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. | File Size : | 1
file
, 2 MB |
| ISBN(s) : | 9780580959929 |
| Note : | This product is unavailable in Ukraine, Russia, Belarus |
| Number of Pages : | 26 |
| Product Code(s) : | 30349569, 30349569, 30349569 |
| Published : | 08/29/2018 |
| Same As : | BS PD ISO/TS 21979:2018 |
