BS ISO 17520:2024
Space environment (natural and artificial). Cosmic ray and solar energetic particle penetration inward the magnetosphere. Method of determination of the effective vertical cut-off rigidity

Standard No.
BS ISO 17520:2024
Release Date
2024
Published By
British Standards Institution (BSI)  GB  /  BSI
Latest
BS ISO 17520:2024
 

Introduction

Technical Overview of Cosmic Ray Penetration Standards

The BS ISO 17520:2024 standard establishes methodologies for calculating effective vertical cut-off rigidities (EVCR) of charged particles in near-Earth space. This revision supersedes the 2016 edition with key updates including:

Feature 2016 Edition 2024 Edition
Reference Epochs 2005-2015 2005-2020
IGRF Models Basic tables for 3 epochs Added 2020 epoch data
Accuracy ±2% Enhanced validation

Core Calculation Methodology

The standard specifies trajectory tracing techniques for negatively charged particles using:

  • IGRF models for internal geomagnetic fields
  • Tsyganenko models for external magnetospheric effects

Critical parameters include:

  • Geographic coordinates (λ,φ)
  • Altitude range: 250-20,000 km
  • Kp-index (0-9 scale)
  • Local time (T)

Implementation Guidelines

For operational applications:

  1. Use Tables B.1-B.4 for IGRF reference values
  2. Apply altitude correction via Formula (B.2)
  3. Calculate disturbance effects using Equations (B.3-B.6)

Practical Example

For a satellite at 1,000 km altitude (λ=10°, φ=0°) during moderate geomagnetic activity (Kp=3):

  • Base R0 = 12.684 GV (from Table B.4)
  • Altitude-adjusted R0 = 12.421 GV
  • Final Reff = 10.751 GV (per Table B.5 validation)

Technical Evolution

The standard reflects 8 years of magnetospheric research advancements:

  • Improved correlation (r=0.998) with 1990 reference data
  • Extended validity to 0.2 GV lower limit
  • Enhanced analytical equations for disturbance modeling

BS ISO 17520:2024 history

  • 2024 BS ISO 17520:2024 Space environment (natural and artificial). Cosmic ray and solar energetic particle penetration inward the magnetosphere. Method of determination of the effective vertical cut-off rigidity
  • 2016 BS ISO 17520:2016 Space environment (natural and artificial). Cosmic ray and solar energetic particle penetration inward the magnetosphere. Method of determination of the effective vertical cut-off rigidity
Space environment (natural and artificial). Cosmic ray and solar energetic particle penetration inward the magnetosphere. Method of determination of the effective vertical cut-off rigidity

Standard and Specification

GSO ISO 17520:2021 Space environment (natural and artificial) — Cosmic ray and solar energetic particle penetration inward the magnetosphereMethod of determination of the effective vertical cut-off rigidity BS ISO 17520:2016 Space environment (natural and artificial). Cosmic ray and solar energetic particle penetration inward the magnetosphere. Method of determination of the effective vertical cut-off rigidity BH GSO ISO 17520:2022 Space environment (natural and artificial) — Cosmic ray and solar energetic particle penetration inward the magnetosphereMethod of determination of the effective vertical cut-off rigidity ISO 17520:2016 Space environment (natural and artificial) - Cosmic ray and solar energetic particle penetration inward the magnetosphere - Method of determination of the effective vertical cut-off rigidity ISO/DIS 17520:2023 Space environment (natural and artificial) — Cosmic ray and solar energetic particle penetration inward the magnetosphereMethod of determination of the effective vertical cut-off rigidity 23/30432825 DC environment (natural and artificial). Cosmic ray and solar energetic particle penetration inward the magnetosphere. Method of determination of the effective vertical cut-off rigidity ISO/TR 18147:2014 Space environment (natural and artificial) - Method of the solar energetic protons fluences and peak fluxes determination ISO 17520:2024 Space environment (natural and artificial GSO ISO/TR 18147:2021 Space environment (natural and artificial) — Method of the solar energetic protons fluences and peak fluxes determination



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