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Fast drift kilometric radio bursts and solar proton eventsInitial results of a comparative study of major fast drift kilometric bursts and solar proton events from Sep. 1978 to Feb. 1983 are presented. It was found that only about half of all intense, long duration ( 40 min above 500 sfu) 1 MHz bursts can be associated with F 20 MeV proton events. However, for the subset of such fast drift bursts accompanied by metric Type 2 and/or 4 activity (approximately 40% of the total), the degree of association with 20 MeV events is 80%. For the reverse association, it was found that proton events with J( 20 MeV) 0.01 1 pr cm(-2)s(-1)sr(-1)MeV(-1) were typically (approximately 80% of the time) preceded by intense 1 MHz bursts that exceeded the 500 sfu level for times 20 min (median duration approximately 35 min).
Document ID
19850026421
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Cliver, E. W.
(Air Force Geophysics Lab. Greenbelt, MD, United States)
Kahler, S. W.
(Emmanuel Coll. Greenbelt, MD, United States)
Cane, H. V.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Mcguire, R. E.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Vonrosenvinge, T. T.
(NASA Goddard Space Flight Center)
Stone, R. G.
(NASA Goddard Space Flight Center)
Date Acquired
August 12, 2013
Publication Date
August 1, 1985
Publication Information
Publication: 19th Intern. Cosmic Ray Conf - Vol. 4
Subject Category
Solar Physics
Report/Patent Number
SH-1.1-7
Report Number: SH-1.1-7
Accession Number
85N34734
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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