXTER 
5.2.2 Pressure conditions
An analysis of (10) and (14) shows that the total magnetic plus mechanical pressure perturbations are proportional to the radial gradient of i.e.,
(43) 
Fixing the total pressure at the boundary in a Lagrangian sense (Curry et al. 1994) is equivalent to setting to zero the above expression at which, in the present case, means setting at those locations^{}. The solution is then given by
which is very similar in form to (38) except that the solution in the domain is composed of even functions and the series includes the mode with m=0, which is the classical channel mode. The correction to the temporal response for all values of is
which is the negative of the solution found in (41). As Fig. 2 indicates, this result says that shear profiles in a channel configuration that promote stability (instability) play a destabilizing (stabilizing) role for configurations with fixedpressure boundary conditions.
However the m=0 mode is a special case which requires a separate analysis. In its simplest guise, the channel mode is a constant with respect to x. Because of the periodicity of Q_{1} it means that = 0 and the analysis advanced up until this point to evaluate the correction shows that it will be zero at this order. Thus given this and the fact that the solution must be expanded according to,
(46) 
(47) 
where , i.e. the temporal response of the channel mode, is given in (29). The equations for the solution of are in successive order given by
The first of these says that the lowest order solution which satisfies the boundary condition is a constant . The next order down the solution is
where
=  
(52) 
In other words the solution is such that which satisfies the boundary condition . In order to generate a bounded solution for a solvability condition must be applied to the RHS of (50), which is obtained by reexpressing in terms of its solution as given in (51) and then integrating the equation from across the domain and setting the result to zero:
However, given the relationship between and Q_{1} it follows after an integration by parts that in fact,
(53) 
Given that for HMI modes
the above solvability condition says something remarkable: that the channel mode is always destabilized no matter what Q_{1} happens to be. By contrast, values of q_{n} may be chosen so that each eigenmode of the system with nontrivial radial structure (i.e. m>0) may be stably influenced by the shear Q_{1}, yet, there is no such configuration of the disturbed shear flow that can act to stabilize a channel mode. This result, above all others, emphasizes the important uniqueness of these modes. Also worth noting is that while the corrections to the growth rates of all modes (except m=0) is proportional to , the corresponding growth rate correction for the channel mode scales as : which means that though the channel mode is consistently destabilized by any periodic shear profile, its influence is markedly weaker.
5.2.3 Periodic conditions
Solutions of
that are periodic on the domain L are given by
where and is an arbitrary phase. The temporal response is given by , as defined in (26). As in the previous section, if attention is first given to those modes where , then one finds that
As in the previous section, the correction for the channel mode (m=0) is zero and the first nontrivial temporal response comes at order . The procedure is exactly the same as found in Sect. 5.2.2 and its correction is
(56) 
with
(57) 
Imposing periodic boundary conditions also implies that there are values of the coefficients of the perturbed shear Q_{1} which can be chosen to promote stability for all the modes of the system except for the channel mode. For example, for the m=1 mode and given its relative phase one can choose q_{2} so that the RHS of (55) is negative. This can be done for all other modes of the system as well except for the m=0 channel mode, which is destabilized no matter what choice is made for the parameters of Q_{1}, i.e. the set q_{n}.
5.3 Single shear defect on an infinite domain: localized disturbances
A profile with a single shear defect located at x=0 is represented by the deltafunction profile
The corresponding departures from the mean Keplerian shear profile U is given by
(59) 
If represents the solution of (15) respectively for x>0 and x<0, then solutions which decay as are
where is as given in (22) and provided that . If the latter condition is not met, then there are no localized normal modes allowed. The coefficients of the streamfunctions in both regions are equal in order that they be continuous across x=0, thus A_{+} = A_{} = A. Integrating (15) in an infinitesimal region around x=0, and given the defect (58), imposes a jump condition for the derivatives of approaching either side of the defect,
Putting in the solutions for the respective domains gives the quantization criterion
Solutions of the above equation are constrained to two possibilities: (i) if Q_{0} < 0, then for a normal mode solution to exist while (ii) if Q_{0} > 0, then it must be that for there to be a normal mode. The first of these cases says that normal modes are allowed only for those values of which are negative which are associated with the HI modes. The second of these cases are associated with the HMI modes of which the MRI is a possibility. Thus it is an interesting result that the MRI is a permitted localized normal mode disturbance only if the shear defect is positive. If the shear defect is negative (so that there is an effective reduction of the shear inside the region), then there are no normal modes predicted.
The solution of (62) is obtained by first taking the square of both sides of (62) yielding,
However one must be careful in interpreting the solutions of this simplified equation. Naively solving (63) will yield twice as many solutions than are allowed. This overcounting is corrected by requiring that only those solutions of (63) that satisfy
are permitted or else (62) cannot be satisfied. Solutions of (62) are,
Because the term inside the radical sign is always greater than zero for q_{0}>0, the ``+'' branch of the above expression is always greater than zero while the ``'' branch is always less than zero. Thus the ``+'' branch is the permitted solution for Q_{0}>0 while the ``'' branch is the allowed one for Q_{0}<0. Incorporating this formally yields the expression
Rewriting the terms appearing in the interior of the radical sign leads to finally,
which is similar in content to the classical channel mode dispersion relation (29) except for the fact that at any one time there exists only one branch of modes as a possible normal mode solution. The MRI mode only manifests as a normal mode when Q_{0} > 0 and its growth rate is enhanced by the defect.
5.4 Symmetric shear step on an infinite domain: localized disturbances
A finite version of the shear profile evaluated in the previous section is,
This profile for Q has a tophat structure and this descriptor will be used interchangeably with the expression symmetric shear step. Evidentally the value of the integral, , is the same for both forms of Q given in (58) and (65). Solutions to (15) must be developed separately in the three regions and appropriately matched across the boundaries separating the regions. Because Q is bounded it will suffice to match both the streamfunctions and their first derivatives across the domain. Thus, for x<L/2 and x>L/2 (15) is
(66) 
The solutions in the region where x<L/2 is given by
(67) 
while for x>L/2
(68) 
together with the constraint that . In the region L/2 < x < L/2 (15) is
(69) 
which has the two linearly independent solutions^{}
in which
The functional form
in which
(73) 
is introduced in order to make the following discussion more transparent. The designation references the HMI or HI modes respectively. It is also worth noting that given the constraint that must be real, that there is an absolute maximum value allowed for and this is dictated by the requirement that the terms subject to the square root operator must remain greater than zero or else the value of will turn out complex. In other words, given the reality of one does not expect solutions of to exceed where
(74) 
In all of the numerical solutions calculated below it is found that, indeed, all the solutions determined satisfy .
Imposing the conditions that the streamfunction and its first derivative match across the two boundaries
reveals that normal mode solutions exist provided the following condition is satisfied
(75) 
The terms in the first bracket represent a quantization condition for oddparity modes, which is to say that in the dimpled region , while the second represents evenparity modes where similarly in the same region.
Attention is first given to the evenparity mode in which the quantization condition,
must be satisfied for some value of . If were real and greater than zero, then the LHS of the above relationship is always positive. Since is real and positive, if the modes are to be localized, then the RHS of this expression is always less than zero. In this case it means that no solution exists for real. On the other hand solutions do exist if . Rewriting then the quantization condition above becomes
now with the constraint for the existence of localized normal modes is reexpressed as
The strategy for obtaining a solution is as follows: find the values of which solve (76), subject to the constraint given in (77), and then given the solution find through the relationship (72). The same procedure will be implemented for the evenparity solution below as well. Solutions of the quantization condition will be sought graphically in the range of values for . Inspection shows that the constraint (77) is violated if Q_{0} < 0 and , or if Q_{0} > 0 and . Since it means that there are no HMI normal modes as allowable solutions if Q_{0} < 0. HI normal modes are associated with the branch of solutions and since this is less than zero except for very special circumstances, one can generally expect HI normal modes for Q_{0} < 0 and for them to be stable. The aforementioned special circumstance occurs if there are solutions to (76) in which since, in that case, and HI modes may exist as well for Q_{0} > 0.
The evenparity mode limits to the singledefect configuration discussed in Sect. 5.3 for small values of the parameter L. Analysis of (76) in this limit shows that,
which, after restoring the definition of and some rearranging, becomes
where the definition of has been restored. For values of Q_{0} such that the above expression reduces to
which is the quantization condition for the singledefect problem on the infinite domain, (62). The range of values for Q_{0} and L for which this limiting form agrees with the actual result of the quantization condition is shown in Fig. 3, where is set to the value in order to compare the temporal response against conditions in which the channel mode is marginal in the classical theory, see (28). The main result is that the temporal response of the defect profile of the previous section closely resembles the temporal response of this step profile here in the limit where kL is small less than one. The limiting form represented by the defect profile becomes a poor representation of the tophat profile when kL exceeds order 1 values, however, the agreement tends to be much better for the HI.
Figure 3: The temporal response resulting from the quantization condition (76) as a function of kL (solid line) compared to the quantization condition (62) for defect profile (dashed line). For both plots with q_{0} = 3/2. a) For Q_{0} > 0 only HMI normal modes are permitted. The agreement between the two profiles severely breaks down for kL exceeding 2. b) For Q_{0} < 0 only HI normal modes are allowed. The agreement between defect theory and step profile is better for HI modes. 

Open with DEXTER 
Additionally, for small values of kL there is always at least one normal mode expected, whether it be the HI or HMI mode. However, as the horizontal length of the symmetric step profile increases, the number of permitted normal modes increases as well (Fig. 4). Similar behavior is predicted for modes which are localized in the vertical direction of the disk (Liverts & Mond 2009). As the number of permitted normal modes increases their values will cluster (countably as ) around the maximum value
(78) 
Oddparity modes are interesting since they have no analogues in the single defect profile studied in the previous section. Examining the quantization condition for it,
shows that there are no real solutions of that satisfy the constraint. Utilizing the expression , as used previously, the quantization condition takes the form
Inspection of the condition (79) shows that for there to exist a normal mode must be greater than as the functional form is positive for values of . This places a constraint upon the minimum value of L that permits this mode to exist and this is obtained by solving
(80) 
and, using the definition for found in (71) one finds that the minimum value for L must satisfy,
Note that the inclusion of the expression reflects how HMI/HI modes associate with the sign of Q_{0} so that the expression appearing above encapsulates both possibilities. Oddparity modes bifurcate into existence for as Q_{0} grows from zero and therefore it means that these modes are not expected to play a role for values of the defect which are small as this would entail very large values of the tophat region. The temporal response of these oddparity modes are otherwise similar in most every respect to their evenparity counterparts and, as such, no further analysis of their properties is pursued here.
Figure 4: Plot showing the increase of allowed normal modes with domain size L. In all plots , q_{0} = 3/2 and Q_{0} = 0.6 (HMI mode permitted). The dashed line is and solid line is . Panel a): corresponds to one normal mode at . Panel b): supporting four normal modes . All modes correspond to values of . . 

Open with DEXTER 
It should be noted that as in the previous section unstable localized MRI normal modes (HMImodes) can exist only if the step function in the shear is greater than zero. If the step is negative (indicating a region of weakened shear), then there are no HMI types of localized normal modes admitted by the configuration and, hence, there is no possibility of normal mode unstable disturbances.
5.5 Single shear defect on a periodic domain
Next a shear defect of the form
(82) 
is considered on the periodic domain . This form is very similar to the one considered in Sect. 5.3 except the integral of the shear over the periodic domain is zero, i.e. . The effects of shear defects with zero mean may be examined. The governing equation for is
where is given by
(84) 
Similar to what was done in the previous sections, one may express in terms of via the expression and, for the sake of completeness, this is written out explicitly,
in which the shear modified epicyclic frequency is defined as . Solutions to (83) must be developed separately for either side of x=0 and matched. Solutions for the streamfunction in which and (i.e. that they are periodic) are given by
where is the solution for the region . Continuity of the stream function is ensured by construction of the form of the solution in (86). The streamfunction must show a jump in its first derivative following the same arguments found in Sect. 5.3. Integrating (83) in a small region around x=0 results in the same condition for the jump in found in (61). Putting in the forms for found in (86) leads to the quantization condition
It should be kept in mind that the quantities as appearing on the RHS of (87) are different functions of depending upon whether one is considering HMI/HI () modes, respectively. Thus when solutions of the quantization condition are sought, separate attention will be given depending upon which type of mode is of interest. Furthermore, consideration of the solutions to (87) must be done by restricting attention to cases where is either real or imaginary. Additionally from previous arguments showing that must be real, there will be a maximum real value possible for
(88) 
Values of which are greater that would lead to complex values of as an inspection of (85) shows that if does exceed this maximum value, then the term inside the squareroot operator becomes negative which would lead to a complex value of . This restriction upon the value of helps in finding solutions for it.
The limit where recovers the classical limits discussed in Sect. 5.1. In that case channel modes, i.e. those modes for which , are the most unstable. In the current setting this corresponds to when Q_{0} = 0. Additionally, for the channel mode is exactly marginal for Q_{0} = 0, viz. the arguments leading to (28). This value for will be assumed so that a controlled analysis may be carried out in which one can track how varying Q_{0} affects the stability characteristics of an otherwise marginal channel mode.
Figures 5, 6 show the graphical solutions of (87) with some details of the results. The main result is that the mode that is identified with the classical channel mode in the ideal limit always exhibits exponential temporal growth no matter what amplitude the shear defect takes. Figure 7 shows that the temporal response of the classical channel mode is maximal for Q_{0} = 0 and that as Q_{0} moves away from zero instability is predicted. The mode exhibits an exponentially decaying spatial character ( ) for Q_{0} > 0, while it is weakly oscillatory ( ) for Q_{0} < 0. This general trend persists for a wide range of kL values. As such, the results depicted in these figures can be taken to be qualitatively representative. The figures also indicate that the unstable HMI mode can also turn into an unstable HI mode if the amplitude of Q_{0} becomes large enough.
Figure 5: Graphical solutions for the quantization condition (87). Attention restricted to real values of marking the mode which becomes the classical channel mode in the limit . Each panel depicts the three functions (thick line), and (dashed/thin lines). In all plots and . Panels a) and b) show that HMI modes are admitted as the solid curve crosses the line while for the latter two it crosses the line corresponding to meaning that HI modes are selected. The solution and temporal response for each: a) Q_{0} = 0.1, , , b) Q_{0} = 0.5, , , c) Q_{0} = 2.0, , and d) Q_{0} = 3.5, , . Notice how the channel mode goes from being an unstable HMI mode to an unstable HI mode as Q_{0} is increased. 

Open with DEXTER 
Figure 6: Similar to Fig. 5 except negative values of Q_{0} are investigated. In all plots and and q_{0} = 3/2. Panel a): the left plot shows that the channel mode admitted is a stable HI mode with and . The right plot in panel a) shows the first two overtone modes. The first HMI mode is unstable with and while the next HI mode admitted has and . Note that in these cases is imaginary. Panel b): stable HMI mode with and . For the first two overtones, the HMI mode is unstable with and while for the HI mode, and . For all values of Q_{0} < 0 there is at least one unstable HMI mode with imaginary . 

Open with DEXTER 
5.6 Single shear defect on finite domain: channel boundary conditions
This section is concerned with the response of disturbances to a Q configuration that is exactly like that considered in Sect. 5.5, where the difference now is that the disturbances are set to zero at the boundaries
.
This is equivalent to enforcing zero normal velocity at the boundaries. Thence, in this case is
where just as in the previous section, is the solution for the region . Evaluating the jump condition at x=0 leads to an analogous quantization condition like that in (87), namely,
in which and and are exactly as they are found in Sect. 5.5. It can be seen here, as before, that there there are never real solutions of for HMI modes if Q_{0} < 0 and, likewise, no such solutions for HI modes if Q_{0} > 0.
Figure 7: Behavior of the classical channel mode as a function of defect amplitude Q_{0} for and , q_{0} = 3/2, corresponding to a marginal ( ) channel mode at Q_{0} = 0. Top panel depicts as a function of Q_{0} in which the classic channel mode has . Bottom panel shows the temporal response which predicts exponential growth/decay for all values . The channel mode goes from being a HMI mode to a HI mode at . 

Open with DEXTER 
In Fig. 8 the
stabilizing behavior of the shear defect on the HMI modes is
depicted for the most unstable mode of the system. The results from the
weak shear limit discussed in Sect. 5.2.1
are used as a reference point to help interpret the following.
From the classical theory discussed in that section it was established
that the most unstable normal mode allowed is the one in which m=1, in turn implying
.
Reference to (27) shows that this mode is marginally stable when
(This is obtained by replacing with in that expression.) The response of the modes for three different values of kL are depicted. With the above choice for all modes are marginal at Q_{0} = 0. For the range of parameters investigated and shown in the figure, must be imaginary in order for the quantization condition to be satisfied. Thus the values for are written as . Inspection of the results show that stability is promoted only for values of Q_{0} which are negative. The range of values of Q_{0} for which stability is predicted decreases for larger domain sizes, i.e. as L is made larger the window in Q_{0} for which disturbances are stable decreases. For those ranges in Q_{0} in which stability is predicted, e.g. for for with given in (91), the temporal response of the other overtones was checked and all were found to have .
Figure 8: The behavior of the first unstable (HMI) mode for the problem with channel walls (q_{0} = 3/2). The values of and the corresponding temporal response are given as a function of the defect amplitude Q_{0} for three values of the parameter kL. The top panel shows . The bottom panel shows the temporal response. The value of for each curve is set so that the temporal response is marginal at Q_{0} = 0  details of this is described in the text. The value of for Q_{0} = 0 are shown by the symbol in the top panel. 

Open with DEXTER 
6 Discussion
This study is devoted to examining the axisymmetric inviscid linear response of a shearing sheet environment threaded by a constant vertical magnetic field for an array of different shear profiles. The motivation for considering this setup are restated from the Introduction:
 1.
 Numerical experiments of low magnetic Prandtl number flows appropriate for cold disk environments are outside current computational reach.
 2.
 Current numerical experiments seem to show the trend that as is lowered so is the corresponding angular momentum transport. The reasons for this is not yet clear.
 3.
 Theoretical analysis of laboratory setups evaluating the response of the MRI subject to a vertical background field find that transport is reduced with . Furthermore this reduction emerges through the modification of the basic shear profile (e.g. TaylorCouette) inside the experimental cavity which, in turn, is driven into place by the MRI itself. The final condition is a stable pattern state.
 4.
 In the final pattern state reached by the model laboratory system the modified shear profile's amplitude is independent of . This is not true of the remaining fluid and magnetic quantities which scale as with typical values . As is made very small one would observe a fluid state characterized by a uniform background magnetic field and an azimuthal flow showing deviations from a Keplerian state.
 5.
 The main mode of instability and driver of turbulence in the numerical experiments of the shearing box is the channel mode which is a special response with no radial structure. This mode precipitates a secondary instability which is understood to lead to a turbulent cascade. There is no channel mode allowed in a setup appropriate for a laboratory experiment.
The main difference between the laboratory setup and numerical calculations of the shearing box are their respective boundary conditions. The numerical experiments adopt periodic boundary conditions while the calculations for the laboratory experiments require no normal flow conditions at an inner and outer radius and the former of these permits channel modes to come into play.
Thus, what has been done here is a simple model calculation in which a shearing box configuration with a constant background vertical magnetic field is tested for stability for a number of different shear profiles. The perspective taken is that if there exists a shear profile (say, whose average over some length scale is zero) that is stable to the MRI, then it would strongly suggest that low flow configurations might saturate the MRI by driving into place a new azimuthal flow profile which leads to saturation.
What is found here is something very interesting. For flow configurations in which nonormal flow conditions are imposed at both radial boundaries (Sects. 5.2.1 and 5.6) there exists a modification to the shear in which the most unstable MRI mode is stabilized. However, for flows in which periodic boundary conditions (Sects. 5.2.3 and 5.5) or fixed Lagrangian pressure conditions (Sect. 5.2.2) are imposed there are no modulations of the shear which shut off the instability. In these cases, all modifications of the shear (with zero mean on some radial length scale) seem to enhance instability of the channel mode. For example, if the given channel mode is marginally stable to exponential growth, then introduction of the modified shear, no matter what is its nonzero amplitude, seems to destabilize it as the results of Sects. 5.2.3 and 5.5 indicate.
This strongly implies that in those numerical experiments in which a shear is threaded by a constant vertical magnetic field, the shear modification/MRIstabilization process may only apply for those flow conditions in which there is no normal flow on either one or both radial boundaries of the system.
On the other hand, for a similar magnetized fluid configuration described by periodic boundaries which therefore permits channel modes to exist, modifications of the shear appears to further destabilize the channel mode. If one were to consider a flow configuration (e.g. the local Keplerian profile in a shearing box threaded by a constant background field) that admits an unstable channel mode, then there seems to be no modification of the shear with zero mean that would saturate the growth of the channel mode since all such modifications further enhances its destabilizing influence. The emergence of a pattern state leading to saturation like the one envisioned by the hypothesis would seem to be out of the question under these circumstances. Moreover this suggests that the tendency for angular momentum transport reduction with , as indicated by numerical experiments of the shearing box, is due to some other process or processes (which are not discussed here).
These issues deserve further investigation as the conclusions reached here were done so utilizing very simple functional forms for the shear profile Q. Namely, the analysis performed in the previous sections either assumed weak values of Q, in order to use singular perturbation theory techniques, or that Q is described by deltafunctions (see also below). Use of these functions, which greatly facilitate analysis, have offered some insights into the nature of the responses of these modes. Of course, further investigation would require considering more physically realizable profiles and to check the robustness of the results they yield against the ones offered by use of these more simplified forms. As such the results reached here can serve as guideposts for further enquiries along these lines.
In the following some reflections are presented on other issues pertaining to the implications of the calculations performed here.
6.1 On the use of deltafunctions
A comparison between the responses of a single deltafunction shear profile on an infinite domain (Sect. 5.3) and a tophat profile for Q (Sect. 5.4) show that the results of the two configurations are qualitatively similar. Although the symmetric step function allows for more normal modes to exist as its radial extent is increased  a feature which is missed if one uses the deltafunction prescription  the qualitative flavor of the response is captured by its use nevertheless.
Another deficiency found in using the defect prescription is that for the tophat profile studied in Sect. 5.4 there are both even and odd parity normal modes possible whereas only the evenparity mode is admitted in the defect model. The oddparity mode has no counterpart in the single defect model. It was also shown that the oddparity mode may exist if the radial domain of the symmetric shear step is large enough as (81) indicates that the minimum size of the domain required for this mode to exist has the proportionality . For small values of the defect amplitude the minimum size of the shear step required for this oddparity mode to exist is so large that one does not expect that this should play any physically relevant role in the dynamics if one is interested in the response to narrow regions of altered shear. It is with some confidence to suppose that it is reasonable to represent the dynamical response of slender regions of modified shear through the use of deltafunction defects and this is the motivation and justification for its use in Sects. 5.5 and 5.6.
6.2 Channel modes
In the small Q theory of Sect. 5.2, it was shown that channel modes exist for periodic boundary conditions and for conditions in which the total pressure perturbations are zero at the two boundaries. Conversely, if either one of the two boundaries force the velocity perturbation to be zero there, then there is no channel mode permitted as a normal mode solution. In light of the previous results it is important that the boundary conditions appropriate for disks be properly ascertained in order to assess and better understand how activity in them are driven.
Channel modes in the classical limit have no radial structure. In Sect. 5.5 the development of this mode was studied as a function of the defect amplitude Q_{0} and it is shown that though the channel mode develops some amount of radial structure, as evinced by the nonzero value of its wavenumber , its tendency to be unstable survives and is even enhanced. In Regev & Umurhan (2008) it was postulated that the channel mode might disappear as a natural mode of the system if some amount of radial symmetry breaking were introduced into the governing equations of motion, for instance, in the form of a radially varying shear profile. However, the results of this section show that the classical channel mode indeed persists in its existence despite the introduction of a shear profile which deviates from the background constant shear state with zero average over some length scale. These conclusions are consistent with similar results regarding the nature of the MRI in more global contexts (Curry et al. 1994).
6.3 On the existence and number of localized normal modes
In Sects. 5.3 and 5.4 the existence of localized modes was examined. Localization is understood in this case to correspond to modal disturbances which show exponential decay as the radial coordinate . Thus, by construction, incoming/outgoing waves are excluded from consideration^{}. The existence of localized normal modes depends on the relative sign of the shear defect/step profile Q_{0}: HMI modes exist if the shear in the defect/tophat region is stronger than the background (Q_{0} > 0) while HI modes exist if the shear is relatively weakened (Q_{0} < 0)^{}  summarized here as
Given that the former mode type leads to the MRI, it means that if the shear in the defect zone is weakened, then there are no localized normal modes which can go unstable as only hydroinertial modes are supported (which happen to be stable except for very extreme circumstances). Of course, as an initial value problem, it does not mean that there are no hydromagnetic inertial modes permitted but, instead, the mode probably has some type of algebraic temporal growth/decay associated with it which cannot be described by the usual normal mode approach. This needs to be further examined by studying the associated initialvalue problem. Similar features are known to exist for vertically localized MRI modes in disks (Liverts & Mond 2009) in which the response of the initial value problem can exhibit exponential growth with an amplitude supporting some algebraic timedependence. Growth can initially be very small and it can take a very long time for a given disturbance to reach the same amplitude as expected for its counterpart normal mode. A conjecture is that the meaning of the absence of normal modes in the problem considered here may have similar attributes to the features associated with the initialvalue problem examined by Liverts & Mond (2009).
Irrespective of this outcome it should be remembered that the dichotomy observed here for modes on an infinite radial domain is a consequence of the imposition of exponential decay of the disturbances. This distinction disappears once waves are allowed to enter and exit from the ``infinite'' boundaries.
Lastly it is also noteworthy that for the localized problems considered here, when normal modes are permitted they usually come as a finite set. This is in contrast to other localized flow problems considered elsewhere in the literature. For example, in the problem of compact rotating magnetized jets in an infinite medium considered by Bodo et al. (1989) a countably infinite number of normalmodes are predicted for that system. This has some origin in the uniformity of both the rotation and magnetic field profiles of the jet considered in that study. By contrast, there are examples in geophysical flows in which the number of normal mode disturbances are discrete and finite. A recent example can be found in the work of Griffiths (2008) where the stability of inertial waves are studied in a stratified rotating flow with strong horizontal shear. For strongly peaked forms of the potential vorticity only a finite set of normal modes are predicted for the system. Such finiteness of the number of normal modes permitted is not so unusual in systems in which background states, like the shear or stratification, have strongly peaked functional forms like they are in the cases studied in this work.
6.4 Stabilization in general and an interpretive tool
The absolute minimum condition that must be met for any normal mode of the system to be unstable in a configuration with constant shear q_{0} is given by the Velikhov criterion (28): if the square of the Alfven frequency ( ) is greater than the shear by , then none of the HMI modes of the system can be unstable. For individual modes in the same system with some amount of radial structure the criterion is given by (27), where is the square of the radial wavenumber of the disturbance. As can be seen, for fixed values of there are two ways in which stability may be promoted  either by weakening the shear or by increasing the radial wavenumber. In the problem where the shear is constant, these quantities are set from the outset as parameters.
At the end of Sect. 4 there is a series of arguments for arbitrary
shear profiles which lead to the identity found in (18), which is like a generalized eigenvalue condition. This relationship
is the analog of the dispersion condition of the classical limit (uniform q) contained in (25)^{}. Care must be adopted before interpreting this expression as an eigenvalue condition since
appears implicitly in
the expressions for
and .
Nonetheless, a parallel analysis shows that stability is promoted if
where the effective wavenumber and shear , given in (19, 20) are,
is the domain and is the radial eigenmode of the disturbance in question. The stability condition for general q may be rationalized in the same way as the criterion is understood for the classical case with the replacements, and . With these aforementioned observations and caveats in mind, one may use (92) as an interpretive tool to aid in understanding the reasons for stability/instability in a particular problem. Thus, stability is promoted if (i) for fixed effective wavenumber, the effective shear is reduced or (ii) for fixed effective shear the effective wavenumber is increased, or in more general terms (iii) if the combination results in an overall reduction of the quotient
If one considers the results concerning the problem with periodic boundaries in Sect. 5.5, then the persistent instability expected for channel modes can be understood in terms of this criterion. In the classical limit where the defect amplitude is zero then for the channel mode is zero. As the defect amplitude is raised increases suggesting that this effect has a stabilizing influence, e.g. see Fig. 9. However, as the defect amplitude is raised away from zero the effective shear increases no matter what the sign of Q_{0} and, to effect, this increase always sufficiently overpowers the increase in so that the end result is further instability. In the same figure is plotted the quantity
(93) 
which, for the generalized Velikhov criterion, is a measure of the ratio of the destabilizing term for the shear profile q compared to its nominal value when the shear is only q_{0}: for one expects enhanced destabilization against the classical mode while for comes with enhanced stabilization. In Fig. 9 this quantity is plotted for one of the channel modes discussed in 5.5. Noting that in this case (i.e. that its radial wavenumber is zero in the ideal case) the radial profile of the mode develops as the amplitude of the shear defect increases no matter what its sign. The stabilizing rise in is accompanied by the destabilizing increase of the effective shear, that is to say , so that the quotient of their respective influences results in , indicating instability.
Similarly plotted in Fig. 10 is the influence Q_{0} has upon , , and the stability measure , for the single defect problem on a finite domain studied in Sect. 5.6. The presence of walls filters out the channel mode and the resulting flow potentially can support shear profiles which can stabilize the least stable mode. The Figure shows that within the range of (negative) values of the defect amplitude Q_{0} for which the mode does not exponentially grow/decay the effective shear is less than the background shear state only for part of the stable range. It means to say, then, in that range of parameter values in which the effective shear is greater than the background shear, yet there is still stability of the mode, stabilization is brought through an increased effective radial wavenumber which overcompensates the increased destabilization brought about by an increase in the effective shear.
Figure 9: The behavior of the unstable channel mode for the problem with periodic boundary conditions examined in Sect. 5.5: and with q_{0} = 3/2. Plotted is the temporal response, , together with its corresponding effective wavenumber and shear and ( plotted), and the stability measure for this mode . All values of the shear defect Q_{0} correspond to increasing the effective shear to above the background value . This increase in always overpowers the stabilizing influence of an increased . Note, the values of have been scaled by an arbitrary factor in order to facilitate clear comparison. 

Open with DEXTER 
Figure 10: The behavior of the least stable HMI mode for the problem with channel walls examined in Sect. 5.6: and with and q_{0} = 3/2. Plotted is the temporal response, , together with its corresponding effective wavenumber and shear and ( plotted), and the stability measure for this mode . Stability occurs for . In this window the effective shear is less than the background value ( ) for only part of this range, i.e. for . Stabilization in the range is achieved by a sufficient increase of the effective wavenumber so that the overall effect upon the stabilization parameter is for it to be less than one. has been similarly scaled as in the previous figure. 

Open with DEXTER 
6.5 Final reflections and an implication
The fundamental basis of this study is the assumption that in low magnetic Prandtl number flows for model environments like that considered in this study, the only noticeable outcome of the development of the MRI is to alter the basic shear profile. All other quantities, such as magnetic fields and the radial and vertical velocities, have saturated profiles which scale as some positive power of so that for their contributions become negligible. The basis of this assumed trend derives from the theoretical calculations of laboratory setups discussed in the Introduction. It is therefore assumed here that a similar trend may appear for configurations in shearing boxes with periodic radial boundary conditions as well. The perspective taken here with regards to those configurations is that if this is indeed the case, then one can (in principle) test the stability of a wide variety of shear profiles which show deviations (constrained to have a zero average over some length scale) from the basic Keplerian profile  configurations which are akin to those predicted from the calculations of laboratory setups. If a stability calculation shows that there exists a shear profile which is stable to these axisymmetric disturbances, then the shearmodification/modesaturation hypothesis should become a serious candidate explanation.
However, the calculations done in this study indicate that for periodic shearing box environments there is always an instability of the basic channel mode no matter what shear profile is assumed (satisfying the aforementioned constraints). Unlike the situation for laboratory setups, where saturation can be achieved by altering the basic shear profile, saturation (if present) in shearing box environments with periodic boundary conditions is likely not due to this mechanism.
This further implies that the nonlinear response of systems supporting the MRI stongly depends upon the boundary conditions employed which is not so surprising as many physical systems in Nature exhibit this sensitivity to their boundaries. Thus it seems to this author that some care must be taken before one equates the results of laboratory experiments to those physically related/analogous systems for which the experiments are meant to represent (cf. Ji et al. 2006). This cautionary note is not to diminish the value of one over the other, rather, it is intended to emphasize that there are many subtle and, at times, conflicting features between such systems that must be clearly understood before any firm conclusions are reached.
The author thanks Marek Abramowicz and the organizers of the Asymptotic Methods in Accretion Disk Theory workshop at CAMK (May/June 2009) where the impetus for this work originated. The author also thanks James Cho, Lancelot Kao, Olivier Gressel, Paola Rebusco, Edgar Knobloch and Oded Regev for their generous support and fruitful conversations during the course of this study.
Appendix A: Proof that is never complex
(15) is rewritten into the form
where . The nature of will be assessed by supposing that
where Reals. It will be shown below that b must be zero.
The boundary conditions on
are one of the following possibilities: (i)
goes to zero on the domain boundary
provided the latter is finite; (ii)
and its derivative go to zero on the domain boundary if the boundary tends to infinite distances; (iii)
is periodic on a length scale L in the domain .
Replacing
with a + ib in the equation for ,
followed by multiplication by the complex conjugate of
(i.e. ), integrating the result and applying the boundary conditions gives
where
I_{1}  =  
(A.2) 
and
(A.3) 
It must be that both I_{1} and I_{2} are zero if (A.1) is to be satisfied. Supposing that then the relationship implied by I_{2}=0, is that
This result used in the expression for I_{1} lead to
(A.4) 
However all the quantities in the above expression are always positive and, therefore, I_{1} can never be zero. Consequently b must be zero which, in turn, means that can only be real.
With b=0 and restoring the definition of a the equation I_{1} = 0 appears now as
0  =  
(A.5) 
Dividing the above expression by and utilizing the definition of given in (22) leads to the expressions appearing in (1820).
References
 Acheson, D. J., & Hide, R. 1973, Rep. Prog. Phys., 36, 159 [NASA ADS] [CrossRef] [Google Scholar]
 Balbus, S. A., & Hawley, J. F. 1991, ApJ, 376, 214 [NASA ADS] [CrossRef] [Google Scholar]
 Balbus, S. A., & Henri, P. 2008, ApJ, 674, 408 [NASA ADS] [CrossRef] [Google Scholar]
 Bender, C. M., & Orszag, O. 1999, Advanced Mathematical Methods for Scientists and Engineers (Springer) [Google Scholar]
 Bodo, G., Rosner, R., Ferrari, A., & Kobloch, E. 1989, ApJ, 341, 631 [NASA ADS] [CrossRef] [Google Scholar]
 Chandrasekhar, S. 1961, Hydrodynamic and Hydromagnetic Stability (Oxford) [Google Scholar]
 Curry, C., Pudritz, R. E., & Sutherland, P. G. 1994, ApJ, 434, 206 [NASA ADS] [CrossRef] [Google Scholar]
 Ebrahimi, F., Prager, S. C., & Schnack, D. D. 2009, ApJ, 698, 233 [NASA ADS] [CrossRef] [Google Scholar]
 Friedman, B. 1956, Principles and Techniques of Applied Mathematics (New York: Wiley) [Google Scholar]
 Fromang, S., Papaloizou, J., Lesur, G., & Heinemann, T. 2007, A&A, 476, 1123 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
 Goldreich, P., & LyndenBell, D. 1965, MNRAS, 130, 125 [NASA ADS] [CrossRef] [Google Scholar]
 Griffiths, S. D. 2008, J. Fluid Mech., 605, 115 [NASA ADS] [Google Scholar]
 Jamroz, B., Julien, K., & Knobloch, E. 2008, Astron. Nachr., 329, 675 [NASA ADS] [CrossRef] [Google Scholar]
 Ji, H., Burin, M., Schartman, E., & Goodman, J. 2006, Nature, 444, 343 [NASA ADS] [CrossRef] [PubMed] [Google Scholar]
 Julien, K., & Knobloch, E. 2006, in Stellar Fluid Dynamics and Numerical Simulations: From the Sun to Neutron Stars, ed. M. Rieutord, & B. Dubrulle, EAS Publ. Ser., 21, 81 [Google Scholar]
 Knobloch, E. 1992, MNRAS, 255, 25 [NASA ADS] [Google Scholar]
 Knobloch, E., & Julien, K. 2005, Phys. Fluids, 17, 094106/16 [NASA ADS] [CrossRef] [MathSciNet] [Google Scholar]
 Lesur, G., & Longaretti, P.Y. 2007, MNRAS, 378, 1471 [NASA ADS] [CrossRef] [Google Scholar]
 Liverts, E., & Mond, M. 2009, MNRAS, 392, 287 [NASA ADS] [CrossRef] [Google Scholar]
 Regev, O., & Umurhan, O. M. 2008, A&A, 481, 1 [NASA ADS] [CrossRef] [EDP Sciences] [Google Scholar]
 Umurhan, O. M., Regev, O., & Menou, K. 2007a, PRL, 98, 034501 [NASA ADS] [CrossRef] [PubMed] [Google Scholar]
 Umurhan, O. M., Menou, K., & Regev, O. 2007b, PRE, 76, 036310 [NASA ADS] [CrossRef] [Google Scholar]
 Velikhov, E. P. 1959, J. Exp. Theor. Phys. (USSR), 36, 995 [Google Scholar]
Footnotes
 ...
^{}  Extreme in the sense that regions of sharp shear are represented by deltafunctions in the analysis herein. See also discussion in Sect. 6.
 ...^{}
 Overbars over quantities refer to their dimensional values.
 ... Ampere's Law^{}
 Note that by its construction (3) contains the statement that the time evolution of the divergence of the magnetic field is zero. If initially everywhere, then it remains identically zero subsequently.
 ... complex^{}
 It was also shown in that study that complex values of can only occur if the field configuration is helical. In this case the instability is of a traveling wave.
 .../2^{}
 This procedure of applying a solvability condition actually requires multiplying across by the adjoint solution of . However since the eigenfunctions comprising and the linear operator of (36) are real and Hermitian, the adjoint is .
 ... locations^{}
 Note that this is valid since by construction the radial gradient of the steady state pressure field is zero at the end points.
 ... solutions^{}
 The second of the solutions appearing in (70) is written in the form displayed in order to make sure that both linearly independent solutions are represented even in the event (Friedman 1990).
 ... consideration^{}
 Given the mathematical structure of the ode describing axisymmetric disturbances, the radial eigenfunctions that are solutions have either strictly oscillatory or exponential radial profiles. Thus the possibility of decaying oscillations is ruled out.
 ... 0)^{}
 The mode existence dependency upon the sign of Q_{0} was checked for other shear profiles (for instance, by replacing the tophat with a truncated parabolic profile). Aside from differences in the magnitude of the temporal response and the multiplicity of modes allowed, the aformentioned sign dependency still holds.
 ...)^{}
 The classical limit is obtained when the replacements and are made.
All Figures
Figure 1: Qualitative depiction of a hypothesized mean rotational velocity profile for a low magnetic Prandtl number disk suggested by Jamroz et al. (2008). The dashed line shows the usual Keplerian velocity profile describing a rotationally supported disk. The mean velocity profile resulting from the saturation of the MRI in the low limit is speculated to consist of alternating regions of low and high shear (black lines). The mean shear over the extent of the disk follows the general Keplerian profile. 

Open with DEXTER  
In the text 
Figure 2: The n=1 component of the shear profile (31). The solid line q_{1} = 1 and the dashed line q_{1} = 1. For problems in which channel wall conditions are imposed the solid line corresponds to a stable deviation profile while the dashed line corresponds to an unstable profile. The situation is reversed when fixedpressure boundary conditions are imposed. 

Open with DEXTER  
In the text 
Figure 3: The temporal response resulting from the quantization condition (76) as a function of kL (solid line) compared to the quantization condition (62) for defect profile (dashed line). For both plots with q_{0} = 3/2. a) For Q_{0} > 0 only HMI normal modes are permitted. The agreement between the two profiles severely breaks down for kL exceeding 2. b) For Q_{0} < 0 only HI normal modes are allowed. The agreement between defect theory and step profile is better for HI modes. 

Open with DEXTER  
In the text 
Figure 4: Plot showing the increase of allowed normal modes with domain size L. In all plots , q_{0} = 3/2 and Q_{0} = 0.6 (HMI mode permitted). The dashed line is and solid line is . Panel a): corresponds to one normal mode at . Panel b): supporting four normal modes . All modes correspond to values of . . 

Open with DEXTER  
In the text 
Figure 5: Graphical solutions for the quantization condition (87). Attention restricted to real values of marking the mode which becomes the classical channel mode in the limit . Each panel depicts the three functions (thick line), and (dashed/thin lines). In all plots and . Panels a) and b) show that HMI modes are admitted as the solid curve crosses the line while for the latter two it crosses the line corresponding to meaning that HI modes are selected. The solution and temporal response for each: a) Q_{0} = 0.1, , , b) Q_{0} = 0.5, , , c) Q_{0} = 2.0, , and d) Q_{0} = 3.5, , . Notice how the channel mode goes from being an unstable HMI mode to an unstable HI mode as Q_{0} is increased. 

Open with DEXTER  
In the text 
Figure 6: Similar to Fig. 5 except negative values of Q_{0} are investigated. In all plots and and q_{0} = 3/2. Panel a): the left plot shows that the channel mode admitted is a stable HI mode with and . The right plot in panel a) shows the first two overtone modes. The first HMI mode is unstable with and while the next HI mode admitted has and . Note that in these cases is imaginary. Panel b): stable HMI mode with and . For the first two overtones, the HMI mode is unstable with and while for the HI mode, and . For all values of Q_{0} < 0 there is at least one unstable HMI mode with imaginary . 

Open with DEXTER  
In the text 
Figure 7: Behavior of the classical channel mode as a function of defect amplitude Q_{0} for and , q_{0} = 3/2, corresponding to a marginal ( ) channel mode at Q_{0} = 0. Top panel depicts as a function of Q_{0} in which the classic channel mode has . Bottom panel shows the temporal response which predicts exponential growth/decay for all values . The channel mode goes from being a HMI mode to a HI mode at . 

Open with DEXTER  
In the text 
Figure 8: The behavior of the first unstable (HMI) mode for the problem with channel walls (q_{0} = 3/2). The values of and the corresponding temporal response are given as a function of the defect amplitude Q_{0} for three values of the parameter kL. The top panel shows . The bottom panel shows the temporal response. The value of for each curve is set so that the temporal response is marginal at Q_{0} = 0  details of this is described in the text. The value of for Q_{0} = 0 are shown by the symbol in the top panel. 

Open with DEXTER  
In the text 
Figure 9: The behavior of the unstable channel mode for the problem with periodic boundary conditions examined in Sect. 5.5: and with q_{0} = 3/2. Plotted is the temporal response, , together with its corresponding effective wavenumber and shear and ( plotted), and the stability measure for this mode . All values of the shear defect Q_{0} correspond to increasing the effective shear to above the background value . This increase in always overpowers the stabilizing influence of an increased . Note, the values of have been scaled by an arbitrary factor in order to facilitate clear comparison. 

Open with DEXTER  
In the text 
Figure 10: The behavior of the least stable HMI mode for the problem with channel walls examined in Sect. 5.6: and with and q_{0} = 3/2. Plotted is the temporal response, , together with its corresponding effective wavenumber and shear and ( plotted), and the stability measure for this mode . Stability occurs for . In this window the effective shear is less than the background value ( ) for only part of this range, i.e. for . Stabilization in the range is achieved by a sufficient increase of the effective wavenumber so that the overall effect upon the stabilization parameter is for it to be less than one. has been similarly scaled as in the previous figure. 

Open with DEXTER  
In the text 
Copyright ESO 2010
Current usage metrics show cumulative count of Article Views (fulltext article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 4896 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.