group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
103 | 627 | 84 | 522 | 16.54 | 268.50 | 48.84 | 296.18 | 0.8056 | -206.8 | 32.3 |
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spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
4 | 327 | 3 | 286 | 15.31 | 271.10 | 51.45 | 293.61 | 0.8255 | 1103.9 | 442.4 | |
20 | -1 | 17 | -1 | 16.34 | 271.09 | 51.43 | 294.80 | 0.8287 | 540.0 | 999999 | |
12 | -1 | 11 | -1 | 16.41 | 270.46 | 50.81 | 295.13 | 0.8234 | 1006.1 | 999999 | |
0 | 3 | 0 | 3 | 14.25 | 269.49 | 49.84 | 293.02 | 0.8070 | 299.0 | 269.6 | |
0 | 3 | 0 | 2 | 17.00 | 269.08 | 49.43 | 296.38 | 0.8131 | 207.0 | 268.0 | |
0 | 3 | 0 | 3 | 16.20 | 268.62 | 48.97 | 295.66 | 0.8059 | 491.0 | 428.0 | |
0 | 3 | 0 | 2 | 17.38 | 268.66 | 49.01 | 297.00 | 0.8107 | 285.0 | 341.6 | |
2 | 18 | 2 | 14 | 15.51 | 267.84 | 48.19 | 295.19 | 0.7960 | -268.3 | -15.6 | |
0 | 4 | 0 | 3 | 17.32 | 268.02 | 48.37 | 297.22 | 0.8046 | -23.0 | -72.1 | |
2 | 11 | 2 | 8 | 15.48 | 266.99 | 47.34 | 295.53 | 0.7877 | -265.8 | -208.8 | |
0 | 4 | 0 | 4 | 17.61 | 267.51 | 47.86 | 297.79 | 0.8011 | 276.0 | 267.7 | |
0 | 12 | 0 | 9 | 16.16 | 266.72 | 47.07 | 296.46 | 0.7878 | -187.0 | -49.3 | |
9 | 110 | 7 | 87 | 17.71 | 266.16 | 46.50 | 298.54 | 0.7889 | -314.1 | -415.6 | |
8 | 124 | 6 | 97 | 15.64 | 265.51 | 45.85 | 296.41 | 0.7738 | -925.8 | -758.2 | |
4 | -14 | 3 | -14 | 15.96 | 265.25 | 45.60 | 296.91 | 0.7726 | -1180.4 | 999999 | |
6 | -14 | 5 | -14 | 16.54 | 265.19 | 45.54 | 297.63 | 0.7746 | -670.7 | 999999 | |
8 | -14 | 6 | -14 | 16.91 | 264.67 | 45.02 | 298.34 | 0.7712 | -949.1 | 999999 | |
28 | -13 | 22 | -13 | 17.76 | 264.82 | 45.17 | 299.27 | 0.7765 | -910.2 | 999999 | |
-18 | -13 | -18 | -13 | 18.17 | 264.61 | 44.95 | 299.85 | 0.7763 | 999999 | 999999 | |
0 | 5 | 0 | 4 | 19.31 | 264.47 | 44.82 | 301.25 | 0.7804 | -481.0 | -443.6 |
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. |
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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. |
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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. |