Standard

ISO/TS 21979:2018

Aug 2018 Published

Corrigendums and amendments are bought separately.

Language English

Services Read online + Print/Download €116.00 Read online €95.00 Printed and bound Delivery time: 5-10 days €116.00

There are no extended editions available for this standard

There are no available corrigendum or amendments for this standard. Any future corrigendum and amendments will be added automatically for subscribers.

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.

Document information

Standard from ISO
Published: 24 August 2018
Edition: 1
Document type: TS
Pages
ISBN:

Publisher ISO
Distributor ISO
ICS 49.140
ISO TC ISO/TC 20/SC 14

ISO/TS 21979:2018

Create subscription

Benefits of a subscription:

ISO/TS 21979:2018

ISO/TS 21979:2018

Abstract

Document information

Create subscription

Benefits of a subscription:

Extended editions Extended editions (0)

Version history Related corrigendum and amendments (0)

Version history History (2)

ISO/TS 21979:2018

ISO/TS 21979:2018

Abstract

Document information