| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 74 | 539 | 58 | 430 | -20.54 | 14.30 | 45.99 | 239.26 | 0.7838 | 100.1 | 168.7 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-07-12 22:23:31 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13 | 87 | 12 | 79 | -19.44 | 20.91 | 52.60 | 243.47 | 0.8394 | -657.3 | -237.0 | |
| 0 | 3 | 0 | 2 | -18.30 | 18.98 | 50.68 | 244.06 | 0.8190 | -728.0 | -665.4 | |
| 4 | 75 | 3 | 64 | -19.06 | 18.77 | 50.46 | 243.10 | 0.8196 | -740.8 | -412.2 | |
| 13 | -3 | 11 | -3 | -19.43 | 18.46 | 50.16 | 242.56 | 0.8181 | -905.7 | 999999 | |
| 0 | 3 | 0 | 3 | -19.92 | 16.66 | 48.36 | 241.24 | 0.8037 | -635.0 | -554.6 | |
| 4 | 17 | 3 | 14 | -20.65 | 16.58 | 48.28 | 240.36 | 0.8058 | -587.3 | -564.6 | |
| 0 | 2 | 0 | 2 | -20.80 | 16.14 | 47.83 | 239.99 | 0.8024 | -510.0 | -540.2 | |
| 0 | 10 | 0 | 8 | -20.35 | 15.82 | 47.52 | 240.37 | 0.7977 | -557.0 | -558.2 | |
| 0 | 4 | 0 | 3 | -20.11 | 13.82 | 45.52 | 239.72 | 0.7780 | 452.0 | 399.9 | |
| 3 | 313 | 2 | 237 | -21.04 | 11.84 | 43.54 | 237.62 | 0.7636 | 553.9 | 538.5 | |
| 0 | 2 | 0 | 1 | -18.18 | 10.54 | 42.24 | 240.41 | 0.7368 | 402.0 | 457.1 | |
| 7 | -10 | 5 | -10 | -20.75 | 11.33 | 43.02 | 237.69 | 0.7572 | 947.5 | 999999 | |
| 13 | -10 | 10 | -10 | -21.67 | 11.37 | 43.07 | 236.62 | 0.7622 | 718.9 | 999999 | |
| 0 | 13 | 0 | 10 | -19.59 | 10.59 | 42.28 | 238.69 | 0.7442 | 538.0 | 162.1 | |
| 9 | -10 | 7 | -10 | -21.26 | 10.93 | 42.62 | 236.87 | 0.7559 | 1206.2 | 999999 | |
| 6 | -10 | 4 | -10 | -21.16 | 9.86 | 41.55 | 236.39 | 0.7451 | 1461.7 | 999999 | |
| 0 | 3 | 0 | 2 | -19.03 | 8.90 | 40.59 | 238.44 | 0.7242 | 655.0 | 541.0 | |
| 2 | 7 | 1 | 5 | -22.07 | 6.27 | 37.97 | 233.08 | 0.7154 | 550.9 | 420.4 | |
| 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. | |