Horizontal flow below solar filaments | Astronomy & Astrophysics (A&A)

Free Access

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.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.