HR: 09:45h
AN: SH11C-05    [Abstracts]
TI: Dynamic Variations in the in Wave Behavior of the Solar Atmosphere
AU: * Armstrong, J D
EM: jd@msrc.um.edu
AF: Maui Scientific Research Center University Of New Mexico, 590 Lipoa Parkway Suite #272, Kihei, HI 96753 United States
AU: Jefferies, S
EM: stuartj@hpc.unm.edu
AF: Maui Scientific Research Center University Of New Mexico, 590 Lipoa Parkway Suite #272, Kihei, HI 96753 United States
AB: 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.
DE: 7522 Helioseismology
SC: SPA-Solar and Heliospheric Physics [SH]
MN: 2005 Joint Assembly