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‡b.C55 1985
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‡aD 301.45/4:85-0180
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‡aD 301.45/39:924
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‡aADA 164458
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‡aAFGL TR 85-180
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‡aCliver, Edward W.
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‡aPeak-flux-density spectra of large solar radio bursts and proton emission from flares /
‡cE.W. Cliver, L.F. McNamara, L.C. Gentile.
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‡aHanscom AFB, Massachusetts :
‡bAir Force Geophysics Laboratory, Air Force Systems Command, United States Air Force,
‡c1985.
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‡avi, 53 pages :
‡billustrations, tables ;
‡c28 cm.
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‡atext
‡btxt
‡2rdacontent
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‡aunmediated
‡bn
‡2rdamedia
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‡avolume
‡bnc
‡2rdacarrier
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‡aEnvironmental Research Papers ;
‡vNo. 924
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‡aAFGL-TR ;
‡v85-180
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‡aResearch supported by the Air Force Geophysics Laboratory, United States AIr Force, Hanscom AFB, Massachusetts.
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‡aSpace Physics Division Project 2311.
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‡aADA164458 (from http://www.dtic.mil).
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‡a"19 August 1985."
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‡aIncludes bibliographical references (pages 50-53).
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‡aWe have reexamined the relationship between U-shaped peak-flux-density microwave spectra and solar proton events for approx 200 large (Sp(> or = 2GHz)> or = 800 solar flux uits (sfu) microwave burst (1965 - 1979). The radio spectra fell into two basic classes: (a) U-shaped with two maxima (> or = 800 sfu) in the range from 200 MHz to> or = 10 GHz (59 percent of all events), and (b) cutoff spectra with a maximum> or = 800 sfu at f> or = 2 GHz and Sp (200 MHz) <100 sfu (18 percent). Nine percent of the events had intermediate spectra with a maximum> or = 800 sfu at f> or = 2 GHz and 100 sfu 10 MeV proton events of any size (> or = 0.01 pr per sq cm per sec per sr) are as follows: U-shaped Type II/IV (90 percent of large microwave bursts with U-shaped spectra are associated with Type II/IV events), protons (77 percent); intermediate Type II/IV (78 percent), protons (73 percent); and cutoff Type II/IV (22 percent), protons (33 percent). These statistics affirm various lines of evidence linking coronal shock waves and interplanetary proton events. They also suggest that the meter wavelength branch of the U-shaped spectrum may be attributable to second phase (vs flash phase) accelerated electrons.
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‡aMode of access: Internet.
|
650 |
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7 |
‡aSolar radio emission.
‡2fast
‡0http://id.worldcat.org/fast/1125185
|
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⊔ |
7 |
‡aSolar radio bursts.
‡2fast
‡0http://id.worldcat.org/fast/1125183
|
650 |
⊔ |
7 |
‡aRadiofrequency spectroscopy.
‡2fast
‡0http://id.worldcat.org/fast/1088068
|
650 |
⊔ |
7 |
‡aRadio sources (Astronomy)
‡2fast
‡0http://id.worldcat.org/fast/1087565
|
650 |
⊔ |
7 |
‡aProton flares.
‡2fast
‡0http://id.worldcat.org/fast/1080070
|
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⊔ |
0 |
‡aRadiofrequency spectroscopy.
‡0http://id.loc.gov/authorities/subjects/sh85110682
|
650 |
⊔ |
0 |
‡aRadio sources (Astronomy)
‡0http://id.loc.gov/authorities/subjects/sh85110574
|
650 |
⊔ |
0 |
‡aSolar radio bursts.
‡0http://id.loc.gov/authorities/subjects/sh94006244
|
650 |
⊔ |
0 |
‡aSolar radio emission.
‡0http://id.loc.gov/authorities/subjects/sh85124541
|
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0 |
‡aProton flares.
‡0http://id.loc.gov/authorities/subjects/sh85107790
|
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‡aGentile, L. C.
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‡aMcNamara, L. F.
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2 |
⊔ |
‡aU.S. Air Force Geophysics Laboratory.
‡0http://id.loc.gov/authorities/names/n79109638
‡1http://id.loc.gov/rwo/agents/n79109638
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‡aTechnical Report Archive & Image Library (TRAIL)
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