๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Solar Maximum Mission

โœ Scribed by J. David Bohlin; Kenneth J. Frost; Peter T. Burr; Arun K. Guha; George L. Withbroe


Publisher
Springer
Year
1980
Tongue
English
Weight
590 KB
Volume
65
Category
Article
ISSN
0038-0938

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โœฆ Synopsis


The scientific objective of the Solar Maximum Mission is to understand the physics of solar flares. A description is provided for the SMM spacecraft, the scientific planning activity, the observing program and the guest investigator program associated with the mission.


๐Ÿ“œ SIMILAR VOLUMES


The solar maximum mission
โœ K. J. Frost ๐Ÿ“‚ Article ๐Ÿ“… 1983 ๐Ÿ› Springer ๐ŸŒ English โš– 17 KB

Individual papers in this issue also give in detail the parameters of the individual experiments carried by the spacecraft. A paper describing the Solar Maximum Mission by Frost will therefore not appear in these proceedings.

The gamma ray spectrometer for the Solar
โœ D. J. Forrest; E. L. Chupp; J. M. Ryan; M. L. Cherry; I. U. Gleske; C. Reppin; K ๐Ÿ“‚ Article ๐Ÿ“… 1980 ๐Ÿ› Springer ๐ŸŒ English โš– 498 KB

The Solar Maximum Mission Gamma Ray Experiment (SMM GRE) utilizes an actively shielded, multicrystal scintillation spectrometer to measure the flux of solar gamma rays. The instrument provides a 476-channel pulse height spectrum (with energy resolution of ~7% at 662 keV) every 16.38 s over the energ