group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
14.66 | 39.29 | 7.44 | 20.10 | -3.93 | 159.24 | -11.20 | 128.42 | 0.2455 | 761.0 | 525.1 |
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spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
10.41 | 23.42 | 5.28 | 11.88 | -3.52 | 161.13 | -9.31 | 131.13 | 0.2153 | 1265.9 | 673.0 | |
4.25 | -1.00 | 2.16 | -1.00 | -3.58 | 160.92 | -9.52 | 130.70 | 0.2187 | 1036.2 | 999999 | |
0.00 | 1.13 | 0.00 | 0.57 | -1.30 | 160.61 | -9.83 | 120.98 | 0.2000 | 921.0 | 739.0 | |
0.00 | 0.95 | 0.00 | 0.48 | -1.88 | 160.24 | -10.20 | 122.41 | 0.2106 | 733.0 | 639.0 | |
0.00 | 1.30 | 0.00 | 0.66 | -4.53 | 159.57 | -10.87 | 130.07 | 0.2467 | 987.0 | 813.5 | |
0.00 | 1.47 | 0.00 | 0.76 | -5.22 | 159.53 | -10.91 | 132.05 | 0.2550 | 793.0 | 563.5 | |
0.00 | 1.82 | 0.00 | 0.93 | -4.32 | 159.49 | -10.95 | 129.18 | 0.2455 | 1064.0 | 840.2 | |
0.00 | 1.04 | 0.00 | 0.53 | -2.85 | 159.38 | -11.06 | 123.95 | 0.2319 | 840.0 | 710.5 | |
0.00 | 0.61 | 0.00 | 0.31 | -4.90 | 159.35 | -11.09 | 130.62 | 0.2535 | 852.0 | 719.6 | |
0.00 | 1.82 | 0.00 | 0.93 | -4.75 | 159.27 | -11.17 | 129.94 | 0.2530 | 956.0 | 840.1 | |
0.00 | 1.13 | 0.00 | 0.58 | -4.54 | 159.15 | -11.29 | 129.00 | 0.2523 | 673.0 | 630.9 | |
0.00 | 1.39 | 0.00 | 0.73 | -7.14 | 154.46 | -15.98 | 126.35 | 0.3408 | 802.0 | 605.6 | |
0.00 | 0.78 | 0.00 | 0.42 | -5.65 | 148.39 | -22.05 | 114.84 | 0.4134 | -701.0 | -584.3 | |
0.00 | 1.56 | 0.00 | 0.85 | -5.34 | 147.63 | -22.81 | 113.42 | 0.4225 | -695.0 | -592.6 | |
0.00 | 0.87 | 0.00 | 0.47 | -4.55 | 146.97 | -23.47 | 111.10 | 0.4273 | -593.0 | -520.7 |
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. |