HR: 1340h
AN: SH13A-0282    [Abstracts]
TI: Case Study of A Sequential Chromospheric Brightening (SCB) Associated with May 6, 2005 event.
AU: * Balasubramaniam, K S
EM: bala@nso.edu
AF: National Solar Observatory, Sacramento Peak, Sunspot, NM 88349
AU: Pevtsov, A A
EM: apevtsov@nso.edu
AF: National Solar Observatory, Sacramento Peak, Sunspot, NM 88349
AU: Hock, R A
EM: rhock@wellesley.edu
AF: National Solar Observatory, Sacramento Peak, Sunspot, NM 88349
AB: A sequential chromospheric brightening on May 6, 2005 was accompanied by a long duration event, LDE (16:00 - 23:00 UT). Using data from ISOON/ H-alpha, TRACE (171 A), and SOHO/MDI (magnetograms) missions, we present a detailed sequential study of this event that includes large scale coronal disturbances(TRACE 171 A), ribbon-ed flares (ISOON & TRACE), large scale motion of magnetic fields (SOHO/MDI), filament eruptions (ISOON & TRACE), flares, and post-flare loops (TRACE). This event presents a good example in the continuity of events comprising an LDE. We present a model of the eruptive process of this LDE.
DE: 7500 SOLAR PHYSICS, ASTROPHYSICS, AND ASTRONOMY
DE: 7507 Chromosphere
DE: 7509 Corona
DE: 7513 Coronal mass ejections (2101)
DE: 7519 Flares
SC: SPA-Solar and Heliospheric Physics [SH]
MN: Fall Meeting 2005