radio bursts and cme’s
DESCRIPTION
Radio bursts and CME’s. Monique Pick RHESSI workshop 5-8 April 2006. 17 March 2002 Y. Yan, M. Pick, M. Wang, S. Krucker, A. Vourlidas. RHESSI. NRH. OSRA. DAM. WAVES. 17 March 2002 Event A. AR 9871 4 NRH frequencies X 164 MHz, 236 MHz West more bursty Type III > 164 MHz. - PowerPoint PPT PresentationTRANSCRIPT
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Radio bursts and CME’s
Monique Pick
RHESSI workshop 5-8 April 2006
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17 March 2002Y. Yan, M. Pick, M. Wang, S. Krucker, A. Vourlidas
RHESSI
OSRA
DAM
WAVES
NRH
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17 March 2002 Event A
AR 9871
4 NRH frequencies•X 164 MHz, 236 MHz
•West more bursty• Type III > 164 MHz
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17 March 2002 Event BRHESSI
HXRWest source + polarityEast and middle sources mixed polarity
SXROutline 2 adjacent loops3 HXR sources at foot points
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17 March 2002 Event B
Continuum
Type III’s
O
236 MHzCadence 1s 600 km/s
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Continuum
17 March 2002 Event B
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17 March 2002 Event APotential magnetic field extrapolation(Yan, 2005)
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17 March 2002 Event BAR 9871 inside old remnant regionInclusion of small interacting loops CME above large extrapolated S loops
HXRWest source + polarityEast and middle sources mixed polaritySXROutline 2 adjacent loops « W » shape
HXR and Radio: Temporal relationshipSprangle &Vlahos, 1993 EM excited by unstable electron distribution inside the flaring loop and excite electrons along Open fields.
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17 March 2002 Event BHXR and Type III same electron population
Small loops emerge(1 or 2) interact with surrounding open field lines
HXR produced by electrons propagating downward
Outward electron beams propagate in the interface region between the ascending CME and the neighboring open field lines
Development of CME this region becomes highly compressed
TypeIII 2fp starting and ending altitudes at each frequency
Apparent motions of type III bursts increase in density 10 (4 at 164 MHz) Newkirk model
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•Electrons trace the expansion of the arch system(~2500 km/sec)•Coronal wave develops along flank of CME In lateral expansion
164 MHz
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