Issue |
A&A
Volume 439, Number 1, August III 2005
|
|
---|---|---|
Page(s) | 351 - 359 | |
Section | The Sun | |
DOI | https://doi.org/10.1051/0004-6361:20042560 | |
Published online | 22 July 2005 |
Electron density along a coronal loop observed with CDS/SOHO
1
Armagh Observatory, College Hill, Armagh BT61 9DG, N. Ireland e-mail: iugarte@ssd5.nrl.navy.mil
2
Centre for Astrophysics, University of Central Lancashire, Preston, PR1 2HE, UK
3
Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Str. 2, 37191 Katlenburg-Lindau, Germany
4
Department of Solar Physics, Royal Observatory of Belgium, Av. Circulaire 3, 1180 Bruxelles, Belgium
Received:
17
December
2004
Accepted:
21
April
2005
The analysis of a coronal loop observed by CDS and EIT on board SOHO is presented.
The loop was situated above the North-East limb at a latitude of ~48°, being
clearly visible in the hottest lines of the dataset, Fe xvi 360.76 Å, i.e.
greater than 2 000 000 K. The cooler lines in the sample (i.e. O v 629.73 Å and
He i 584.35 Å) showed only a brightening at the footpoints location. Based on the
Fe xiv 353.84/334.17 line ratio, the electron density along the loop was determined
following three different approaches for the background subtraction. No differences, within the
error bars, can be found between the three methods. At the apex, the density is
cm-3, while at the footpoint it is 50% greater, i.e.
cm-3. The inferred filling factor values along the loop, at the formation temperature of
the lines, are in the range 0.2–0.9.
One dimensional hydrodynamic modelling of the loop along a given field line, gravity
neglected, was performed. A minimum
analysis results in a best fit case
where the total energy input is directed preferentially to the loop footpoint (the
heating rate is three times larger at the base than at the apex). An isochoric
solution can not be ruled out completely. The exercise illustrates the necessity
of accurate spectral diagnostics in order to derive definite conclusions from theoretical models
and suggests the need for simultaneous density and temperature diagnostics.
Key words: Sun: corona / plasmas / hydrodynamics
© ESO, 2005
Current usage metrics show cumulative count of Article Views (full-text 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 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.