Physics
Scientific paper
Oct 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990soph..129..343k&link_type=abstract
Solar Physics (ISSN 0038-0938), vol. 129, Oct. 1990, p. 343-349.
Physics
1
Solar Flares, Solar X-Rays, X Ray Spectra, H Alpha Line, Light Curve, Solar Maximum Mission, Ultraviolet Spectra
Scientific paper
Observations of the 15:22 UT flare of June 24, 1980 were made using the VLA at 6 cm wavelength simultaneously with the Hard X-Ray Imaging Spectrometer (HXIS) aboard the Solar Maximum Mission. It was found that at the peak of the impulsive phase, the brightest microwave point appeared to lie between the soft (3.6-8.0 keV) and hard (22-30 keV) X-ray maxima, which were themselves separated by about 20 arcsec. Since the publication of these results, the imaging data from the Ultraviolet Spectrometer Polarimeter (UVSP) have been analyzed with the goal of narrowing the possible interpretations of the event. Like the VLA and HXIS, the UVSP observations provide information about the location of the primary electrons; the observations taken together suggest that the fast electrons were symmetrically distributed within the flare loop.
Cheng Chung-Chieh
Kundu Mukul R.
Schmahl Ed. J.
No associations
LandOfFree
UVSP and VLA observations of the 24 June 1980 flare - Asymmetric or isotropic beaming? 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 UVSP and VLA observations of the 24 June 1980 flare - Asymmetric or isotropic beaming?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and UVSP and VLA observations of the 24 June 1980 flare - Asymmetric or isotropic beaming? will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1305731