The rotation axis of the Sun, as we know it today, was determined from the proper motion of sunspots by Carrington (1863). The solar axis is inclined toward the Ecliptic by an amount varying from +7o15’ to -7o15’. Furthermore, the position of solar axis is variable with respect to the north-south direction or respect to the great circle that passes through the celestial poles and the center of the Sun. This variation of the solar axis reaches the relatively large amount from +26o22’ to -26o22’. By table bellows we present day nottion B0 (heliographic latitude of the solar disk),
position angle of solar rotational axis from the north-south direction P0 and the longitude of center of solar disk L0.
The table data are calculated for 12:00 UT.
Recent comments
23 weeks 3 days ago
23 weeks 3 days ago
23 weeks 4 days ago
24 weeks 1 day ago
32 weeks 6 days ago
34 weeks 5 days ago
1 year 6 weeks ago
1 year 24 weeks ago
1 year 24 weeks ago
1 year 24 weeks ago