The Auroral Particle Detection

The Auroral Particle Detection

An outline of the auroral particle detector which is planned to be flown in the Japanese Antarctic rocket experiments during IMS is presented. The detector uses a combination of curved plate electrostatic analysers and channel electron multipliers together with thin foils. It measures 0.1, 0.3, 0.5,...

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Main Author: Haruya MATSUMOTO
Format: Article
Language:English
Published: National Institute of Polar Research 1975-03-01
Series:Antarctic Record
Online Access:https://doi.org/10.15094/00007793
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spelling doaj-55e389130e254bfbad9124977f6782c82020-11-25T00:03:39ZengNational Institute of Polar ResearchAntarctic Record0085-72892432-079X1975-03-0152747710.15094/00007793The Auroral Particle DetectionHaruya MATSUMOTO0Faculty of Engineering, Kobe UniversityAn outline of the auroral particle detector which is planned to be flown in the Japanese Antarctic rocket experiments during IMS is presented. The detector uses a combination of curved plate electrostatic analysers and channel electron multipliers together with thin foils. It measures 0.1, 0.3, 0.5, 1, 3, 5keV electrons. The observable fluxes are 10^5-10^8/cm^2 s sr keV for all energies with the pitch angle resolution of 20°-30°. Measurements of proton flux are also under consideration.https://doi.org/10.15094/00007793
collection DOAJ
language English
format Article
sources DOAJ
author Haruya MATSUMOTO
spellingShingle Haruya MATSUMOTO
The Auroral Particle Detection
Antarctic Record
author_facet Haruya MATSUMOTO
author_sort Haruya MATSUMOTO
title The Auroral Particle Detection
title_short The Auroral Particle Detection
title_full The Auroral Particle Detection
title_fullStr The Auroral Particle Detection
title_full_unstemmed The Auroral Particle Detection
title_sort auroral particle detection
publisher National Institute of Polar Research
series Antarctic Record
issn 0085-7289
2432-079X
publishDate 1975-03-01
description An outline of the auroral particle detector which is planned to be flown in the Japanese Antarctic rocket experiments during IMS is presented. The detector uses a combination of curved plate electrostatic analysers and channel electron multipliers together with thin foils. It measures 0.1, 0.3, 0.5, 1, 3, 5keV electrons. The observable fluxes are 10^5-10^8/cm^2 s sr keV for all energies with the pitch angle resolution of 20°-30°. Measurements of proton flux are also under consideration.
url https://doi.org/10.15094/00007793
work_keys_str_mv AT haruyamatsumoto theauroralparticledetection
AT haruyamatsumoto auroralparticledetection
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