A statistical inference method for interpreting the CLASP observations
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.
document
http://n2t.net/ark:/85065/d70c4zp0
eng
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publication
2016-01-01T00:00:00Z
publication
2018-09-20T00:00:00Z
Copyright 2018 The American Astronomical Society.
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