Issue 
A&A
Volume 519, September 2010



Article Number  A39  
Number of page(s)  24  
Section  Interstellar and circumstellar matter  
DOI  https://doi.org/10.1051/00046361/200913906  
Published online  09 September 2010 
Online Material
Appendix A: Emission by an electric dipole in an infinite medium
We first study the electric field created by a single electric dipole, with dipole moment , in an infinite homogenous medium, and its decomposition into s and ppolarized components. The configuration is described by Fig. A.1 and many notations used are listed in Table A.1.Figure A.1: Coordinate system and angles used to calculate the decomposition of the electric field , created by an electrical dipole , into s and ppolarized components. 

Open with DEXTER 
Table A.1: Definition of axis, angles, and other notations.
The refractive index is complex if the medium j is absorbing. In the case of considering a nonabsorbing medium j, the imaginary part of the index, , is zero. The refractive index is given by the relation A.1, and the wave vector (in the direction of the observator) is linked to the complex refractive index by Eq. (A.2):
A.1 Polarization of the electric field
The electric field is perpendicular to the direction of observation and can be decomposed into two orthogonal components, i.e., two polarizations: the spolarized one is perpendicular to the observation plane and the (p)polarized one is in this plane:
With Eqs. (A.7) and (A.8), we find
A.2 Radiant intensity in an infinite medium
The next equations show how to obtain the intensity from the electric field amplitude. We can linked the electric field to the irradiance that is the incident power of electromagnetic radiation at a surface, per unit area.
where is the vacuum permittivity, c the speed of light in vacuum, and n the refractive index of the medium.
Radiant intensity (incident power per unit solid angle) I and irradiance created by the electric dipole are normalized as
where r is the radius of the sphere where the irradiance is calculated, and is the total^{} power emitted at the wavelength by a single dipole , in all directions of the space.
=  
=  (A.12) 
and 
The normalization Eq. (A.11) let us obtain factor F:
The radiant intensity emitted by one electric dipole , in the direction given by the angles (,), is given by the next equation (whatever the distance from source dipole since the medium is infinite, homogenous and not absorbing):
(A.13) 
Consider now a luminescent layer of thickness H, and thus an ensemble of incoherently radiating electric dipoles having equal dipole moment but randomly oriented. To take this random orientation of the dipoles into account, we have to average over the direction of , i.e., and . The intensity obtained is named :
The dipoles are located in the layer of thickness H; the total intensity emitted from this luminescent layer is thus obtained by integrating the product of with L_{z}(h), the linear density of the radiating dipoles (m^{1}), over the layer depth h. As the layer is formed by a homogenous medium, L_{z}(h) is constant with h:
Let us consider now an absorbing medium with an index that is thus complex. The following equations show the effect of propagation of an electromagnetic wave (wave vector ) on a length r in this medium of complex refractive index
 on the wave amplitude E:
E' = E' =
 on the wave intensity I:
I' I' =
Appendix B: Effects of the interfaces of the film
In this appendix, we introduce the effects of the interfaces of the film and calculate the emission amplitude in a medium 1 by summing all the transmitted components (of each polarization), taking the phase shift and absorption due to propagation in each medium into account. As a result, the radiation pattern are obtained: it is the angular distribution of the light emitted by the film into the halfspace 1.
Until now, we have considered an infinite medium. We now consider three different homogenous media (medium 0 is a film between semiinfinite media 1 and 2) and their interfaces. The emitting dipole is now located in the film 0. Our aim is to determine the radiation transmitted in medium 1 under the angle of observation .
We separate the light transmitted in medium 1 into two beams: the direct beam D is the one emitted directly in the direction of medium 1 (with an emission angle given by the angle of observation and the SnellDescartes relation of refraction). The reflected beam R is the beam that is first directed toward medium 2 and reflected off the interface 0/2 before being transmitted in medium 1. Each of these beams is reflected multiple times between each interface of the film 0. In this paragraph, we see that interference effects appear because of these multiple reflections and also because of the sum of the two different beams, D and R. This latter case of interference is known as the wideangle effect.
Figure B.1: Schematic diagram of the emission geometry for a dipole embedded in a thin film (medium 0), at a distance h from the surface, for an emission angle in medium 1. This emission is the combinaison of light from the direct beam D (red solid line) and from the reflected beam R (green dashed line). 

Open with DEXTER 
B.1 The direct beam D
We first consider the the direct beam D, with its multiple reflection back and forth in layer 0, transmitted in medium 1 as shown in Fig. B.2:
=  
=  (B.1)  
The following notations are used to lighten expressions.
Remark: is defined with a factor to obtain a power attenuation of .
absorption:  
phase shift:  
where and are the phase shift and the absorption due to only one wave back and forth in layer 0 before being transmitted in medium 1.
Hence, one derives
(B.2)  
Figure B.2: Schematic diagram of the emission geometry for the direct beam D. 

Open with DEXTER 
B.2 The reflected beam R
Figure B.3: Schematic diagram of the emission geometry of the reflected beam R. 

Open with DEXTER 
=  
=  
=  (B.3) 
B.3 Combination of the D and R beams
We calculated the expression of the electric field amplitude transmitted in medium 1 of the direct beam and of the reflected beam , for each polarization, (s) and (p). These amplitudes are exprimed as a function of and , which are the electric field amplitude emitted by an electric dipole in the direction and , respectively:
The Eqs. (A.9) and (A.10) give the influence of the angle on . One obtain
(B.4)  
(B.5)  
(B.6)  
To combine the electric fields in medium 1 due to the direct and reflected beams and , we have to pay attention to the direction of these vectors and not only to their amplitude,
Let us consider the direction of the vectors , , and in medium 0, before any reflection or transmission at the film interfaces. The Eqs. (A.3) and (A.4) show that
The reflection at the interface 0/2 of the reflected beam changes the sign of , so the direction of and become opposite. As one can see in Figs. B.1B.3, the direct and reflected beam transmitted in medium 1, and , respectively, are
 in the same direction for the spolarization
 in opposite direction for the ppolarization.
and: 
=  
=  (B.7) 
where and .
B.3.1 spolarized
(B.8)  
B.3.2 ppolarized
(B.9) 
and .
B.4 Radiation pattern
The radiation pattern is the angular distribution of the light emitted by the source
located in layer 0 into the halfspace 1, expressed by
the intensity (
)
emitted in the direction given the angles
into the halfspace 1.
=  
=  (B.10) 
=  
=  (B.11)  
where: .
B.4.1 Solid angle modification at the interface
The ratio
represents the modification of solid angle when the medium changes,
is the radiated power in medium i into the solid angle
.
When the wave goes through the interface i/j, the solid angle is modified and the power conservation is given by Eq. (B.12) (when the transmission coefficient is 1):
This is the origin of the factor in the expression of the intensity ,
(B.12) 
using the derivative of the SnellDescartes law.
B.4.2 Random orientation of the dipoles
To take a random orientation for the electric dipoles embedded in the film account, the intensity is averaged over and . The geometry is thus no more dependent on the angle ; I_{1} is now only depending on the angle of observation . , which is the total power emitted in all directions of the space, at the wavelength , by a single dipole at the depth h, does not vary with the direction of the dipole.
The intensity ( ) emitted by a film layer of thickness dh, at the film depth h, is
(B.13) 
=  
=  
=  (B.14) 
Finally, the specific radiant intensity in medium 1 and created by electric dipoles of random orientation at the film depth h is
where , and are expressed in the next section. The variable gives the influence of the multiplebeam interference, and is due to the wide angle interference.
B.4.3 Radiant intensity observed in medium 1
Until now, we have not being interested in the wavelength dependence of the emission. The observed intensity depends on
because each dipole radiates with a power
that depends on the wavelength through an emission profile
(in nm^{1})
proper to the material of the film. In the case of photoluminescence,
the emission of each dipole will also result in an excitation absorbed
by the film (
is the power absorbed in unit of length (W.m^{1})) that can depend on the film depth h. The emission also results in the photoluminescence yield
^{}.
The specific power emitted by unit of film length (W nm^{1} m^{1}) is
(B.16) 
The total power (W) between the wavelengths and , emitted by the film in all directions in space is
=  (B.17)  
=  (B.18) 
Moreover, because the whole film is radiating, the electric dipoles are located at all the film depths h between 0 and H, with a constant distribution on this interval. Thus, to obtain the specific radiant intensity that is observed in medium 1, we must integrate the expression given by the Eq. (B.15) on the interval [0,H]:
(B.19)  
(B.20) 
The total power between the wavelengths and , received on a detector D that ``sees'' an solid angle is
(B.21) 
Appendix C: Fresnel coefficients
In this appendix, we express the Fresnel coefficients for an absorbing medium (meaning with a complex refractive index).
C.1 Reflection
The Fresnel reflection coefficients are given by the equations:
(C.1) 
The angles are here complex angles given by the DescartesSnell law of refraction for absorbing media, i.e., with complex refractive indexes (Kovalenko 2001):
(C.2) 
The variables and are defined by .
C.2 Transmission
The Fresnel transmission coefficients (ratio of wave amplitudes) are given by the equations:
(C.3) 
(C.4) 
The Fresnel transmittances (ratio of powers) are given by the equations
=  (C.5) 
where A_{i,j} is the surface section of the light beam in medium i or j, and P_{i,j} and are the incident and transmitted power (in Watt) and the irradiance (in :
=  (C.6)  
=  (C.7) 
Remark: In the same way, the reflectance is also defined as
(C.8) 
We can also define another transmission factor that takes the modification of the solid angle due to refraction at the interface between media i and j into account:
=  (C.9)  
=  (C.10)  
=  (C.11) 
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.