Polarimetry of Saturnian satellite Enceladus

Домашня сторінка
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Фізико-технічні та математичні науки
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Відділення фізики і астрономії
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Advances in Astronomy and Space Physics
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Advances in Astronomy and Space Physics, 2015, том 5
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Advances in Astronomy and Space Physics, 2015, вип. 1
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dc.contributor.author	Zaitsev, S.V.
dc.contributor.author	Kiselev, N.N.
dc.contributor.author	Rosenbush, V.K.
dc.contributor.author	Kolesnikov, S.V.
dc.contributor.author	Shakhovskoy, D.N.
dc.date.accessioned	2017-06-09T20:51:13Z
dc.date.available	2017-06-09T20:51:13Z
dc.date.issued	2015
dc.identifier.citation	Polarimetry of Saturnian satellite Enceladus / S.V. Zaitsev, N.N. Kiselev, V.K. Rosenbush, S.V. Kolesnikov, D.N. Shakhovskoy // Advances in Astronomy and Space Physics. — 2015. — Т. 5., вип. 1. — С. 29-32. — Бібліогр.: 32 назв. — англ.	uk_UA
dc.identifier.issn	2227-1481
dc.identifier.other	DOI: 10.17721/2227-1481.5.29-32
dc.identifier.uri	http://dspace.nbuv.gov.ua/handle/123456789/119822
dc.description.abstract	We present results of polarimetric observations of Saturn's moon Enceladus carried out from April 14, 2010 to April 13, 2013 in WR spectral band (550-750 nm). We used 2.6-m telescope equipped with a one-channel photoelectric photometer-polarimeter (Crimean Astrophysical Observatory). The measurements were performed at phase angles ranging from 1.65° to 5.71°. The phase-angle dependence of linear polarization of Enceladus was obtained using the results of our observations. Results obtained are discussed in terms of existing models of light scattering by regolith surfaces.	uk_UA
dc.language.iso	en	uk_UA
dc.publisher	Головна астрономічна обсерваторія НАН України	uk_UA
dc.relation.ispartof	Advances in Astronomy and Space Physics
dc.title	Polarimetry of Saturnian satellite Enceladus	uk_UA
dc.type	Article	uk_UA
dc.status	published earlier	uk_UA