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GB/T 31157-2014: Classification for the intensity of solar soft X-ray flare
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Classification for the intensity of solar soft X-ray flare
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GB/T 31157-2014
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Basic data | Standard ID | GB/T 31157-2014 (GB/T31157-2014) | | Description (Translated English) | Classification for the intensity of solar soft X-ray flare | | Sector / Industry | National Standard (Recommended) | | Classification of Chinese Standard | A47 | | Classification of International Standard | 07.060 | | Word Count Estimation | 18,156 | | Date of Issue | 9/3/2014 | | Date of Implementation | 1/1/2015 | | Regulation (derived from) | People's Republic of China Announcement of Newly Approved National Standards No. 21 of 2014 | | Issuing agency(ies) | General Administration of Quality Supervision, Inspection and Quarantine of the People's Republic of China, Standardization Administration of the People's Republic of China | | Summary | This Standard specifies the classification of soft X-ray solar flares strength. This Standard is applicable to the monitoring and early warning service solar soft X-ray flares. | GB/T 31157-2014: Classification for the intensity of solar soft X-ray flare---This is a DRAFT version for illustration, not a final translation. Full copy of true-PDF in English version (including equations, symbols, images, flow-chart, tables, and figures etc.) will be manually/carefully translated upon your order.
Classification for the intensity of solar soft X-ray flare
ICS 07.060
A47
National Standards of People's Republic of China
Solar soft X-ray flares strength rating
Issued on. 2014-09-03
2015-01-01 implementation
Administration of Quality Supervision, Inspection and Quarantine of People's Republic of China
Standardization Administration of China released
Table of Contents
Introduction Ⅲ
Introduction Ⅳ
1 Scope 1
2 Terms and definitions 1
3 solar soft X-ray flare intensity grading 1
References 13
Foreword
This standard was drafted in accordance with GB/T 1.1-2009 given rules.
The standard proposed by the China Meteorological Administration.
This standard by the National Satellite Meteorology and Space Weather Space Weather Monitoring and Warning Committee for Standardization Technical Committee (SAC/TC347/SC3)
Centralized.
This standard was drafted. National Satellite Meteorological Center (National Space Weather Monitoring and Warning Center).
The main drafters of this standard. your music out, Zhaohai Juan, Tian Mao Zong bit country.
Introduction
Solar Soft X-ray flares accompanied by enhanced electromagnetic radiation and particle acceleration of particles in the ionosphere and space weather environment may cause
A great influence. Solar soft X-ray flare monitoring space weather monitoring and early warning has become an important business. In order to quantitatively describe too
The degree of strength of the male soft X-ray flare, the standard is formulated.
Solar soft X-ray flares strength rating
1 Scope
This standard specifies the soft X-ray solar flares strength rating.
This standard applies to the monitoring and early warning service solar soft X-ray flares.
2 Terms and definitions
The following terms and definitions apply to this document.
2.1
Solar flares solarflare
Local area solar atmosphere suddenly lightened active phenomena, often accompanied by enhanced electromagnetic radiation and particle emission.
2.2
Soft X-ray solar flares solarsoftX-rayflare
Solar flares in soft X-ray band phenomenon occurred.
2.3
Soft X-ray intensity solar flares intensityofsolarsoftX-rayflare
In the Earth's atmosphere, the astronomical units from the sun at a solar soft X-ray flares in 1 × 10-10m ~ 8 × 10-10m band Fan
Around the peak flow of the electromagnetic radiation.
Note 1. The symbol FX expressed in units of J/(m2 · s).
Note 2. 1 astronomical unit = 149598000km.
3 solar soft X-ray flares strength rating
3.1 solar soft X-ray flare intensity according to traffic volume is divided into A, B, C, M, X five levels, see Table 1.
Table 1 solar soft X-ray flare intensity level
Intensity level
Flow range
J/(m2 · s)
A 1.00 × 10-8≤FX < 1.00 × 10-7
B 1.00 × 10-7≤FX < 1.00 × 10-6
C 1.00 × 10-6≤FX < 1.00 × 10-5
M 1.00 × 10-5≤FX < 1.00 × 10-4
X 1.00 × 10-4≤FX
3.2 A class flares subdivided into 90, from A1.0 [1.00 × 10-8J/(m2 · s)] began, FX for each additional 0.1 × 10-8J/(m2 · s), Yao
Spot intensity level increased by 0.1, see Table 2.
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