| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 89 | 634 | 50 | 363 | -18.75 | 49.35 | -20.46 | 138.78 | 0.5011 | -778.9 | -211.2 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-07-05 06:23:31 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 3 | 0 | 2 | -14.85 | 53.58 | -16.23 | 139.03 | 0.4138 | -569.0 | -416.3 | |
| 52 | 334 | 29 | 187 | -17.73 | 52.50 | -17.30 | 141.65 | 0.4585 | -1832.3 | -702.6 | |
| -2 | -2 | -2 | -2 | -17.91 | 52.09 | -17.72 | 141.26 | 0.4646 | 999999 | 999999 | |
| -2 | -2 | -2 | -2 | -17.91 | 51.79 | -18.02 | 140.80 | 0.4677 | 999999 | 999999 | |
| 0 | 5 | 0 | 3 | -19.12 | 51.35 | -18.46 | 141.80 | 0.4859 | -769.0 | -537.4 | |
| 0 | 5 | 0 | 3 | -19.39 | 50.74 | -19.07 | 141.28 | 0.4947 | -782.0 | -599.4 | |
| 0 | 2 | 0 | 1 | -19.52 | 50.36 | -19.45 | 140.93 | 0.4998 | -645.0 | -464.0 | |
| 0 | 15 | 0 | 9 | -18.49 | 50.49 | -19.32 | 139.70 | 0.4870 | -1133.0 | -712.3 | |
| 0 | 9 | 0 | 5 | -19.15 | 50.01 | -19.80 | 139.92 | 0.4990 | -759.0 | -588.7 | |
| 0 | 4 | 0 | 2 | -18.14 | 49.20 | -20.61 | 137.40 | 0.4961 | -686.0 | -536.6 | |
| 10 | 20 | 6 | 11 | -20.43 | 48.35 | -21.46 | 139.43 | 0.5292 | -941.8 | -606.3 | |
| 4 | 16 | 2 | 9 | -19.01 | 48.28 | -21.53 | 137.42 | 0.5148 | -584.1 | -496.6 | |
| 0 | 4 | 0 | 2 | -19.32 | 48.15 | -21.66 | 137.67 | 0.5193 | -399.0 | -219.8 | |
| 0 | 4 | 0 | 2 | -20.70 | 47.90 | -21.91 | 139.21 | 0.5364 | -448.0 | -282.2 | |
| 0 | 4 | 0 | 2 | -16.30 | 48.13 | -21.68 | 133.23 | 0.4886 | 564.0 | 535.7 | |
| 0 | 8 | 0 | 5 | -18.98 | 47.74 | -22.07 | 136.69 | 0.5200 | -431.0 | -341.8 | |
| 0 | 3 | 0 | 2 | -16.64 | 47.91 | -21.90 | 133.48 | 0.4944 | 618.0 | 450.7 | |
| 0 | 4 | 0 | 2 | -18.57 | 46.99 | -22.82 | 135.17 | 0.5237 | 263.0 | 311.0 | |
| 7 | 48 | 4 | 28 | -19.87 | 46.61 | -23.20 | 136.52 | 0.5405 | 1171.1 | 648.9 | |
| 0 | 8 | 0 | 4 | -18.62 | 46.61 | -23.20 | 134.80 | 0.5281 | 607.0 | 747.7 | |
| 2 | -19 | 1 | -19 | -19.79 | 46.16 | -23.65 | 135.89 | 0.5443 | 837.5 | 999999 | |
| 0 | 10 | 0 | 6 | -18.33 | 46.29 | -23.52 | 134.00 | 0.5286 | 802.0 | 801.1 | |
| 0 | 7 | 0 | 4 | -21.36 | 45.71 | -24.09 | 137.45 | 0.5644 | 785.0 | 611.8 | |
| 0 | 4 | 0 | 2 | -19.02 | 46.05 | -23.76 | 134.70 | 0.5379 | 796.0 | 830.1 | |
| 0 | 5 | 0 | 3 | -18.64 | 45.97 | -23.84 | 134.07 | 0.5350 | 1186.0 | 1073.1 | |
| 0 | 7 | 0 | 4 | -19.64 | 45.59 | -24.22 | 135.01 | 0.5487 | 1004.0 | 764.7 | |
| 0 | 12 | 0 | 7 | -19.39 | 45.21 | -24.60 | 134.25 | 0.5502 | 1148.0 | 1023.9 | |
| 0 | 2 | 0 | 1 | -18.83 | 45.30 | -24.51 | 133.57 | 0.5440 | 769.0 | 787.3 | |
| 0 | 8 | 0 | 5 | -20.60 | 45.01 | -24.80 | 135.66 | 0.5639 | 817.0 | 725.0 | |
| 14 | 41 | 8 | 25 | -19.97 | 44.37 | -25.44 | 134.12 | 0.5645 | 1117.1 | 775.2 | |
| 0 | 4 | 0 | 3 | -23.62 | 43.57 | -26.24 | 137.93 | 0.6069 | 571.0 | 329.8 | |
| 0 | 6 | 0 | 4 | -20.46 | 43.82 | -25.99 | 134.18 | 0.5748 | 704.0 | 689.5 | |
| 0 | 4 | 0 | 2 | -21.25 | 43.62 | -26.19 | 135.01 | 0.5840 | 509.0 | 419.7 | |
| 0 | 5 | 0 | 3 | -20.86 | 43.60 | -26.21 | 134.48 | 0.5806 | 667.0 | 543.6 | |
| 0 | 4 | 0 | 3 | -21.74 | 43.19 | -26.62 | 135.20 | 0.5929 | 707.0 | 540.8 | |
| 0 | 3 | 0 | 2 | -20.49 | 42.77 | -27.04 | 133.14 | 0.5858 | 825.0 | 629.9 | |
| 0 | 5 | 0 | 3 | -21.90 | 42.25 | -27.56 | 134.45 | 0.6037 | 567.0 | 467.6 | |
| 0 | 3 | 0 | 2 | -21.11 | 42.36 | -27.45 | 133.55 | 0.5955 | 599.0 | 444.7 | |
| 0 | 8 | 0 | 5 | -20.65 | 41.73 | -28.07 | 132.33 | 0.5979 | 716.0 | 478.7 | |
| 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. | |