Hostname: page-component-8448b6f56d-t5pn6 Total loading time: 0 Render date: 2024-04-19T15:32:29.693Z Has data issue: false hasContentIssue false
  • English
  • Français

A Satellite Experiment to Measure the Intensity and the Energy Spectrum of Gamma Rays from Solar Flares in the Range 50–500 MeV

Published online by Cambridge University Press:  14 August 2015

G. F. Bignami ,
C. J. Bland ,
O. Citterio ,
A. J. Dean  and
P. Inzani
G. F. Bignami
Affiliation:
Università Degli Studi di Milano, Istituto di Scienze Fisiche, Milano, Italy
C. J. Bland
Affiliation:
Università Degli Studi di Milano, Istituto di Scienze Fisiche, Milano, Italy
O. Citterio
Affiliation:
Università Degli Studi di Milano, Istituto di Scienze Fisiche, Milano, Italy
A. J. Dean
Affiliation:
Università Degli Studi di Milano, Istituto di Scienze Fisiche, Milano, Italy
P. Inzani
Affiliation:
Università Degli Studi di Milano, Istituto di Scienze Fisiche, Milano, Italy

Extract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A high energy solar gamma-ray telescope incorporating a lenticular Čerenkov for directional measurement and an energy calorimeter is described. The instrument is included in the payload of the TD-1 ESRO spacecraft to be launched into a sun-pointing orbit during spring 1972. The results of laboratory and accelerator tests are presented and the sensitivity and measurement capability to solar flare gamma rays is discussed.

Type
Part I: Gamma-Ray Astronomy
Information
Symposium - International Astronomical Union , Volume 41: New Technique in Space Astronomy , 1971 , pp. 44
Copyright
Copyright © Reidel 1971