SOHO MDI 2000-07-08 14:23:31 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 146 | 1180 | 86 | 690 | -18.41 | 49.46 | 23.78 | 225.68 | 0.5371 | -695.7 | -206.4 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-07-08 14:23:31 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 4 | 0 | 2 | -25.29 | 53.64 | 27.97 | 221.53 | 0.6418 | 750.0 | 692.5 | |
| 8 | 39 | 5 | 23 | -16.27 | 51.74 | 26.06 | 231.45 | 0.5415 | -1164.5 | -923.7 | |
| 46 | 759 | 28 | 447 | -18.09 | 51.65 | 25.97 | 228.68 | 0.5564 | -1605.6 | -326.2 | |
| 8 | -3 | 5 | -3 | -17.01 | 51.02 | 25.34 | 229.58 | 0.5398 | -1349.7 | 999999 | |
| 0 | 5 | 0 | 3 | -16.07 | 50.71 | 25.03 | 230.65 | 0.5278 | -940.0 | -871.4 | |
| 7 | -3 | 4 | -3 | -18.02 | 50.90 | 25.22 | 227.97 | 0.5476 | -1619.0 | 999999 | |
| 0 | 6 | 0 | 3 | -16.18 | 50.31 | 24.64 | 230.04 | 0.5244 | -1255.0 | -950.6 | |
| 5 | -3 | 3 | -3 | -17.54 | 50.46 | 24.78 | 228.18 | 0.5384 | -1417.8 | 999999 | |
| 5 | -3 | 3 | -3 | -17.14 | 49.90 | 24.22 | 228.13 | 0.5285 | -1605.0 | 999999 | |
| 9 | -3 | 5 | -3 | -17.74 | 49.94 | 24.26 | 227.31 | 0.5345 | -1482.6 | 999999 | |
| 0 | 5 | 0 | 3 | -20.01 | 49.92 | 24.24 | 224.13 | 0.5563 | -562.0 | -546.6 | |
| 2 | 9 | 1 | 5 | -18.61 | 49.15 | 23.48 | 225.15 | 0.5346 | -1120.5 | -889.2 | |
| 14 | 100 | 8 | 59 | -19.30 | 49.07 | 23.40 | 224.11 | 0.5406 | -1414.3 | -766.0 | |
| 0 | 1 | 0 | 1 | -16.98 | 48.61 | 22.93 | 226.86 | 0.5128 | 379.0 | 283.0 | |
| 0 | 5 | 0 | 3 | -18.69 | 48.75 | 23.08 | 224.57 | 0.5312 | -985.0 | -917.1 | |
| 4 | -13 | 2 | -13 | -19.59 | 48.84 | 23.17 | 223.43 | 0.5412 | -1141.6 | 999999 | |
| 0 | 10 | 0 | 6 | -19.87 | 47.93 | 22.25 | 221.94 | 0.5349 | -501.0 | -433.8 | |
| 5 | -3 | 3 | -3 | -17.12 | 47.51 | 21.83 | 225.27 | 0.5022 | 1388.0 | 999999 | |
| 0 | 3 | 0 | 2 | -20.73 | 47.69 | 22.01 | 220.52 | 0.5417 | -164.0 | -268.5 | |
| 4 | -3 | 2 | -3 | -17.11 | 47.06 | 21.38 | 224.71 | 0.4973 | 1689.8 | 999999 | |
| 5 | -3 | 3 | -3 | -17.70 | 47.04 | 21.37 | 223.82 | 0.5033 | 1452.6 | 999999 | |
| 0 | 2 | 0 | 1 | -20.07 | 47.27 | 21.60 | 220.85 | 0.5306 | -333.0 | -255.8 | |
| 0 | 2 | 0 | 1 | -17.74 | 46.69 | 21.01 | 223.30 | 0.5000 | 1076.0 | 976.3 | |
| 4 | 10 | 2 | 5 | -16.67 | 46.52 | 20.84 | 224.64 | 0.4870 | 1211.9 | 952.2 | |
| 3 | 37 | 2 | 21 | -21.01 | 46.87 | 21.19 | 219.12 | 0.5369 | 947.5 | 429.0 | |
| 0 | 4 | 0 | 2 | -17.05 | 46.34 | 20.66 | 223.84 | 0.4891 | 1161.0 | 899.9 | |
| 0 | 5 | 0 | 3 | -19.18 | 46.29 | 20.62 | 220.75 | 0.5115 | 786.0 | 733.3 | |
| 0 | 5 | 0 | 3 | -20.96 | 46.50 | 20.82 | 218.70 | 0.5329 | 504.0 | 509.9 | |
| 0 | 7 | 0 | 4 | -18.70 | 46.10 | 20.42 | 221.14 | 0.5043 | 1194.0 | 1077.1 | |
| 6 | 108 | 3 | 63 | -20.59 | 45.76 | 20.09 | 218.19 | 0.5221 | 1417.7 | 604.4 | |
| 6 | -30 | 4 | -30 | -20.94 | 45.59 | 19.91 | 217.52 | 0.5243 | 1228.2 | 999999 | |
| 0 | 5 | 0 | 3 | -19.42 | 45.34 | 19.66 | 219.13 | 0.5049 | 993.0 | 909.9 | |
| 0 | 4 | 0 | 2 | -18.25 | 44.98 | 19.30 | 220.21 | 0.4882 | 839.0 | 708.0 | |
| 5 | -30 | 3 | -30 | -20.80 | 45.16 | 19.49 | 217.11 | 0.5189 | 1466.0 | 999999 | |
| 0 | 5 | 0 | 3 | -21.49 | 44.99 | 19.31 | 216.02 | 0.5253 | 692.0 | 657.3 | |
| 0 | 5 | 0 | 3 | -21.18 | 44.58 | 18.91 | 215.84 | 0.5181 | 1118.0 | 867.4 | |
| 0 | 4 | 0 | 2 | -18.36 | 44.06 | 18.39 | 218.72 | 0.4806 | 891.0 | 775.7 | |
| 0 | 3 | 0 | 2 | -21.87 | 44.27 | 18.60 | 214.57 | 0.5236 | 788.0 | 742.3 | |
| 0 | 8 | 0 | 4 | -20.19 | 43.39 | 17.71 | 215.31 | 0.4960 | 1063.0 | 862.5 | |
| 0 | 6 | 0 | 3 | -22.55 | 43.01 | 17.34 | 211.99 | 0.5215 | 802.0 | 694.2 | |
| 0 | 7 | 0 | 4 | -20.91 | 42.41 | 16.73 | 212.95 | 0.4965 | 746.0 | 790.2 | |
| 0 | 2 | 0 | 1 | -21.26 | 42.18 | 16.51 | 212.20 | 0.4989 | 530.0 | 523.3 | |
| 0 | 5 | 0 | 3 | -18.04 | 41.15 | 15.48 | 214.49 | 0.4499 | 986.0 | 744.7 | |
| 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. | |