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Observations From NOAA's Newest Solar Proton Sensor
Space Weather ( IF 3.8 ) Pub Date : 2021-07-17 , DOI: 10.1029/2021sw002750
B. T. Kress 1, 2 , J. V. Rodriguez 1, 3 , A. Boudouridis 1, 2 , T. G. Onsager 4 , B. K. Dichter 5 , G. E. Galica 5 , S. Tsui 5
Affiliation  

Space weather instrumentation on board the National Oceanic and Atmospheric Administration's (NOAA's) newest Geostationary Operational Environmental Satellite (GOES)-R series includes the Solar and Galactic Proton Sensor (SGPS), which has been collecting data since January 8, 2017. SGPS supports real-time alerts of solar energetic particle events at the NOAA Space Weather Prediction Center (SWPC) and provides data to the space science community, advancing basic space science research and understanding of space weather effects on satellite systems. The first GOES-R series spacecraft, GOES-16, was launched on November 19, 2016. A series of solar particle events in September 2017 enabled cross-calibration of GOES-16 SGPS with the Energetic Particle Sensors on GOES-13 and -15. This paper is intended as a resource for SGPS data users, including comparisons with legacy GOES energetic particle measurements, corrections applied to SGPS Level-2 data, important caveats, background level fluxes, and measurements of trapped magnetospheric protons.

中文翻译:

NOAA 最新太阳质子传感器的观测结果

美国国家海洋和大气管理局 (NOAA) 最新的地球静止运行环境卫星 (GOES)-R 系列上的空间天气仪器包括太阳和银河质子传感器 (SGPS),自 2017 年 1 月 8 日以来一直在收集数据。 SGPS 支持真实- NOAA 空间天气预报中心 (SWPC) 的太阳高能粒子事件时间警报,并向空间科学界提供数据,推进基础空间科学研究和了解空间天气对卫星系统的影响。第一个 GOES-R 系列航天器 GOES-16 于 2016 年 11 月 19 日发射。 2017 年 9 月的一系列太阳粒子事件使 GOES-16 SGPS 与 GOES-13 和 -15 上的高能粒子传感器进行交叉校准. 本文旨在作为 SGPS 数据用户的资源,
更新日期:2021-07-17
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