Astronomy and Astrophysics – Astrophysics
Scientific paper
Sep 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...308..436k&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 308, Sept. 1, 1986, p. 436-442.
Astronomy and Astrophysics
Astrophysics
19
Solar Flares, Solar Radio Bursts, Solar X-Rays, Spectroheliographs, Type 3 Bursts
Scientific paper
Microbursts are low-brightness-temperature bursts observed by the Clark Lake radioheliograph. The bursts occur several times per hour during quiet-sun periods and are seen at the observing frequencies from 30 to 70 MHz. They are stationary at a given frequency, have short rise times and durations of 2-10 s. Here, observations of the bursts are presented and interpretated in terms of plasma emission. The burst properties suggest that they are weak type III bursts. The observations imply that energy releases on the sun continue to be impulsive, with nonthermal electron distributions, for small releases of energy. The relation of the bursts to type III bursts and hard X-ray bursts is discussed.
Gergely Tomas E.
Kundu Mukul R.
Loiacono R.
Szabo Andras
White Stephen M.
No associations
LandOfFree
Solar microbursts at meter-dekameter wavelengths 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 Solar microbursts at meter-dekameter wavelengths, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar microbursts at meter-dekameter wavelengths will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1290798