๐”– Bobbio Scriptorium
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Detecting the flux of solar X-ray bursts from the ground

โœ Scribed by Yong-rui Miao; Ke-jun Yang; Da-ming Li; Lu-zheng Tu

Book ID
115957705
Publisher
Elsevier Science
Year
1985
Tongue
English
Weight
390 KB
Volume
47
Category
Article
ISSN
0021-9169

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๐Ÿ“œ SIMILAR VOLUMES

Hard X-ray bursts from flares behind the
Hard X-ray bursts from flares behind the solar limb
โœ David L. Mckenzie ๐Ÿ“‚ Article ๐Ÿ“… 1975 ๐Ÿ› Springer ๐ŸŒ English โš– 459 KB

The determination of the location of the region of origin of hard X-rays is important in evaluating the importance of 10-100 keV electrons in solar flares arm in understanding flare particle acceleration. At present only limb-occulted events are available to give some information on the height of X-

The Hard X-Ray Burst Spectrometer on the
The Hard X-Ray Burst Spectrometer on the Solar Maximum Mission
โœ L. E. Orwig; K. J. Frost; B. R. Dennis ๐Ÿ“‚ Article ๐Ÿ“… 1980 ๐Ÿ› Springer ๐ŸŒ English โš– 740 KB

The primary scientific objectives of the Hard X-Ray Burst Spectrometer (HXRBS) to be flown on the Solar Maximum Mission are as follows: (1) To determine the nature of the mechanisms which accelerate electrons to 20-100 keV in the first stage of a solar flare and to > 1 MeV in the second stage of man