Solar Cycle 24 Group F: Difference between revisions
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''Introduction'' 14:30 - 16:00 | ''Introduction'' 14:30 - 16:00 | ||
STERLING Earliest phases of solar eruptions | [[STERLING]] [[Earliest phases of solar eruptions]] | ||
preflare phase & trigger mechanism | preflare phase & trigger mechanism | ||
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QUESTIONS ARISING: | |||
how common is a slow rise? | how common is a slow rise? | ||
what triggers slow & fast rise phases? | what triggers slow & fast rise phases? | ||
Revision as of 23:20, 9 December 2008
Tuesday 9th Dec:
Introduction 14:30 - 16:00
STERLING Earliest phases of solar eruptions
preflare phase & trigger mechanism for filaments as tracer of B field, slow rise -> flare + fast rise
few (12) example event studied. 2 may 2007, TRACE & HINODE, good example.
filaments undergo slow rise (few km/s), then fast. the slow rise is linear then flare at start of fast eruption. could be some signatures of 'breakout'
dimmings - local (near neutral line) or remote (associated with breakout?)
QUESTIONS ARISING:
how common is a slow rise?
what triggers slow & fast rise phases?
where to go from here? Clearly Hinode and SECCHI 171 2 min cadence? so synoptic data modes are fine for this project?
McAteer
Atrill
Steed
Howard
Events 17:00-18:30