Detail publikace
Low Earth Orbit determination in small satellite mission proposal for corona observation of close solar surface region
BARTONĚK, J. LAZAR, V. MALANÍK, P. RYDLO, Š. LÁZNIČKA, T. POPELA, R. DRUCKMÜLLER, M.
Anglický název
Low Earth Orbit determination in small satellite mission proposal for corona observation of close solar surface region
Typ
článek v časopise ve Web of Science, Jimp
Jazyk
en
Originální abstrakt
A space-based observation of the solar corona is currently done in multiple wavelengths including visible, extreme-ultraviolet (EUV) and x-ray. White light coronagraph observations are restricted to regions beyond 1 RꙨ above the solar surface, while EUV remains blind above 0.25 RꙨ. White light corona images close to the solar surface limb may be documented during terrestrial total eclipse observations. These occur once in one to two years and are burdened with light scattering background caused by Earth's atmosphere. In this document, we propose a space-based small satellite mission which would have the advantage of performing white light corona observations under 2 RꙨ. The observation is done from Low Earth Orbit, utilizing the lunar limb to occult the solar disc during the artificial orbit-determined total eclipse. We present a list of the potential observation orbits, each with a single, yet unique observation opportunity. We extend the concurrent terrestrial options by finding extra space-based total eclipses. Observation requirements show that such a challenging mission would be achievable with the relatively affordable 6U CubeSat spacecraft.
Anglický abstrakt
A space-based observation of the solar corona is currently done in multiple wavelengths including visible, extreme-ultraviolet (EUV) and x-ray. White light coronagraph observations are restricted to regions beyond 1 RꙨ above the solar surface, while EUV remains blind above 0.25 RꙨ. White light corona images close to the solar surface limb may be documented during terrestrial total eclipse observations. These occur once in one to two years and are burdened with light scattering background caused by Earth's atmosphere. In this document, we propose a space-based small satellite mission which would have the advantage of performing white light corona observations under 2 RꙨ. The observation is done from Low Earth Orbit, utilizing the lunar limb to occult the solar disc during the artificial orbit-determined total eclipse. We present a list of the potential observation orbits, each with a single, yet unique observation opportunity. We extend the concurrent terrestrial options by finding extra space-based total eclipses. Observation requirements show that such a challenging mission would be achievable with the relatively affordable 6U CubeSat spacecraft.
Klíčová slova anglicky
Eclipses, Space mission, CubeSat, Orbital mechanics, Sun: corona
Vydáno
29.11.2022
ISSN
0094-5765
Ročník
203
Číslo
Feb. 2023
Strany od–do
202–213
Počet stran
12
BIBTEX
@article{BUT180427,
author="Jaroslav {Bartoněk} and Václav {Lazar} and Petr {Malaník} and Štěpán {Rydlo} and Tomáš {Láznička} and Robert {Popela} and Miloslav {Druckmüller},
title="Low Earth Orbit determination in small satellite mission proposal for corona observation of close solar surface region",
year="2022",
volume="203",
number="Feb. 2023",
month="November",
pages="202--213",
issn="0094-5765"
}