group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
112 | 549 | 85 | 427 | 16.35 | 268.13 | 45.45 | 297.52 | 0.7728 | -8.9 | 67.7 |
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-04-02 23:59:33 UT |
spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
24 | 258 | 19 | 209 | 15.51 | 270.51 | 47.82 | 295.36 | 0.7925 | 1057.2 | 556.7 | |
23 | -1 | 19 | -1 | 16.32 | 270.70 | 48.02 | 296.22 | 0.7975 | 791.2 | 999999 | |
0 | 7 | 0 | 5 | 14.28 | 269.61 | 46.93 | 294.29 | 0.7790 | 702.0 | 244.7 | |
5 | -1 | 4 | -1 | 16.81 | 269.60 | 46.92 | 297.30 | 0.7891 | 580.3 | 999999 | |
5 | 15 | 4 | 12 | 15.49 | 268.31 | 45.63 | 296.35 | 0.7710 | 84.3 | 219.6 | |
0 | 4 | 0 | 3 | 15.99 | 268.34 | 45.66 | 296.93 | 0.7735 | 535.0 | 476.3 | |
0 | 4 | 0 | 3 | 16.59 | 268.53 | 45.84 | 297.56 | 0.7779 | 391.0 | 369.9 | |
0 | 29 | 0 | 22 | 15.50 | 267.40 | 44.71 | 296.80 | 0.7619 | 156.0 | -62.6 | |
0 | 4 | 0 | 3 | 16.29 | 266.94 | 44.26 | 298.00 | 0.7609 | 37.0 | 64.7 | |
0 | 9 | 0 | 7 | 16.01 | 266.46 | 43.78 | 297.89 | 0.7548 | -488.0 | -309.0 | |
0 | 18 | 0 | 14 | 17.59 | 266.30 | 43.62 | 299.88 | 0.7607 | -261.0 | -58.3 | |
3 | 70 | 2 | 52 | 16.11 | 265.71 | 43.03 | 298.42 | 0.7477 | -520.4 | -718.6 | |
7 | -12 | 5 | -12 | 15.80 | 265.46 | 42.78 | 298.17 | 0.7436 | -1033.3 | 999999 | |
8 | -12 | 6 | -12 | 16.38 | 265.40 | 42.71 | 298.91 | 0.7458 | -686.1 | 999999 | |
25 | 93 | 18 | 69 | 17.73 | 265.00 | 42.32 | 300.77 | 0.7487 | -1064.0 | -423.7 | |
12 | 38 | 8 | 28 | 16.83 | 264.69 | 42.01 | 299.85 | 0.7409 | -1160.4 | -824.2 |
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. |