group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
94 | 532 | 52 | 290 | 20.37 | 281.99 | -14.66 | 35.42 | 0.4099 | 426.0 | 165.0 |
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spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
8 | 296 | 5 | 160 | 20.06 | 283.80 | -12.84 | 32.67 | 0.3886 | 1682.7 | 621.3 | |
42 | -1 | 23 | -1 | 20.67 | 283.71 | -12.94 | 31.96 | 0.3975 | 1593.0 | 999999 | |
5 | 41 | 3 | 22 | 19.33 | 282.90 | -13.74 | 35.55 | 0.3873 | 463.5 | 261.6 | |
0 | 5 | 0 | 3 | 20.33 | 281.63 | -15.01 | 36.32 | 0.4119 | -87.0 | -341.3 | |
0 | 5 | 0 | 3 | 18.72 | 281.75 | -14.90 | 38.74 | 0.3910 | -180.0 | -132.2 | |
0 | 19 | 0 | 10 | 20.09 | 281.02 | -15.62 | 37.78 | 0.4147 | -161.0 | -265.1 | |
0 | 4 | 0 | 2 | 16.71 | 281.00 | -15.64 | 43.71 | 0.3755 | 323.0 | 488.0 | |
0 | 5 | 0 | 3 | 18.47 | 280.76 | -15.89 | 40.91 | 0.3982 | -663.0 | -394.8 | |
0 | 15 | 0 | 8 | 20.33 | 280.36 | -16.29 | 38.52 | 0.4241 | -680.0 | -536.6 | |
0 | 9 | 0 | 5 | 18.67 | 280.11 | -16.54 | 41.67 | 0.4074 | -741.0 | -534.8 | |
0 | 7 | 0 | 4 | 19.03 | 279.35 | -17.29 | 42.28 | 0.4195 | -639.0 | -540.8 | |
14 | 115 | 8 | 64 | 20.48 | 278.98 | -17.67 | 40.49 | 0.4399 | -1243.3 | -619.8 | |
4 | -12 | 2 | -12 | 19.87 | 278.88 | -17.77 | 41.62 | 0.4340 | -693.8 | 999999 | |
8 | -12 | 4 | -12 | 20.68 | 278.48 | -18.17 | 40.93 | 0.4472 | -1264.6 | 999999 | |
13 | -12 | 7 | -12 | 21.05 | 278.30 | -18.35 | 40.62 | 0.4531 | -880.1 | 999999 | |
0 | 5 | 0 | 3 | 21.25 | 276.97 | -19.68 | 42.22 | 0.4690 | -832.0 | -739.9 | |
0 | 6 | 0 | 3 | 22.96 | 275.92 | -20.73 | 41.07 | 0.4981 | -774.0 | -669.4 |
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. |