| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 139 | 832 | 80 | 485 | -22.63 | 306.22 | -16.02 | 150.68 | 0.5221 | -1104.5 | -420.2 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-10-30 09:35:32 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 3 | 0 | 2 | -23.12 | 318.85 | -3.39 | 173.30 | 0.4680 | -582.0 | -539.8 | |
| 0 | 3 | 0 | 2 | -27.27 | 312.05 | -10.19 | 163.32 | 0.5501 | -729.0 | -631.8 | |
| 0 | 6 | 0 | 3 | -20.75 | 310.97 | -11.27 | 156.70 | 0.4642 | -778.0 | -702.0 | |
| 0 | 7 | 0 | 4 | -22.53 | 310.06 | -12.18 | 156.68 | 0.4944 | -1062.0 | -845.3 | |
| 9 | 27 | 5 | 15 | -23.22 | 309.95 | -12.29 | 157.09 | 0.5046 | -1006.3 | -583.0 | |
| 0 | 6 | 0 | 3 | -22.75 | 309.61 | -12.63 | 156.12 | 0.5002 | -1039.0 | -843.8 | |
| 0 | 3 | 0 | 2 | -22.94 | 309.08 | -13.16 | 155.41 | 0.5060 | -388.0 | -298.0 | |
| 12 | 44 | 7 | 26 | -23.44 | 307.77 | -14.47 | 153.79 | 0.5211 | -1110.2 | -364.2 | |
| 35 | 204 | 20 | 117 | -22.23 | 307.56 | -14.68 | 152.30 | 0.5067 | -1708.6 | -794.2 | |
| 0 | 5 | 0 | 3 | -19.17 | 307.48 | -14.76 | 148.86 | 0.4673 | 707.0 | 571.9 | |
| 0 | 4 | 0 | 2 | -23.50 | 306.81 | -15.43 | 152.38 | 0.5284 | -663.0 | -572.1 | |
| 0 | 5 | 0 | 3 | -23.29 | 306.57 | -15.67 | 151.82 | 0.5273 | -604.0 | -589.7 | |
| 0 | 3 | 0 | 2 | -25.32 | 306.09 | -16.15 | 153.02 | 0.5564 | -259.0 | -167.9 | |
| 14 | 341 | 8 | 199 | -23.57 | 305.88 | -16.36 | 151.07 | 0.5357 | -1290.7 | -468.5 | |
| 18 | -14 | 10 | -14 | -23.00 | 305.96 | -16.29 | 150.60 | 0.5281 | -1746.1 | 999999 | |
| 0 | 9 | 0 | 5 | -21.75 | 306.02 | -16.22 | 149.40 | 0.5118 | -623.0 | -480.2 | |
| 0 | 3 | 0 | 2 | -22.27 | 305.65 | -16.59 | 149.40 | 0.5212 | -849.0 | -819.9 | |
| 7 | -14 | 4 | -14 | -22.84 | 305.54 | -16.70 | 149.82 | 0.5291 | -1741.6 | 999999 | |
| 17 | -14 | 10 | -14 | -23.15 | 305.28 | -16.96 | 149.77 | 0.5349 | -1250.5 | 999999 | |
| 0 | 7 | 0 | 4 | -21.55 | 305.48 | -16.76 | 148.36 | 0.5134 | -864.0 | -706.3 | |
| 7 | -14 | 4 | -14 | -22.41 | 305.16 | -17.09 | 148.82 | 0.5267 | -1216.6 | 999999 | |
| 0 | 8 | 0 | 5 | -21.13 | 305.19 | -17.06 | 147.45 | 0.5106 | 412.0 | 350.3 | |
| 2 | 27 | 1 | 15 | -20.49 | 305.04 | -17.20 | 146.51 | 0.5039 | 667.7 | 755.1 | |
| 0 | 6 | 0 | 4 | -21.56 | 304.83 | -17.41 | 147.41 | 0.5188 | -868.0 | -656.5 | |
| 4 | -23 | 2 | -23 | -20.46 | 304.66 | -17.58 | 145.89 | 0.5067 | 1035.4 | 999999 | |
| 0 | 3 | 0 | 2 | -19.95 | 304.72 | -17.52 | 145.37 | 0.5001 | 654.0 | 612.1 | |
| 0 | 3 | 0 | 2 | -21.97 | 304.12 | -18.12 | 146.84 | 0.5294 | -445.0 | -303.3 | |
| 5 | 23 | 3 | 13 | -21.24 | 304.13 | -18.11 | 146.02 | 0.5206 | -239.3 | 36.2 | |
| 0 | 5 | 0 | 3 | -22.32 | 303.86 | -18.39 | 146.85 | 0.5358 | -187.0 | 22.0 | |
| 0 | 3 | 0 | 2 | -23.19 | 303.69 | -18.55 | 147.57 | 0.5475 | 352.0 | 199.3 | |
| 0 | 7 | 0 | 4 | -20.52 | 303.87 | -18.37 | 144.81 | 0.5142 | 834.0 | 736.0 | |
| 0 | 1 | 0 | 1 | -20.99 | 303.73 | -18.51 | 145.16 | 0.5211 | 525.0 | 505.8 | |
| 3 | 45 | 2 | 26 | -22.68 | 303.37 | -18.88 | 146.57 | 0.5440 | 953.5 | 484.9 | |
| 0 | 6 | 0 | 4 | -23.90 | 303.18 | -19.06 | 147.64 | 0.5599 | -593.0 | -466.2 | |
| 6 | -33 | 4 | -33 | -22.68 | 303.14 | -19.10 | 146.27 | 0.5459 | 796.9 | 999999 | |
| 0 | 11 | 0 | 7 | -23.56 | 302.97 | -19.27 | 146.99 | 0.5575 | -783.0 | -686.4 | |
| 0 | 4 | 0 | 3 | -22.46 | 301.85 | -20.40 | 144.30 | 0.5541 | -561.0 | -482.7 | |
| 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. |
||
| 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. | |