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Kilometric shock-associated events and microwave burstsThe peak times of impulsive microwaves bursts are compared with those of shock-associated (SA) kilometric radio events. The first peaks in these two frequency regimes are usually well-correlated in time, but the last peaks of the SA events observed at 1 MHz occur an average of 20 min after the last impulsive microwave peaks. In some cases, the SA events overlap in time with the post-burst increases of microwave bursts; sometimes there is general correspondence in their intensity time profiles. These observations suggest that the earlier components of the SA events are usually caused by electrons accelerated in or near the microwave source region. The possibility that the later components of some SA events could be associated with nonthermal electrons responsible for microwave post-burst increases, although they have traditionally been attributed to electrons accelerated at type II burst producing shocks in the upper corona is discussed.
Document ID
19900049330
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Kundu, M. R.
(Maryland, University College Park, United States)
Macdowall, R. J.
(ST Systems Corp Lanham, MD, United States)
Stone, R. G.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 14, 2013
Publication Date
March 1, 1990
Publication Information
Publication: Astrophysics and Space Science
Volume: 165
Issue: 1 Ma
ISSN: 0004-640X
Subject Category
Solar Physics
Accession Number
90A36385
Funding Number(s)
CONTRACT_GRANT: NSF ATM-87-17157
Distribution Limits
Public
Copyright
Other

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