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Title: Peak-flux-density spectra of large solar radio bursts and proton emission from flares. Environmental research papers, July 1981-July 1985

Technical Report ·
OSTI ID:5728307

The relationship between U-shaped peak-flux-density microwave spectra and solar proton events was re-examined 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% 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%). Nine percent of the events had intermediate spectra with a maximum > or = 800 sfu at f > or = 2 GHz and 100 sfu < or = Sp (200 MHz) < 800 sfu. The authors were unable to classify 15% of the events because of incomplete data. The associations of the three classes of spectra with Type II (and/or Type IV) meter-wavelenght bursts and > 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% of large microwave bursts with U-shaped spectra are associated with Type II/IV events), protons (77%); intermediate Type II/IV (78%), protons (73%); and cutoff Type II/IV (22%), protons (33%). 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.

Research Organization:
Air Force Geophysics Lab., Hanscom AFB, MA (USA)
OSTI ID:
5728307
Report Number(s):
AD-A-164458/2/XAB; AFGL-TR-85-0180
Country of Publication:
United States
Language:
English