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  1. 学術雑誌論文
  2. 4 自然科学

Polarization Spectrum of Near-Infrared Zodiacal Light Observed with CIBER

http://hdl.handle.net/10228/00009072
http://hdl.handle.net/10228/00009072
7d287a9e-ae14-438e-aa23-444b2585f7ab
名前 / ファイル ライセンス アクション
LaSEINE-2021_038.pdf LaSEINE-2021_038.pdf (1.6 MB)
アイテムタイプ 学術雑誌論文 = Journal Article(1)
公開日 2023-02-03
資源タイプ
資源タイプ識別子 http://purl.org/coar/resource_type/c_6501
資源タイプ journal article
タイトル
タイトル Polarization Spectrum of Near-Infrared Zodiacal Light Observed with CIBER
言語 en
言語
言語 eng
著者 Takimoto, Kohji

× Takimoto, Kohji

WEKO 34634

en Takimoto, Kohji

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Arai, Toshiaki

× Arai, Toshiaki

WEKO 34635

en Arai, Toshiaki
Arai, T.

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Matsuura, Shuji

× Matsuura, Shuji

WEKO 34636

en Matsuura, Shuji
Matsuura, S.

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Bock, James J.

× Bock, James J.

WEKO 34637

en Bock, James J.
Bock, J.

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Cooray, Asantha

× Cooray, Asantha

WEKO 34638

en Cooray, Asantha
Cooray, A.

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Feder, Richard M.

× Feder, Richard M.

WEKO 34639

en Feder, Richard M.
Feder, R.

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Korngut, Phillip M.

× Korngut, Phillip M.

WEKO 34640

en Korngut, Phillip M.
Korngut, P.M.

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Lanz, Alicia

× Lanz, Alicia

WEKO 34641

en Lanz, Alicia
Lanz, A.

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Lee, Dae Hee

× Lee, Dae Hee

WEKO 34642

en Lee, Dae Hee
Lee, D.H.

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Matsumoto, Toshio

× Matsumoto, Toshio

WEKO 34643

en Matsumoto, Toshio
Matsumoto, T.

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Nguyen, Chi H.

× Nguyen, Chi H.

WEKO 34644

en Nguyen, Chi H.
Nguyen, C.

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Onishi, Yosuke

× Onishi, Yosuke

WEKO 34645

en Onishi, Yosuke
Onishi, Y.

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佐野, 圭

× 佐野, 圭

WEKO 31407
e-Rad 70802908
Scopus著者ID 56708069700
ORCiD 0000-0002-6468-8532
九工大研究者情報 100001400

en Sano, Kei

ja 佐野, 圭

ja-Kana サノ, ケイ


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Shirahata, Mai

× Shirahata, Mai

WEKO 34647

en Shirahata, Mai
Shirahata, M.

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Takahashi, Aoi

× Takahashi, Aoi

WEKO 34648

en Takahashi, Aoi
Takahashi, A.

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Tsumura, Kohji

× Tsumura, Kohji

WEKO 34649

en Tsumura, Kohji
Tsumura, K.

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Zemcov, Michael

× Zemcov, Michael

WEKO 34650

en Zemcov, Michael
Zemcov, M.

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抄録
内容記述タイプ Abstract
内容記述 We report the first measurement of the zodiacal light (ZL) polarization spectrum in the near-infrared between 0.8 and 1.8 μm. Using the low-resolution spectrometer on board the Cosmic Infrared Background Experiment, calibrated for absolute spectrophotometry and spectropolarimetry, we acquire long-slit polarization spectral images of the total diffuse sky brightness toward five fields. To extract the ZL spectrum, we subtract the contribution of other diffuse radiation, such as the diffuse galactic light, the integrated starlight, and the extragalactic background light. The measured ZL polarization spectrum shows little wavelength dependence in the near-infrared, and the degree of polarization clearly varies as a function of the ecliptic coordinates and solar elongation. Among the observed fields, the North Ecliptic Pole shows the maximum degree of polarization of ∼20%, which is consistent with an earlier observation from the Diffuse Infrared Background Experiment on board on the Cosmic Background Explorer. The measured degree of polarization and its solar elongation dependence are reproduced by an empirical scattering model in the visible band and also by a Mie scattering model for large absorptive particles, while a Rayleigh scattering model is ruled out. All of our results suggest that the interplanetary dust is dominated by large particles.
言語 en
書誌情報 en : Astrophysical Journal

巻 926, 号 1, p. 6-1-6-16, 発行日 2022-02-08
出版社
出版者 IOP Publishing
言語 en
DOI
関連タイプ isIdenticalTo
識別子タイプ DOI
関連識別子 https://doi.org/10.3847/1538-4357/ac416f
日本十進分類法
主題Scheme NDC
主題 440
ISSN
収録物識別子タイプ EISSN
収録物識別子 1538-4357
ISSN
収録物識別子タイプ PISSN
収録物識別子 0004-637X
著作権関連情報
権利情報Resource http://creativecommons.org/licenses/by/4.0/
権利情報 Copyright (c) 2022. The Author(s). Published by the American Astronomical Society. Original content from this work may be used under the terms of the Creative Commons Attribution 4.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI.
出版タイプ
出版タイプ VoR
出版タイプResource http://purl.org/coar/version/c_970fb48d4fbd8a85
査読の有無
値 yes
連携ID
値 10865
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