group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
61.20 | 112.74 | 39.63 | 72.66 | -16.48 | 242.19 | -33.11 | 125.02 | 0.6416 | -142.1 | 13.1 |
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spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
0.00 | 3.53 | 0.00 | 2.18 | -16.15 | 245.71 | -29.59 | 127.56 | 0.6005 | 849.0 | 745.8 | |
0.00 | 1.54 | 0.00 | 0.95 | -16.06 | 245.43 | -29.87 | 127.19 | 0.6029 | 651.0 | 579.4 | |
0.00 | 2.17 | 0.00 | 1.35 | -16.50 | 245.32 | -29.98 | 127.68 | 0.6076 | 675.0 | 502.8 | |
0.00 | 2.08 | 0.00 | 1.30 | -16.44 | 245.11 | -30.19 | 127.42 | 0.6094 | 667.0 | 590.0 | |
0.00 | 1.08 | 0.00 | 0.68 | -15.11 | 244.38 | -30.92 | 124.95 | 0.6074 | 431.0 | 405.5 | |
2.26 | 3.07 | 1.44 | 1.95 | -17.23 | 243.93 | -31.37 | 127.44 | 0.6284 | -758.1 | -521.4 | |
0.00 | 1.27 | 0.00 | 0.79 | -14.81 | 243.35 | -31.94 | 123.68 | 0.6169 | 726.0 | 606.2 | |
2.62 | 41.41 | 1.66 | 26.40 | -15.57 | 243.19 | -32.11 | 124.59 | 0.6242 | -771.6 | 20.3 | |
0.00 | 1.36 | 0.00 | 0.87 | -17.14 | 242.67 | -32.63 | 126.27 | 0.6413 | 185.0 | 258.4 | |
7.78 | -8.00 | 4.96 | -8.00 | -15.99 | 242.74 | -32.56 | 124.79 | 0.6322 | -477.8 | 999999 | |
15.64 | -8.00 | 9.97 | -8.00 | -15.77 | 242.63 | -32.67 | 124.40 | 0.6319 | 731.3 | 999999 | |
0.00 | 0.81 | 0.00 | 0.52 | -16.41 | 242.32 | -32.98 | 125.02 | 0.6398 | 474.0 | 309.3 | |
0.99 | -8.00 | 0.64 | -8.00 | -15.96 | 242.14 | -33.16 | 124.28 | 0.6386 | 579.0 | 999999 | |
0.00 | 2.44 | 0.00 | 1.58 | -16.60 | 241.86 | -33.43 | 124.91 | 0.6461 | 400.0 | 167.5 | |
11.75 | 14.28 | 7.68 | 9.33 | -17.37 | 241.67 | -33.63 | 125.77 | 0.6537 | -791.2 | -572.2 | |
0.00 | 2.26 | 0.00 | 1.45 | -15.78 | 241.87 | -33.43 | 123.83 | 0.6404 | 683.0 | 491.2 | |
0.00 | 2.53 | 0.00 | 1.64 | -15.97 | 241.41 | -33.88 | 123.73 | 0.6467 | 552.0 | 361.0 | |
20.16 | 32.91 | 13.28 | 21.67 | -17.03 | 240.74 | -34.56 | 124.62 | 0.6613 | -778.0 | -581.2 |
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. |