Anton Reva, Sergey Kuzin, Andrey Pertsov, Alexey Kirichenko, Sergey Dyatkov, Ivan Loboda, Viktor Chervinsky, Anton Kholodilov, Alexey Trifonov, Sergey Bogachev, Sergei Chumak
{"title":"REFOS:纳米卫星上的太阳软x射线分光光度计","authors":"Anton Reva, Sergey Kuzin, Andrey Pertsov, Alexey Kirichenko, Sergey Dyatkov, Ivan Loboda, Viktor Chervinsky, Anton Kholodilov, Alexey Trifonov, Sergey Bogachev, Sergei Chumak","doi":"10.1007/s11207-025-02511-2","DOIUrl":null,"url":null,"abstract":"<div><p>In this work, we describe the design and flight performance of the REFOS instrument (from Russian <i>REntgenovskiy FOto Spektrometr</i>; in English “X-ray Photo Spectrometer”). REFOS is a soft X-ray spectrophotometer that registers full-disk integrated solar spectra (“Sun as a star”). It operates on board the <i>Impulse-1</i> nanosatellite, which was launched on 24 June 2023. REFOS has a 1.2 – 30 keV spectral range, a 0.123 keV nominal full width at half-maximum (FWHM) resolution at 5.9 keV, and a cadence of 16 s. We illustrate the instrument flight performance using the spectra of the X5.0 flare that occurred on 31 December 2023 at 21:55 UT. For this flare, REFOS registered a meaningful signal in all of its energy bins. Based on a comparison between the GOES and REFOS fluxes, we corrected the REFOS spectral sensitivity. Additionally, we assessed the quality of the calibration based on the shape of the continuum. The observed continuum allows diagnosing the plasma temperature, and the observed spectral lines allow studying abundances of the Mg, Si, S, Ar, Ca, Fe, and Ni.</p></div>","PeriodicalId":777,"journal":{"name":"Solar Physics","volume":"300 7","pages":""},"PeriodicalIF":2.4000,"publicationDate":"2025-07-16","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"REFOS: Solar Soft X-ray Spectrophotometer on Board Nanosatellite\",\"authors\":\"Anton Reva, Sergey Kuzin, Andrey Pertsov, Alexey Kirichenko, Sergey Dyatkov, Ivan Loboda, Viktor Chervinsky, Anton Kholodilov, Alexey Trifonov, Sergey Bogachev, Sergei Chumak\",\"doi\":\"10.1007/s11207-025-02511-2\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>In this work, we describe the design and flight performance of the REFOS instrument (from Russian <i>REntgenovskiy FOto Spektrometr</i>; in English “X-ray Photo Spectrometer”). REFOS is a soft X-ray spectrophotometer that registers full-disk integrated solar spectra (“Sun as a star”). It operates on board the <i>Impulse-1</i> nanosatellite, which was launched on 24 June 2023. REFOS has a 1.2 – 30 keV spectral range, a 0.123 keV nominal full width at half-maximum (FWHM) resolution at 5.9 keV, and a cadence of 16 s. We illustrate the instrument flight performance using the spectra of the X5.0 flare that occurred on 31 December 2023 at 21:55 UT. For this flare, REFOS registered a meaningful signal in all of its energy bins. Based on a comparison between the GOES and REFOS fluxes, we corrected the REFOS spectral sensitivity. Additionally, we assessed the quality of the calibration based on the shape of the continuum. The observed continuum allows diagnosing the plasma temperature, and the observed spectral lines allow studying abundances of the Mg, Si, S, Ar, Ca, Fe, and Ni.</p></div>\",\"PeriodicalId\":777,\"journal\":{\"name\":\"Solar Physics\",\"volume\":\"300 7\",\"pages\":\"\"},\"PeriodicalIF\":2.4000,\"publicationDate\":\"2025-07-16\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Solar Physics\",\"FirstCategoryId\":\"101\",\"ListUrlMain\":\"https://link.springer.com/article/10.1007/s11207-025-02511-2\",\"RegionNum\":3,\"RegionCategory\":\"物理与天体物理\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q2\",\"JCRName\":\"ASTRONOMY & ASTROPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Solar Physics","FirstCategoryId":"101","ListUrlMain":"https://link.springer.com/article/10.1007/s11207-025-02511-2","RegionNum":3,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
REFOS: Solar Soft X-ray Spectrophotometer on Board Nanosatellite
In this work, we describe the design and flight performance of the REFOS instrument (from Russian REntgenovskiy FOto Spektrometr; in English “X-ray Photo Spectrometer”). REFOS is a soft X-ray spectrophotometer that registers full-disk integrated solar spectra (“Sun as a star”). It operates on board the Impulse-1 nanosatellite, which was launched on 24 June 2023. REFOS has a 1.2 – 30 keV spectral range, a 0.123 keV nominal full width at half-maximum (FWHM) resolution at 5.9 keV, and a cadence of 16 s. We illustrate the instrument flight performance using the spectra of the X5.0 flare that occurred on 31 December 2023 at 21:55 UT. For this flare, REFOS registered a meaningful signal in all of its energy bins. Based on a comparison between the GOES and REFOS fluxes, we corrected the REFOS spectral sensitivity. Additionally, we assessed the quality of the calibration based on the shape of the continuum. The observed continuum allows diagnosing the plasma temperature, and the observed spectral lines allow studying abundances of the Mg, Si, S, Ar, Ca, Fe, and Ni.
期刊介绍:
Solar Physics was founded in 1967 and is the principal journal for the publication of the results of fundamental research on the Sun. The journal treats all aspects of solar physics, ranging from the internal structure of the Sun and its evolution to the outer corona and solar wind in interplanetary space. Papers on solar-terrestrial physics and on stellar research are also published when their results have a direct bearing on our understanding of the Sun.