| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57 | 400 | 30 | 210 | -12.82 | 177.04 | 6.76 | 202.51 | 0.3006 | 1541.6 | 544.5 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-10 22:23:32 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 4 | 0 | 2 | -17.64 | 179.88 | 9.60 | 204.11 | 0.3909 | -717.0 | -667.3 | |
| 0 | 5 | 0 | 3 | -16.20 | 179.60 | 9.33 | 205.13 | 0.3681 | -843.0 | -670.1 | |
| 0 | 12 | 0 | 6 | -12.92 | 178.86 | 8.59 | 207.68 | 0.3147 | -520.0 | -597.2 | |
| 11 | 333 | 6 | 173 | -13.24 | 177.68 | 7.40 | 203.92 | 0.3108 | 1315.2 | 709.4 | |
| 15 | -4 | 8 | -4 | -12.23 | 177.45 | 7.18 | 204.65 | 0.2940 | 2033.0 | 999999 | |
| 14 | -4 | 7 | -4 | -12.83 | 177.27 | 6.99 | 203.27 | 0.3019 | 1492.1 | 999999 | |
| 17 | -4 | 9 | -4 | -12.71 | 176.79 | 6.52 | 201.99 | 0.2969 | 1751.2 | 999999 | |
| 0 | 5 | 0 | 3 | -14.43 | 176.56 | 6.28 | 199.29 | 0.3224 | 506.0 | 415.4 | |
| 0 | 13 | 0 | 7 | -13.58 | 175.98 | 5.70 | 198.50 | 0.3059 | 706.0 | 637.0 | |
| 0 | 4 | 0 | 2 | -12.58 | 175.84 | 5.56 | 199.17 | 0.2893 | 530.0 | 577.1 | |
| 0 | 5 | 0 | 3 | -10.16 | 174.65 | 4.38 | 198.01 | 0.2442 | -428.0 | -358.9 | |
| 0 | 5 | 0 | 3 | -9.56 | 173.79 | 3.51 | 195.28 | 0.2303 | -774.0 | -627.5 | |
| 0 | 5 | 0 | 3 | -14.14 | 173.37 | 3.10 | 189.96 | 0.3041 | -617.0 | -696.9 | |
| 0 | 5 | 0 | 3 | -13.29 | 172.85 | 2.57 | 188.74 | 0.2888 | -688.0 | -680.9 | |
| 0 | 4 | 0 | 2 | -12.53 | 171.81 | 1.54 | 185.52 | 0.2739 | -762.0 | -614.4 | |
| 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. | |