SOHO MDI 2000-11-27 12:47:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r |
| 159 | 1123 | 122 | 851 | 19.82 | 358.25 | 46.67 | 295.45 | 0.7599 | |
|
previous
or next day for the same group /
back to the solar disc SOHO MDI 2000-11-27 12:47:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r |
| 0 | 4 | 0 | 3 | 19.57 | 2.39 | 50.81 | 293.81 | 0.8006 | |
| 0 | 3 | 0 | 3 | 20.85 | 1.67 | 50.10 | 295.57 | 0.7970 | |
| 8 | 969 | 6 | 740 | 18.85 | 359.29 | 47.71 | 293.85 | 0.7678 | |
| 43 | -3 | 34 | -3 | 20.43 | 359.73 | 48.15 | 295.68 | 0.7769 | |
| 45 | -3 | 35 | -3 | 20.11 | 358.87 | 47.29 | 295.58 | 0.7673 | |
| 6 | -3 | 5 | -3 | 18.51 | 358.14 | 46.56 | 293.78 | 0.7549 | |
| 9 | -3 | 7 | -3 | 17.51 | 357.63 | 46.05 | 292.67 | 0.7464 | |
| 7 | -3 | 5 | -3 | 18.07 | 357.64 | 46.06 | 293.39 | 0.7482 | |
| 7 | -3 | 5 | -3 | 19.76 | 358.13 | 46.55 | 295.39 | 0.7587 | |
| 0 | 4 | 0 | 3 | 16.40 | 356.76 | 45.18 | 291.49 | 0.7337 | |
| 13 | -3 | 9 | -3 | 17.76 | 357.01 | 45.44 | 293.20 | 0.7406 | |
| 7 | -3 | 5 | -3 | 19.09 | 356.66 | 45.08 | 295.06 | 0.7410 | |
| 0 | 2 | 0 | 2 | 21.08 | 356.99 | 45.41 | 297.48 | 0.7514 | |
| 8 | 118 | 6 | 86 | 21.79 | 356.10 | 44.52 | 298.74 | 0.7449 | |
| 6 | -14 | 5 | -14 | 21.51 | 355.42 | 43.84 | 298.67 | 0.7368 | |
| 0 | 2 | 0 | 1 | 23.85 | 349.86 | 38.28 | 304.47 | 0.6897 | |
| 0 | 16 | 0 | 10 | 22.67 | 348.36 | 36.78 | 303.78 | 0.6671 | |
| 0 | 5 | 0 | 3 | 22.00 | 345.52 | 33.94 | 304.68 | 0.6318 | |
| 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 | |