We have estimated the radial gradient of angular velocity in the near subsurface layers of the sun for the period 07/2001-07/2007 which covers 80 Carrington rotations, starts at the maximum of cycle 23 and ends at its minimum. This analysis confirms that, on average, the radial gradient of angular velocity remains negative and roughly constant...
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August 1, 2008 (v1)Conference paperUploaded on: December 4, 2022
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2009 (v1)Journal article
Astrophysics and Space Science, p. 200 (2009)
Uploaded on: December 3, 2022 -
2009 (v1)Journal article
Astronomy and Astrophysics, 504, pp. 589-594 (2009)
Uploaded on: December 4, 2022 -
2007 (v1)Journal article
Astronomy and Astrophysics, 469, pp. 1145-1149, http://dx.doi.org./10.1051/0004-6361:7212
Uploaded on: December 3, 2022 -
2006 (v1)Journal article
Solar Physics, 236, pp. 227-244, http://dx.doi.org./10.1007/s11207-006-0106-5
Uploaded on: December 4, 2022 -
August 20, 2007 (v1)Conference paper
Mapping the solar surface is a crucial step in any local helioseismology technique. Because the acoustic waves propagate along great circles at the solar surface, it has been shown that these circles need to be used in the geometrical construction of the plane grid. We study different types of projections based on great circles for the...
Uploaded on: December 4, 2022