group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
90 | 575 | 60 | 406 | 28.04 | 108.95 | 42.26 | 303.37 | 0.7098 | 202.9 | 132.7 |
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spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
26 | 252 | 20 | 191 | 26.38 | 115.02 | 48.33 | 298.63 | 0.7648 | 814.4 | 375.4 | |
10 | -1 | 7 | -1 | 26.56 | 113.88 | 47.19 | 299.20 | 0.7541 | 876.9 | 999999 | |
3 | -1 | 2 | -1 | 26.54 | 113.16 | 46.47 | 299.39 | 0.7468 | 901.9 | 999999 | |
9 | 18 | 6 | 13 | 27.62 | 110.46 | 43.77 | 301.73 | 0.7230 | 582.8 | 444.0 | |
0 | 7 | 0 | 5 | 26.82 | 108.28 | 41.59 | 301.52 | 0.6972 | 435.0 | 413.2 | |
7 | 29 | 5 | 20 | 28.06 | 108.73 | 42.05 | 303.00 | 0.7070 | 521.5 | 277.1 | |
0 | 6 | 0 | 4 | 28.73 | 108.88 | 42.20 | 303.83 | 0.7114 | -317.0 | -159.3 | |
0 | 5 | 0 | 4 | 29.68 | 107.73 | 41.05 | 305.60 | 0.7039 | -212.0 | -200.0 | |
0 | 8 | 0 | 6 | 28.87 | 105.99 | 39.30 | 305.34 | 0.6823 | 189.0 | 239.6 | |
0 | 24 | 0 | 16 | 29.67 | 106.30 | 39.61 | 306.26 | 0.6894 | 697.0 | 687.4 | |
1 | 45 | 0 | 30 | 28.85 | 105.12 | 38.43 | 305.75 | 0.6731 | 806.3 | 402.6 | |
1 | -11 | 0 | -11 | 29.17 | 104.29 | 37.60 | 306.63 | 0.6661 | -34.0 | 999999 | |
0 | 3 | 0 | 2 | 30.34 | 103.60 | 36.91 | 308.60 | 0.6656 | 281.0 | 233.1 | |
1 | 178 | 0 | 115 | 30.01 | 101.55 | 34.87 | 309.37 | 0.6427 | -578.7 | -476.1 | |
9 | -14 | 6 | -14 | 29.38 | 101.25 | 34.56 | 308.70 | 0.6357 | -937.4 | 999999 | |
19 | -14 | 12 | -14 | 30.54 | 101.27 | 34.59 | 310.29 | 0.6432 | -887.0 | 999999 | |
4 | -14 | 2 | -14 | 30.34 | 100.48 | 33.79 | 310.53 | 0.6338 | -848.5 | 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. |
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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. |