ISO/TS 21979:2018

Published (Edition 1, 2018)

This publication was last reviewed and confirmed in 2021. Therefore this version remains current.

ISO/TS 21979:2018

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Abstract

This document, by using a model that reproduces the fluctuations of radiation belts, defines the calculation method (orbit, operation period) of the radiation fluence received by a satellite. The quasi-dynamic model of Earth's radiation belts adopts input parameters (index values) to predict variation. The input parameters are selected from those that are easy to obtain data and have high correlation with the variation in Earth's radiation belts.

NOTE This method is an engineering method used for satellite design and similar purposes.

General information

Status
: Published

Publication date
: 2018-09

Stage
: International Standard under systematic review [90.20]
Edition
: 1

Number of pages
: 18
Technical Committee :
ISO/TC 20/SC 14

ICS :
49.140
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