SOHO MDI 2000-11-03 08:42:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 79 | 468 | 41 | 241 | -10.15 | 277.47 | 7.45 | 207.46 | 0.2878 | -1185.0 | -413.8 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-03 08:42:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48 | 297 | 25 | 154 | -9.36 | 280.00 | 9.98 | 216.52 | 0.2887 | -1998.9 | -664.0 | |
| 6 | -1 | 3 | -1 | -9.75 | 279.49 | 9.48 | 214.33 | 0.2891 | -1328.2 | 999999 | |
| 10 | 59 | 5 | 31 | -9.86 | 278.47 | 8.45 | 211.14 | 0.2813 | -1416.5 | -731.6 | |
| 0 | 11 | 0 | 6 | -7.84 | 277.17 | 7.15 | 210.98 | 0.2407 | -975.0 | -802.0 | |
| 0 | 7 | 0 | 3 | -10.70 | 274.08 | 4.06 | 195.30 | 0.2650 | -526.0 | -450.8 | |
| 0 | 4 | 0 | 2 | -12.77 | 270.68 | 0.66 | 182.21 | 0.2909 | -493.0 | -357.8 | |
| 0 | 6 | 0 | 3 | -13.86 | 270.36 | 0.34 | 181.08 | 0.3089 | -763.0 | -607.8 | |
| 0 | 4 | 0 | 2 | -16.51 | 269.88 | -0.13 | 179.63 | 0.3527 | -896.0 | -737.8 | |
| 6 | 32 | 3 | 16 | -11.73 | 269.65 | -0.37 | 178.68 | 0.2732 | 1264.0 | 986.6 | |
| 0 | 8 | 0 | 4 | -13.45 | 269.53 | -0.49 | 178.42 | 0.3023 | 1014.0 | 754.4 | |
| 5 | -9 | 3 | -9 | -11.65 | 269.30 | -0.72 | 177.39 | 0.2721 | 1363.8 | 999999 | |
| 0 | 6 | 0 | 3 | -13.33 | 269.13 | -0.88 | 177.13 | 0.3005 | 557.0 | 559.1 | |
| 0 | 7 | 0 | 3 | -14.51 | 268.14 | -1.88 | 174.30 | 0.3213 | 926.0 | 760.3 | |
| 0 | 5 | 0 | 2 | -13.34 | 267.91 | -2.11 | 173.16 | 0.3023 | 563.0 | 534.8 | |
| 4 | 22 | 2 | 12 | -13.50 | 267.51 | -2.51 | 171.97 | 0.3058 | 1277.9 | 964.0 | |
| 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. | |