group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
67 | 367 | 55 | 292 | -21.73 | 116.53 | 48.73 | 243.09 | 0.7824 | 411.7 | 397.5 |
previous
or next observation for the same group /
back to the solar disc SOHO MDI 1999-05-23 09:35:33 UT ![]() |
spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
13 | 40 | 13 | 41 | -19.71 | 127.92 | 60.12 | 248.44 | 0.8797 | -553.0 | -141.6 | |
0 | 4 | 0 | 3 | -19.78 | 120.01 | 52.22 | 246.70 | 0.8119 | -365.0 | -416.5 | |
6 | 16 | 5 | 14 | -20.04 | 119.72 | 51.92 | 246.31 | 0.8098 | -721.8 | -502.3 | |
5 | 13 | 4 | 11 | -19.43 | 119.11 | 51.31 | 246.89 | 0.8025 | -945.6 | -764.5 | |
0 | 4 | 0 | 3 | -19.97 | 118.95 | 51.15 | 246.19 | 0.8023 | -728.0 | -746.6 | |
0 | 3 | 0 | 2 | -19.73 | 118.70 | 50.91 | 246.42 | 0.7994 | -625.0 | -550.9 | |
0 | 3 | 0 | 3 | -21.52 | 118.81 | 51.01 | 244.27 | 0.8049 | 528.0 | 372.5 | |
0 | 4 | 0 | 3 | -21.73 | 116.92 | 49.12 | 243.43 | 0.7875 | 598.0 | 448.6 | |
0 | 1 | 0 | 0 | -20.12 | 115.83 | 48.03 | 245.08 | 0.7721 | 422.0 | 422.0 | |
0 | 2 | 0 | 1 | -20.87 | 115.89 | 48.09 | 244.16 | 0.7749 | 547.0 | 447.6 | |
0 | 10 | 0 | 8 | -21.94 | 115.16 | 47.36 | 242.59 | 0.7709 | -28.0 | -18.7 | |
0 | 7 | 0 | 6 | -22.66 | 115.10 | 47.30 | 241.67 | 0.7728 | 160.0 | 169.8 | |
1 | 6 | 1 | 5 | -22.07 | 114.78 | 46.98 | 242.28 | 0.7676 | 495.5 | 420.4 | |
0 | 11 | 0 | 8 | -21.53 | 114.42 | 46.62 | 242.83 | 0.7623 | 768.0 | 684.0 | |
7 | 243 | 5 | 184 | -22.21 | 114.09 | 46.29 | 241.86 | 0.7613 | 882.7 | 665.9 | |
6 | -15 | 5 | -15 | -21.93 | 113.60 | 45.80 | 242.03 | 0.7554 | 1262.4 | 999999 | |
13 | -15 | 10 | -15 | -22.90 | 113.83 | 46.03 | 240.90 | 0.7611 | 973.6 | 999999 | |
16 | -15 | 12 | -15 | -22.52 | 113.43 | 45.63 | 241.21 | 0.7557 | 1592.4 | 999999 |
Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
that the umbra consists of fragmented regions which cannot be separated without losing umbral area. In this way several spots (intensity minima in the umbra) have a common umbra, e.g. -2 means that the given spot shares an umbra with spot No.2, and the common U value is indicated at spot No.2. |
||
Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
that several umbras have a common penumbra, e.g. -7 means that the given umbra shares a penumbra with umbra No.7, and the WS value is indicated at No.7. |
||
Corr. U | - Corrected umbra area in millionths of solar hemisphere, for negative values see above | |
Corr. WS | - Corrected whole spot area in millionths of solar hemisphere, for negative values see above | |
B | - Heliographic latitude B; positive: North, negative: South | |
L | - Heliographic longitude L | |
LCM | - Longitudinal distance from the Sun's central meridian | |
Pos. angle | - Position angle | |
r | - Distance from the centre of Sun's disc in terms of Sun's radius | |
MU | - Mean magnetic field within the umbra contour averaged the pixel values with sign. | |
MP | - Mean magnetic field within the penumbra contour averaged the pixel values with sign. |