| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 47 | 489 | 26 | 260 | 10.16 | 268.07 | -19.91 | 72.17 | 0.3536 | 1122.2 | 369.2 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-01 23:59:32 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 6 | 0 | 3 | 7.00 | 276.70 | -11.29 | 75.45 | 0.2016 | 1064.0 | 878.8 | |
| 0 | 7 | 0 | 3 | 5.22 | 275.79 | -12.19 | 84.70 | 0.2122 | 858.0 | 804.0 | |
| 0 | 6 | 0 | 3 | 14.03 | 275.38 | -12.60 | 50.80 | 0.2744 | 655.0 | 536.0 | |
| 0 | 4 | 0 | 2 | 8.18 | 275.47 | -12.51 | 71.62 | 0.2270 | 578.0 | 446.6 | |
| 0 | 5 | 0 | 2 | 9.01 | 274.28 | -13.70 | 69.81 | 0.2503 | 652.0 | 666.3 | |
| 0 | 4 | 0 | 2 | 7.39 | 274.22 | -13.76 | 76.23 | 0.2440 | 745.0 | 654.1 | |
| 0 | 3 | 0 | 2 | 12.16 | 272.92 | -15.06 | 60.95 | 0.2919 | 682.0 | 672.5 | |
| 0 | 12 | 0 | 6 | 8.82 | 272.28 | -15.70 | 72.70 | 0.2814 | 1153.0 | 908.0 | |
| 0 | 5 | 0 | 3 | 9.24 | 272.01 | -15.97 | 71.52 | 0.2876 | 1222.0 | 983.6 | |
| 0 | 11 | 0 | 6 | 8.92 | 271.46 | -16.52 | 73.10 | 0.2949 | 1151.0 | 906.5 | |
| 3 | 21 | 2 | 11 | 9.53 | 271.35 | -16.63 | 71.20 | 0.2995 | 862.5 | 683.6 | |
| 0 | 6 | 0 | 3 | 8.37 | 271.40 | -16.58 | 74.94 | 0.2936 | 752.0 | 642.9 | |
| 0 | 4 | 0 | 2 | 8.02 | 271.22 | -16.76 | 76.25 | 0.2954 | 603.0 | 545.9 | |
| 0 | 10 | 0 | 5 | 8.90 | 270.81 | -17.17 | 73.69 | 0.3053 | 793.0 | 711.5 | |
| 9 | 228 | 5 | 120 | 10.03 | 269.40 | -18.58 | 71.42 | 0.3326 | 1757.8 | 693.7 | |
| 0 | 5 | 0 | 3 | 7.52 | 269.40 | -18.58 | 78.92 | 0.3233 | 685.0 | 589.7 | |
| 0 | 9 | 0 | 5 | 8.98 | 269.25 | -18.73 | 74.60 | 0.3305 | 1157.0 | 829.2 | |
| 7 | -15 | 4 | -15 | 9.48 | 269.10 | -18.88 | 73.25 | 0.3349 | 1412.7 | 999999 | |
| 5 | -15 | 3 | -15 | 9.98 | 269.07 | -18.91 | 71.82 | 0.3375 | 1765.7 | 999999 | |
| 6 | -15 | 3 | -15 | 9.98 | 268.78 | -19.20 | 72.07 | 0.3420 | 1441.3 | 999999 | |
| 10 | -15 | 5 | -15 | 9.89 | 268.37 | -19.61 | 72.62 | 0.3480 | 1306.4 | 999999 | |
| 0 | 5 | 0 | 3 | 6.49 | 268.38 | -19.60 | 82.42 | 0.3378 | -782.0 | -648.4 | |
| 3 | -15 | 2 | -15 | 9.69 | 267.93 | -20.05 | 73.50 | 0.3541 | 1219.1 | 999999 | |
| 0 | 4 | 0 | 2 | 8.75 | 267.52 | -20.46 | 76.33 | 0.3571 | 756.0 | 643.0 | |
| 0 | 4 | 0 | 2 | 9.63 | 267.10 | -20.89 | 74.20 | 0.3669 | 530.0 | 299.3 | |
| 0 | 9 | 0 | 5 | 9.72 | 266.12 | -21.86 | 74.54 | 0.3824 | 961.0 | 679.4 | |
| 0 | 6 | 0 | 3 | 9.25 | 265.86 | -22.12 | 75.89 | 0.3849 | -589.0 | -438.8 | |
| 4 | 14 | 2 | 7 | 10.01 | 265.34 | -22.64 | 74.26 | 0.3955 | 1084.1 | 796.7 | |
| 0 | 4 | 0 | 2 | 12.40 | 264.72 | -23.26 | 68.94 | 0.4152 | -669.0 | -628.7 | |
| 0 | 7 | 0 | 4 | 12.86 | 264.46 | -23.52 | 68.08 | 0.4213 | -820.0 | -778.2 | |
| 0 | 6 | 0 | 3 | 10.10 | 264.61 | -23.37 | 74.42 | 0.4071 | 321.0 | 400.1 | |
| 0 | 5 | 0 | 3 | 12.88 | 264.06 | -23.92 | 68.30 | 0.4272 | -636.0 | -561.4 | |
| 0 | 9 | 0 | 5 | 12.18 | 264.00 | -23.98 | 69.93 | 0.4247 | -888.0 | -795.4 | |
| 0 | 3 | 0 | 2 | 12.70 | 262.96 | -25.03 | 69.47 | 0.4426 | -713.0 | -709.6 | |
| 0 | 5 | 0 | 3 | 12.64 | 262.52 | -25.46 | 69.85 | 0.4486 | -1132.0 | -1000.3 | |
| 0 | 6 | 0 | 3 | 12.25 | 262.43 | -25.55 | 70.75 | 0.4483 | -968.0 | -908.2 | |
| 0 | 14 | 0 | 8 | 13.03 | 262.31 | -25.67 | 69.17 | 0.4535 | -785.0 | -761.5 | |
| 0 | 12 | 0 | 7 | 12.83 | 262.15 | -25.83 | 69.68 | 0.4549 | -981.0 | -867.4 | |
| 0 | 8 | 0 | 5 | 13.09 | 261.90 | -26.08 | 69.28 | 0.4597 | -953.0 | -834.8 | |
| 0 | 4 | 0 | 2 | 12.76 | 261.41 | -26.57 | 70.25 | 0.4654 | -824.0 | -782.9 | |
| 0 | 7 | 0 | 4 | 13.19 | 261.27 | -26.71 | 69.46 | 0.4692 | -779.0 | -609.8 | |
| 0 | 4 | 0 | 2 | 12.68 | 261.11 | -26.87 | 70.60 | 0.4694 | -779.0 | -696.9 | |
| 0 | 3 | 0 | 2 | 8.25 | 261.09 | -26.89 | 80.04 | 0.4564 | -766.0 | -667.2 | |
| 0 | 4 | 0 | 2 | 13.28 | 260.51 | -27.47 | 69.71 | 0.4807 | -591.0 | -599.9 | |
| 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. |
||
| 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. |
||
| 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. | |