SOLar-STellar Irradiance Comparison Experiment II (SOLSTICE II): End-of-Mission Validation of the SOLSTICE Technique

被引:10
|
作者
Snow, Martin [1 ,2 ,3 ]
McClintock, William E. [1 ]
Woods, Thomas N. [1 ]
Elliott, Joshua P. [1 ]
机构
[1] Univ Colorado, Lab Atmospher & Space Phys, 1234 Innovation Dr, Boulder, CO 80303 USA
[2] South African Natl Space Agcy, Hosp St, ZA-7200 Hermanus, South Africa
[3] Univ Western Cape, Dept Phys & Astron, Robert Sobukwe Rd, ZA-7535 Bellville, South Africa
基金
新加坡国家研究基金会;
关键词
Chromosphere; Instrumentation and data management; Integrated Sun observations; Solar irradiance; SPECTRAL IRRADIANCE; ABSOLUTE CALIBRATION; UV VARIATIONS; MONITOR; NM; VARIABILITY;
D O I
10.1007/s11207-022-01984-9
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The SOLar-STellar Irradiance Comparison Experiment (SOLSTICE: McClintock, Rottman, and Woods, Solar Phys. 230, 225, 2005) onboard the SOlar Radiation and Climate Experiment (SORCE: Rottman, Solar Phys. 230, 7, 2005) observed ultraviolet solar spectral irradiance (SSI) from 2003 - 2020. This article gives an overview of the end-of-mission algorithms and calibration of SOLSTICE. Many of the algorithms were updated after the early mission, either due to an improved understanding of the instrument and the space environment, or due to operational constraints as the spacecraft systems aged. We validate the final official data version (V18) with comparisons to other observations and models. The SOLSTICE observations of the solar-cycle variability in the ultraviolet are compared to model estimates.
引用
收藏
页数:30
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