✦ LIBER ✦

The Solar Maximum Mission workshops

✍ Scribed by Keith T. Strong

Publisher: Springer
Year: 1987
Tongue: English
Weight: 188 KB
Volume: 113
Category: Article
ISSN: 0038-0938
DOI: 10.1007/bf00147679

No coin nor oath required. For personal study only.

📜 SIMILAR VOLUMES

The solar maximum mission

✍ K. J. Frost 📂 Article 📅 1983 🏛 Springer 🌐 English ⚖ 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.

Solar Maximum Mission

✍ J. David Bohlin; Kenneth J. Frost; Peter T. Burr; Arun K. Guha; George L. Withbr 📂 Article 📅 1980 🏛 Springer 🌐 English ⚖ 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

✍ D. J. Forrest; E. L. Chupp; J. M. Ryan; M. L. Cherry; I. U. Gleske; C. Reppin; K 📂 Article 📅 1980 🏛 Springer 🌐 English ⚖ 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

Observation of chromospheric evaporation

Observation of chromospheric evaporation during the solar maximum mission

✍ E. Antonucci; B. R. Dennis 📂 Article 📅 1983 🏛 Springer 🌐 English ⚖ 507 KB

White-light flares observed by the solar

White-light flares observed by the solar maximum mission satellite

✍ E. Rieger; Wei-Qun Gan 📂 Article 📅 1994 🏛 Elsevier Science 🌐 English ⚖ 97 KB

The Hard X-Ray Burst Spectrometer on the

The Hard X-Ray Burst Spectrometer on the Solar Maximum Mission

✍ L. E. Orwig; K. J. Frost; B. R. Dennis 📂 Article 📅 1980 🏛 Springer 🌐 English ⚖ 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