Partial Frequency Redistribution is a radiative transfer model in solar chromospheric physics that describes the scattering of spectral lines where the absorbed and re-emitted photons are partially correlated in frequency due to the finite width of atomic energy levels and thermal motions, distinguishing it from complete redistribution by retaining a memory of the incident radiation field.
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Tiago M. D. Pereira, H. Uitenbroek · Springer Link (Chiba Institute of Technology) · 2015 · 95 citations · Full text
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Indian Institute of Astrophysics
Bengaluru, India
14 h-index
45 publications
913 citations
Istituto Ricerche Solari Locarno
Locarno, Switzerland
12 h-index
25 publications
509 citations
Instituto de Astrofísica de Canarias
Tenerife, Spain
11 h-index
24 publications
656 citations
Universidad de La Laguna
San Cristóbal de La Laguna, Spain
11 h-index
19 publications
578 citations
Consejo Superior de Investigaciones Científicas
Madrid, Spain
10 h-index
10 publications
280 citations
ETH Zurich
Zurich, Switzerland
10 h-index
14 publications
285 citations
Centre National de la Recherche Scientifique
Paris, France
8 h-index
14 publications
350 citations
National Solar Observatory
Boulder, United States
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5 publications
752 citations
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ApJ · 46 publications · 1.7K citations
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Repository · 3 publications · 134 citations
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- Journal of Quantitative Spectroscopy and Radiative Transfer
JQSRT · 3 publications · 208 citations
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- Physical Review A
PRA · 3 publications · 81 citations
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