๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

The solar maximum mission

โœ Scribed by K. J. Frost

Publisher
Springer
Year
1983
Tongue
English
Weight
17 KB
Volume
86
Category
Article
ISSN
0038-0938

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โœฆ Synopsis

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.

๐Ÿ“œ SIMILAR VOLUMES

Solar Maximum Mission
Solar Maximum Mission
โœ J. David Bohlin; Kenneth J. Frost; Peter T. Burr; Arun K. Guha; George L. Withbr ๐Ÿ“‚ Article ๐Ÿ“… 1980 ๐Ÿ› Springer ๐ŸŒ English โš– 590 KB

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.

The gamma ray spectrometer for the Solar
The gamma ray spectrometer for the Solar Maximum Mission
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

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