Issue |
A&A
Volume 419, Number 3, June I 2004
|
|
---|---|---|
Page(s) | 1149 - 1158 | |
Section | The Sun | |
DOI | https://doi.org/10.1051/0004-6361:20041088-1 | |
Published online | 07 May 2004 |
Radiative hydrodynamic modeling of the Bastille-Day flare (14 July, 2000)
I. Numerical simulations
1
Joule Physics Laboratory, School of Computing, Science & Engineering, University of Salford, Salford M5 4WT, UK
2
Lockheed Martin, Advanced Technology Center Solar & Astrophysics Laboratory, Dept. L9-41, Bldg. 252 3251 Hanover Street, Palo Alto, CA 94304, USA
3
Physics Department, University of Warwick, Coventry CV4 7AL, UK
Corresponding author: D. Tsiklauri, D.Tsiklauri@salford.ac.uk
Received:
23
January
2004
Accepted:
26
February
2004
A 1D loop radiative hydrodynamic model that incorporates the effects of gravitational stratification, heat conduction, radiative losses, external
heat input, presence of helium, and Braginskii viscosity
is used to simulate elementary flare loops. The physical parameters
for the input are taken from observations of the Bastille-Day flare of 2000 July 14.
The present analysis shows that:
a) the obtained maximum values of the electron density
can be considerably higher (4.2 1011 cm-3 or more)
in the case of footpoint heating than in the case of apex
heating (2.5
1011 cm-3);
b) the average cooling time after the flare peak takes less time in the case of
footpoint heating than in the case of apex heating;
c) the peak apex temperatures are significantly lower
(by about 10 MK) for the case of footpoint heating than for apex heating
(for the same average loop temperature of about 30 MK).
This characteristic would allow to discriminate between different
heating positioning;
d) in both cases (of apex and footpoint heating),
the maximum obtained apex temperature
is practically independent of the heating duration
,
but scales directly with the heating rate
;
e) the maximum obtained densities at the loop apex,
, increase with the heating rate
and heating duration
for both footpoint and apex heating.
In Paper II we will use the outputs of these hydrodynamic simulations, which
cover a wide range of the parameter space of heating rates and durations,
as an input for forward-fitting of the multi-loop arcade of the
Bastille-day flare.
Key words: Sun: flares / Sun: activity / Sun: corona
© ESO, 2004
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