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A Statistical Inference Method for Interpreting the CLASP Observations

delete2018-09-20
delete4
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OA
AI
J
Jiří Štěpán *
J
J. Trujillo Bueno
B
Belluzzi, L.
A
Asensio Ramos, A.
S
Sainz, R. Manso
D
del Pino Aleman, T.
R
R. Casini
R
Ryouhei Kano
A
Amy R. Winebarger
A
Aucherer, F.
I
Ishikawa, R.
N
Narukage, N.
K
Kobayashi, K.
B
Bando, T.
Y
Yukio Katsukawa
K
Kubo, M.
I
Ishikawa, S.
G
Giono, G.
H
Hara, H.
Y
Y. Suematsu
S
Shimizu, T.
S
Sakao, T.
T
Tsuneta, S.
K
Kiyoshi Ichimoto
J
Jonathan Cirtain
P
Patrick Champey
D
De Pontieu, B.
M
M. Carlsson
DOI：10.3847/1538-4357/aad910delete
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摘要

摘要

En 中文
On 2015 September 3, the Chromospheric Lyman-Alpha SpectroPolarimeter (CLASP) successfully measured the linear polarization produced by scattering processes in the hydrogen Ly alpha line of the solar disk radiation, revealing conspicuous spatial variations in the Q/I and U/I signals. Via the Hanle effect, the line-center Q/I and U/I amplitudes encode information on the magnetic field of the chromosphere-corona transition region, but they are also sensitive to the three-dimensional structure of this corrugated interface region. With the help of a simple line-formation model, here we propose a statistical inference method for interpreting the Ly alpha line-center polarization observed by CLASP.
Keyword:
methods: statistical
polarization
radiative transfer
Sun: chromosphere
Sun: transition region
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期刊

Astrophysical Journal 封面图
Astrophysical Journal
IF:
5.4
论文数:
8.3W
被引数:
32.0W

机构

K
kiepenheuer institut fur sonnenphysik
学者数:
140
论文数: 184
被引数: 0
N
national center atmospheric research (ncar) - usa
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被引数: 8
C
centre national de la recherche scientifique (cnrs)
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N
national institutes of natural sciences (nins) - japan
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C
consejo superior de investigaciones cientificas (csic)
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N
national aeronautics & space administration (nasa)
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C
czech academy of sciences
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3.4W
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M
Max Planck Society
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national astronomical observatory of japan (naoj)
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4.1K
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被引数: 3
U
Universite Paris Saclay
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被引数: 540
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