Reference number
ISO/TR 18147:2014
Technical Report
ISO/TR 18147:2014
Space environment (natural and artificial) — Method of the solar energetic protons fluences and peak fluxes determination
Edition 1
2014-04
Technical Report
Preview
ISO/TR 18147:2014
61603
недоступно на русском языке
Опубликовано (Версия 1, 2014)

ISO/TR 18147:2014

ISO/TR 18147:2014
61603
Язык
Формат
CHF 129
Пересчитать швейцарские франки (CHF) в ваша валюта

Тезис

ISO/TR 18147:2014 is intended for calculating the probability for solar energetic particle (SEP) to have an impact on materials, hardware, and biological objects.

ISO/TR 18147:2014 establishes the differential energy spectra for the (0,1/103) MeV SEP fluences and/or peak fluxes in the near-earth space, beyond the earth magnetosphere during the missions any duration under varying solar activity.

If additional prepositions are used, the method establishes the basic fluences and peak fluxes for their determination throughout the heliosphere. When the effect of the particle penetration into the magnetosphere is taken into account, the method establishes the basic fluences and peak fluxes for their determination on the near-earth spacecraft and manned station orbits.

Because the occurrence of SEP is a process a probabilistic nature, fluences and peak fluxes calculation relate to the different levels of probability.

The method is intended for specialists engaged in determination of radiation conditions in space.

Общая информация

  •  : Опубликовано
     : 2014-04
    : Опубликование международного стандарта [60.60]
  •  : 1
  • ISO/TC 20/SC 14
    49.140 
  • RSS обновления

Жизненный цикл

Цели в области устойчивого развития

Данный стандарт разработан для достижения следующих Цель устойчивого развития

Появились вопросы?

Ознакомьтесь с FAQ