Horizontal flow below solar filaments

P. Ambrož; W. Pötzi

doi:10.1051/0004-6361/201731162

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Volume 613 (May 2018)

A&A, 613 (2018) A39

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Table A.1

Differential rotation coefficients.

Rotation profile	Coefficients (μrad s⁻¹)




	A	B	C
Magnetic, Snodgrass (1983)	2.890	−0.400	−0.434
Doppler, Snodgrass (1983)	2.857	−0.347	−0.477
Sunspots, Newton & Nunn (1951)	2.900	−0.598
LCT, k = 1.0	2.875	−0.147	−0.075
LCT, k = 3.8	2.901	−0.559	−0.285
F-Corona, Trellis (1957)	2.860	−0.452	0.063
F-Corona, Sýkora (1994)	2.898	−0.074
K-Corona, Fisher & Sime (1984)	2.870	−0.115

Notes. Selected coefficients of differential rotation for different height levels of the solar atmosphere. For comparison, we added the results of our measurements for a basic set of k = 1.0 and for the corrected factor k = 3.8.

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