Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988apj...327..998r&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 327, April 15, 1988, p. 998-1008.
Astronomy and Astrophysics
Astrophysics
46
Helium Isotopes, Radio Bursts, Solar Flares, Solar Radio Emission, Solar X-Rays, Type 3 Bursts, Goes Satellites, International Sun Earth Explorers, Solar Maximum Mission, X Ray Spectra
Scientific paper
Radio and X-ray properties of solar flares associated with a new sample of individual (He-3) rich solar particle events are examined. Given the association between kilometric type III bursts and (He-3) rich events, the timing of the radio events is used to identify the related X-ray increases. The X-ray events exhibit a rich variety, from the standpoint of both intensity and complexity. Examination of the events shows statistically significant anticorrelations between the He-3/He-4 ratio and the intensity of the event as measured at kilometric wavelengths and in hard and soft X-rays; larger He-3/He-4 ratios occur in smaller flares. The result suggests that a coupling may exist between the preheating phase and the acceleration phase of these events or that mixing occurs between an enriched particle population accelerated within the compact flare and a normal population accelerated by a shock propagating away from an intense flare.
Dennis Brian R.
Lin Robert P.
Reames Donald. V.
Stone Robert G.
No associations
LandOfFree
X-ray and radio properties of solar (He-3) rich events does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with X-ray and radio properties of solar (He-3) rich events, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and X-ray and radio properties of solar (He-3) rich events will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-848094