| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 320 | 2069 | 257 | 1664 | 17.96 | 308.95 | -51.13 | 70.10 | 0.7879 | -384.8 | -391.1 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-07-10 12:47:31 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22 | 79 | 14 | 50 | 18.90 | 322.89 | -37.19 | 64.65 | 0.6351 | 1173.7 | 599.5 | |
| 0 | 4 | 0 | 2 | 18.15 | 319.92 | -40.16 | 66.96 | 0.6682 | 538.0 | 511.3 | |
| 5 | 92 | 3 | 64 | 19.24 | 317.36 | -42.72 | 66.33 | 0.7017 | -1172.7 | -547.4 | |
| 0 | 14 | 0 | 9 | 18.61 | 317.27 | -42.81 | 67.23 | 0.7007 | -1222.0 | -861.6 | |
| 0 | 5 | 0 | 4 | 17.56 | 317.59 | -42.49 | 68.60 | 0.6940 | -875.0 | -754.9 | |
| 5 | -3 | 3 | -3 | 19.13 | 316.93 | -43.15 | 66.62 | 0.7062 | -913.9 | 999999 | |
| 0 | 4 | 0 | 3 | 18.44 | 316.99 | -43.09 | 67.57 | 0.7035 | -847.0 | -739.2 | |
| 3 | 17 | 2 | 12 | 17.79 | 316.44 | -43.64 | 68.62 | 0.7080 | -769.0 | -705.7 | |
| 14 | 84 | 10 | 60 | 19.09 | 315.96 | -44.12 | 66.99 | 0.7170 | -1024.6 | -437.0 | |
| 0 | 8 | 0 | 5 | 17.73 | 315.99 | -44.09 | 68.84 | 0.7129 | -409.0 | -328.2 | |
| 6 | -9 | 4 | -9 | 18.86 | 315.51 | -44.57 | 67.44 | 0.7215 | -756.7 | 999999 | |
| 0 | 5 | 0 | 3 | 19.74 | 313.88 | -46.20 | 66.75 | 0.7417 | -565.0 | -551.6 | |
| 0 | 4 | 0 | 3 | 18.95 | 313.13 | -46.95 | 67.99 | 0.7478 | 270.0 | 362.5 | |
| 0 | 6 | 0 | 4 | 18.27 | 312.70 | -47.38 | 68.99 | 0.7508 | 570.0 | 461.2 | |
| 0 | 3 | 0 | 3 | 17.97 | 312.43 | -47.65 | 69.45 | 0.7530 | 186.0 | 170.5 | |
| 0 | 3 | 0 | 2 | 21.03 | 310.56 | -49.52 | 66.00 | 0.7794 | 415.0 | 555.9 | |
| 0 | 6 | 0 | 4 | 19.91 | 310.72 | -49.36 | 67.37 | 0.7752 | 525.0 | 528.6 | |
| 0 | 4 | 0 | 3 | 17.02 | 311.58 | -48.50 | 70.88 | 0.7602 | -427.0 | -505.2 | |
| 6 | 1678 | 5 | 1387 | 18.30 | 309.95 | -50.13 | 69.59 | 0.7797 | -1752.4 | -426.9 | |
| 52 | -19 | 42 | -19 | 18.86 | 309.66 | -50.42 | 68.94 | 0.7838 | 750.5 | 999999 | |
| -20 | -19 | -20 | -19 | 18.60 | 309.37 | -50.71 | 69.33 | 0.7862 | 999999 | 999999 | |
| 7 | -19 | 6 | -19 | 18.03 | 309.47 | -50.61 | 70.03 | 0.7842 | -1999.5 | 999999 | |
| 20 | -19 | 16 | -19 | 15.55 | 309.98 | -50.10 | 73.08 | 0.7747 | -1559.8 | 999999 | |
| 39 | -19 | 31 | -19 | 16.70 | 309.19 | -50.89 | 71.77 | 0.7848 | -1312.0 | 999999 | |
| 10 | -19 | 8 | -19 | 15.97 | 309.45 | -50.63 | 72.64 | 0.7810 | -1122.6 | 999999 | |
| -24 | -19 | -24 | -19 | 16.38 | 309.31 | -50.77 | 72.15 | 0.7831 | 999999 | 999999 | |
| 9 | -19 | 7 | -19 | 18.86 | 308.04 | -52.04 | 69.28 | 0.7999 | 605.2 | 999999 | |
| 23 | -19 | 19 | -19 | 18.27 | 307.82 | -52.26 | 70.05 | 0.8011 | -867.7 | 999999 | |
| 29 | -19 | 25 | -19 | 19.28 | 306.60 | -53.48 | 69.04 | 0.8145 | 847.5 | 999999 | |
| 6 | -19 | 5 | -19 | 18.10 | 306.86 | -53.22 | 70.44 | 0.8102 | 55.8 | 999999 | |
| 0 | 5 | 0 | 4 | 15.04 | 307.11 | -52.97 | 74.17 | 0.8036 | -121.0 | -116.7 | |
| 0 | 14 | 0 | 12 | 14.46 | 306.97 | -53.11 | 74.90 | 0.8044 | -43.0 | 367.5 | |
| 4 | 17 | 4 | 15 | 15.99 | 305.98 | -54.10 | 73.15 | 0.8158 | -770.9 | -546.8 | |
| 20 | -19 | 18 | -19 | 18.77 | 304.15 | -55.93 | 70.07 | 0.8364 | -300.0 | 999999 | |
| 3 | 17 | 2 | 15 | 16.10 | 305.01 | -55.07 | 73.14 | 0.8252 | -578.1 | -300.1 | |
| 18 | -19 | 16 | -19 | 17.78 | 304.04 | -56.04 | 71.27 | 0.8361 | -1179.6 | 999999 | |
| 4 | -19 | 4 | -19 | 18.30 | 303.78 | -56.30 | 70.69 | 0.8391 | -659.1 | 999999 | |
| 15 | -19 | 13 | -19 | 17.27 | 303.83 | -56.25 | 71.90 | 0.8375 | -702.9 | 999999 | |
| -38 | -19 | -38 | -19 | 16.86 | 303.87 | -56.21 | 72.38 | 0.8367 | 999999 | 999999 | |
| 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. | |