group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
83 | 480 | 60 | 344 | -13.98 | 269.42 | 46.74 | 256.77 | 0.7277 | 421.6 | -11.3 |
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 |
0 | 3 | 0 | 2 | -14.27 | 276.14 | 53.46 | 256.98 | 0.8014 | -497.0 | -416.7 | |
0 | 5 | 0 | 4 | -14.25 | 274.60 | 51.92 | 256.91 | 0.7856 | -694.0 | -502.1 | |
18 | 204 | 14 | 154 | -13.05 | 271.97 | 49.28 | 258.30 | 0.7564 | -1102.7 | -502.2 | |
0 | 2 | 0 | 2 | -13.31 | 270.76 | 48.08 | 257.87 | 0.7429 | -584.0 | -544.2 | |
0 | 2 | 0 | 1 | -14.32 | 270.98 | 48.29 | 256.53 | 0.7462 | -408.0 | -447.2 | |
2 | -3 | 2 | -3 | -13.38 | 270.36 | 47.68 | 257.74 | 0.7384 | -846.0 | 999999 | |
5 | 54 | 3 | 38 | -14.16 | 269.03 | 46.35 | 256.55 | 0.7237 | 498.6 | -325.2 | |
3 | -7 | 2 | -7 | -13.99 | 268.70 | 46.02 | 256.75 | 0.7196 | -418.3 | 999999 | |
0 | 5 | 0 | 3 | -14.92 | 267.91 | 45.23 | 255.35 | 0.7114 | 150.0 | 192.0 | |
0 | 6 | 0 | 4 | -15.53 | 267.73 | 45.05 | 254.47 | 0.7101 | 503.0 | 385.0 | |
8 | 197 | 6 | 135 | -14.25 | 267.34 | 44.65 | 256.22 | 0.7037 | 559.4 | 648.5 | |
13 | -11 | 9 | -11 | -14.71 | 267.06 | 44.37 | 255.53 | 0.7009 | 1097.8 | 999999 | |
0 | 2 | 0 | 1 | -15.70 | 267.10 | 44.41 | 254.13 | 0.7028 | 535.0 | 535.0 | |
25 | -11 | 17 | -11 | -15.02 | 266.63 | 43.95 | 255.02 | 0.6962 | 1225.6 | 999999 | |
5 | -11 | 4 | -11 | -15.18 | 266.11 | 43.43 | 254.71 | 0.6902 | 1308.4 | 999999 | |
4 | -11 | 3 | -11 | -15.33 | 265.65 | 42.97 | 254.41 | 0.6848 | 1083.6 | 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. |