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BS PD ISO/TS 21979:2018, 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.

Cross References:
ISO 16695:2014
ISO 12208:2015
ISO 22009:2009
ISO 16698:2013

All current amendments available at time of purchase are included with the purchase of this document.

Product Details

Published:
08/29/2018
ISBN(s):
9780580959929
Number of Pages:
26
File Size:
1 file , 2 MB
Same As:
ISO/TS 21979:2018
Product Code(s):
30349569, 30349569, 30349569