Dynamic Variations in the in Wave Behavior of the Solar Atmosphere

Details Dynamic Variations in the in Wave Behavior of the Solar Atmosphere Dynamic Variations in the in Wave Behavior of the Solar Atmosphere

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005agusmsh11c..05a&link_type=abstract

American Geophysical Union, Spring Meeting 2005, abstract #SH11C-05

Physics

7522 Helioseismology

Scientific paper

It has been speculated that observed dynamic variations in the in wave behavior of the solar atmosphere are indications of rapid changes in the solar atmosphere. In particular, Finsterle et al. (SoPh 220 317-331) report an observation of rapidly changing wave behavior associated with an EIT observation suggestive of the break up of a magnetic loop. We examine the transient wave behavior using 100 hours of velocity observations using the K (770nm) and Na (589) Frauenhaufer lines from the Magneto Optical filter at Two Heights (MOTH) experiment compared to EIT observations.

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