ISO/TR 23989:2020

недоступно на русском языке

Тезис

This document provides guidelines for specifying the qualitative estimation of the solar wind energy input into the magnetosphere with use of operative ground-based information on the polar cap magnetic activity (PC index).

The solar wind energy incoming into the magnetosphere predetermines development of the magnetospheric disturbances: magnetic storms and substorms. Magnetospheric disturbances include a wide range of phenomena and processes directly affecting human activity, such as satellite damage, radiation hazards for astronauts and airline passengers, telecommunication problems, outrages of power and electronic systems, effects in the atmospheric processes, and impact on human health.

This document is intended for on-line monitoring the magnetosphere state and nowcasting the intensity and extent of magnetic disturbances as well as parameters of the high-latitude ionosphere. The method and accuracy of estimating is ascertained by close relationship between the PC index and interplanetary electric field (as the most geoeffective solar wind parameter), on the one hand, and between the PC index and magnetoshpheric disturbances, on the other hand.

Общая информация

Текущий статус
: Published

Дата публикации
: 2020-01
Версия
: 1
Технический комитет
: ISO/TC 20/SC 14 Space systems and operations
ICS
:
49.140 Space systems and operations

Данный стандарт разработан для достижения следующих Цель устойчивого развития:

Индустриализация, инновации и инфраструктура

Приобрести данный стандарт

	Формат	Язык
std 1 61	PDF
std 2 61	Бумажный

CHF61

Жизненный цикл

Сейчас

Published

ISO/TR 23989:2020
Этап: 60.60

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