Marsh, M. S. and Walsh, Robert William
Using HINODE/Extreme-Ultraviolet Imaging Spectrometer to confirm a seismologically inferred coronal temperature.
The Astrophysical Journal, 706
Official URL: http://dx.doi.org/10.1088/0004-637X/706/1/L76
The Extreme-Ultraviolet Imaging Spectrometer on board the HINODE satellite is used to examine the loop system described in Marsh et al. (2009) by applying spectroscopic diagnostic methods. A simple isothermal mapping algorithm is applied to determine where the assumption of isothermal plasma may be valid, and the emission measure locii technique is used to determine the temperature profile along the base of the loop system. It is found that, along the base, the loop has a uniform temperature profile with a mean temperature of 0.89 +- 0.09 MK which is in agreement with the temperature determined seismologically in Marsh et al. (2009), using observations interpreted as the slow magnetoacoustic mode. The results further strengthen the slow mode interpretation, propagation at a uniform sound speed, and the analysis method applied in Marsh et al. (2009). It is found that it is not possible to discriminate between the slow mode phase speed and the sound speed within the precision of the present observations.
|Additional Information:||(c) 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A.|
|Uncontrolled Keywords (separate with ;):||Solar and Stellar Astrophysics (astro-ph.SR); Plasma physics; Astrophysics and astroparticles; MHD; stars: oscillations; Sun: atmospheric motions; Sun: corona; Sun: oscillations; waves|
|Subjects:||Q Science > QB Astronomy|
|Schools:||School of Computing Engineering & Physcial Sciences|
|Deposited On:||24 Jan 2011 15:04|
|Last Modified:||12 Mar 2012 17:25|
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