Capabilities of the Sun-Terahertz Scientific Instrumentation Detectors in Registering Solar Radiation: Preliminary Evaluation from the Ground-Based Data

The paper describes the Sun-Terahertz space experiment planned for 2025–2027 onboard the Russian segment of the International Space Station (ISS). The main goals of the experiment are to obtain information on the terahertz radiation of the Sun, as well as to study active regions and solar flares. The scientific instrumentation of the Sun-Terahertz experiment contains eight channels (detectors) sensitive to radiation in a frequency range of 0.4–12.0 THz. The purpose of this study is to estimate the voltage at the output of scientific instrumentation detectors during the ISS onboard experiment from the ground-based measurement data and to determine minimal increases in the radiation flux reliably registered by the scientific instrumentation against the background of inherent noises.

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Publication Details

Journal
Solar System Research
Published
2025-11-10
DOI
https://doi.org/10.1134/s0038094625600635
Primary Topic
Solar and Space Plasma Dynamics
Type
article
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article

Capabilities of the Sun-Terahertz Scientific Instrumentation Detectors in Registering Solar Radiation: Preliminary Evaluation from the Ground-Based Data

В. С. Махмутов, Г. И. Кропотов, С. В. Соков, M. V. Razumeyko et al.
Solar System Research
Solar and Space Plasma Dynamics
article

Capabilities of the Sun-Terahertz Scientific Instrumentation Detectors in Registering Solar Radiation: Preliminary Evaluation from the Ground-Based Data

В. С. Махмутов, Г. И. Кропотов, С. В. Соков, M. V. Razumeyko, Maxim Philippov, E. D. Tulnikov
article en

Abstract

The paper describes the Sun-Terahertz space experiment planned for 2025–2027 onboard the Russian segment of the International Space Station (ISS). The main goals of the experiment are to obtain information on the terahertz radiation of the Sun, as well as to study active regions and solar flares. The scientific instrumentation of the Sun-Terahertz experiment contains eight channels (detectors) sensitive to radiation in a frequency range of 0.4–12.0 THz. The purpose of this study is to estimate the voltage at the output of scientific instrumentation detectors during the ISS onboard experiment from the ground-based measurement data and to determine minimal increases in the radiation flux reliably registered by the scientific instrumentation against the background of inherent noises.

Solar System ResearchVol. 59(7)
P.N. Lebedev Physical Institute of the Russian Academy of Sciences (RU)
Openalex Percentile: Top 77%
Solar and Space Plasma Dynamics
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