group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
65 | 354 | 55 | 293 | -21.79 | 116.24 | 50.20 | 243.50 | 0.7967 | 435.7 | 377.0 |
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spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
11 | 34 | 12 | 37 | -19.70 | 127.89 | 61.86 | 248.72 | 0.8928 | -539.1 | -172.5 | |
0 | 1 | 0 | 1 | -19.73 | 120.05 | 54.01 | 247.19 | 0.8284 | -325.0 | -371.3 | |
5 | 16 | 4 | 14 | -19.99 | 119.75 | 53.71 | 246.81 | 0.8263 | -697.7 | -474.5 | |
5 | 12 | 4 | 10 | -19.29 | 119.27 | 53.23 | 247.53 | 0.8204 | -784.1 | -604.2 | |
0 | 4 | 0 | 4 | -19.71 | 118.98 | 52.94 | 246.95 | 0.8187 | -767.0 | -750.4 | |
0 | 2 | 0 | 2 | -20.01 | 118.91 | 52.88 | 246.58 | 0.8187 | -607.0 | -731.5 | |
0 | 2 | 0 | 2 | -21.52 | 118.76 | 52.73 | 244.74 | 0.8207 | 239.0 | 286.5 | |
0 | 4 | 0 | 3 | -21.77 | 116.89 | 50.86 | 243.91 | 0.8042 | 426.0 | 354.7 | |
0 | 3 | 0 | 3 | -21.31 | 114.96 | 48.92 | 243.88 | 0.7844 | 0.0 | 139.2 | |
0 | 4 | 0 | 4 | -21.90 | 115.03 | 49.00 | 243.18 | 0.7869 | -185.0 | -122.2 | |
0 | 3 | 0 | 3 | -22.66 | 115.00 | 48.97 | 242.24 | 0.7889 | 395.0 | 281.2 | |
2 | 9 | 2 | 7 | -21.49 | 114.40 | 48.36 | 243.48 | 0.7795 | 774.0 | 646.7 | |
0 | 4 | 0 | 3 | -22.20 | 114.72 | 48.69 | 242.71 | 0.7848 | 247.0 | 299.0 | |
7 | 256 | 6 | 200 | -22.30 | 114.00 | 47.96 | 242.34 | 0.7781 | 819.9 | 593.2 | |
8 | -14 | 6 | -14 | -21.93 | 113.58 | 47.54 | 242.65 | 0.7728 | 1221.1 | 999999 | |
27 | -14 | 21 | -14 | -22.89 | 113.83 | 47.79 | 241.55 | 0.7784 | 1288.7 | 999999 | |
-16 | -14 | -16 | -14 | -22.52 | 113.46 | 47.43 | 241.88 | 0.7736 | 999999 | 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. |