Imaging Polarimetry of Geostationary Satellite Express-AM5

This paper reports on the optical imaging polarimetry of geostationary satellite Express-AM5. Precise optical polarimetry was carried out using the Nayuta 2-m telescope at Nishi-Harima Astronomical Observatory and a polarimeter. V-band images were continuously taken in 312 minutes. The degree of pol...

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Main Authors: N. Kosaka, Yoichi Itoh, T. Saito, M. Tozuka, T. Endo, T. Ando
Format: Article
Language:English
Published: Odessa I. I. Mechnykov National University 2020-07-01
Series:Odessa Astronomical Publications
Subjects:
Online Access:http://oap.onu.edu.ua/article/view/207036
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author N. Kosaka
Yoichi Itoh
T. Saito
M. Tozuka
T. Endo
T. Ando
author_facet N. Kosaka
Yoichi Itoh
T. Saito
M. Tozuka
T. Endo
T. Ando
author_sort N. Kosaka
collection DOAJ
description This paper reports on the optical imaging polarimetry of geostationary satellite Express-AM5. Precise optical polarimetry was carried out using the Nayuta 2-m telescope at Nishi-Harima Astronomical Observatory and a polarimeter. V-band images were continuously taken in 312 minutes. The degree of polarization decreased with time until the minimum phase angle was reached at midnight, and then, it increased until morning. This change in the degree of polarization is well explained by the reflection of sunlight from monocrystalline solar panels of the satellite and possibly from other satellite components such as the antenna dishes and/or bus.
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spelling doaj.art-b800743eead44b6bada4ae978493d1a02022-12-21T22:33:34ZengOdessa I. I. Mechnykov National UniversityOdessa Astronomical Publications1810-42152020-07-0133011511810.18524/1810-4215.2020.33.207036207036Imaging Polarimetry of Geostationary Satellite Express-AM5N. Kosaka0Yoichi Itoh1T. SaitoM. TozukaT. EndoT. AndoNishi-Harima Astronomical Observatory, Center for Astronomy, University of HyogoNishi-Harima Astronomical Observatory, Center for Astronomy, University of HyogoThis paper reports on the optical imaging polarimetry of geostationary satellite Express-AM5. Precise optical polarimetry was carried out using the Nayuta 2-m telescope at Nishi-Harima Astronomical Observatory and a polarimeter. V-band images were continuously taken in 312 minutes. The degree of polarization decreased with time until the minimum phase angle was reached at midnight, and then, it increased until morning. This change in the degree of polarization is well explained by the reflection of sunlight from monocrystalline solar panels of the satellite and possibly from other satellite components such as the antenna dishes and/or bus.http://oap.onu.edu.ua/article/view/207036polarizationplanets and satellites: individualartificial satellite
spellingShingle N. Kosaka
Yoichi Itoh
T. Saito
M. Tozuka
T. Endo
T. Ando
Imaging Polarimetry of Geostationary Satellite Express-AM5
Odessa Astronomical Publications
polarization
planets and satellites: individual
artificial satellite
title Imaging Polarimetry of Geostationary Satellite Express-AM5
title_full Imaging Polarimetry of Geostationary Satellite Express-AM5
title_fullStr Imaging Polarimetry of Geostationary Satellite Express-AM5
title_full_unstemmed Imaging Polarimetry of Geostationary Satellite Express-AM5
title_short Imaging Polarimetry of Geostationary Satellite Express-AM5
title_sort imaging polarimetry of geostationary satellite express am5
topic polarization
planets and satellites: individual
artificial satellite
url http://oap.onu.edu.ua/article/view/207036
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AT mtozuka imagingpolarimetryofgeostationarysatelliteexpressam5
AT tendo imagingpolarimetryofgeostationarysatelliteexpressam5
AT tando imagingpolarimetryofgeostationarysatelliteexpressam5