GB/T 41457-2022Space environment - Solar proton fluences at GEO and guideline for selection of confidence level in statistical model of solar proton fluencies (English PDF)
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Issued by
State Administration for Market Regulation, China National Standardization Administration
Level / Type
National · Recommended
Issue date
April 15, 2022
Implementation date
November 1, 2022
Scope
GB/T 41457-2022 (Space environment - Solar proton fluences at GEO and guideline for selection of confidence level in statistical model of solar proton fluencies) is available as an English-translated PDF.
GB/T 41457-2022 — This document presents the method and options for estimating the long-term (solar activity cycle greater than 11 years) fluence of solar protons in geosynchronous orbit (GEO). Guidelines for choosing confidence levels for solar proton fluence models. This document applies to performance degradation estimates of solar cells. Charge coupled device (CCD), image sensor (APS) and other optoelectronic devices The performance degradation estimation is used for reference.
Document preview — GB/T 41457-2022
National Standard of the People's Republic of China
- Classification
- V 06
Issued by: State Administration for Market Regulation, China National Standardization Administration
Contents
- foreword
- 1 Scope
- 2 Normative references
- 3 Terms and Definitions
foreword
This document is in accordance with the provisions of GB/T 1.1-2020 "Guidelines for Standardization Work Part 1.Structure and Drafting Rules of Standardization Documents"
drafted.
This document is modified and adopted ISO 12208.2015 "Space system space environment (artificial and natural) long-term observation quality in geosynchronous orbit
Guidelines for choosing confidence levels for statistical models of sub-fluence and solar proton fluence.
Compared with ISO 12208.2015, this document has the following structural adjustments.
--- Added "2 Normative Reference Documents";
--- Added "3.6 relative damage coefficient" in "Terms and Definitions".
Compared with ISO 12208.2015, this document has many technical differences. In the outer margins of the clauses involved, vertical
A single line (︱) is marked. See Appendix A for a list of these technical differences and their reasons.
The following editorial changes have been made to this document.
--- Modify the title of the document to adapt to the Chinese, and change it to "Space Environment Geosynchronous Orbit Solar Proton Flux and Its Statistics
Model Confidence Selection Guide;
--- Reorganization and identification of references;
--- The title of Appendix B has been rewritten;
--- Modify "AE-8" in B.3.1 to "AE-9".
Please note that some content of this document may be patented. The issuing agency of this document assumes no responsibility for identifying patents.
1 Scope
This document presents the method and options for estimating the long-term (solar activity cycle greater than 11 years) fluence of solar protons in geosynchronous orbit (GEO).
Guidelines for choosing confidence levels for solar proton fluence models.
This document applies to performance degradation estimates of solar cells. Charge coupled device (CCD), image sensor (APS) and other optoelectronic devices
The performance degradation estimation is used for reference.
2 Normative references
The contents of the following documents constitute essential provisions of this document through normative references in the text. Among them, dated citations
documents, only the version corresponding to that date applies to this document; for undated references, the latest edition (including all amendments) applies to
this document.
GB/T 32452 Spacecraft Space Environment Terminology
3 Terms and Definitions
The terms and definitions defined in GB/T 32452 and the following apply to this document.
3.1
confidence level
Confidence level
The confidence level used for cumulative fluence estimates.
3.2
extremely rare event extremelyrareevent
The solar energy proton (SEP) event occurs only once in a solar cycle, and the mass in a complete solar cycle
The sub-fluence is mainly derived from this SEP event.
Note. SEP events that occurred in August 1972, October 1989 or July.2000 are extremely rare events.
3.3
flux
The number of particles passing through a specific area per unit time.
3.4
fluence
Time integral of flux.
3.5
n-year fluence
The fluence for the n-year mission period.
......
This preview omits tables, figures, formulas and parts of the technical clauses. The complete document — all pages — is available in the English PDF.
Referenced standards
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