| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 107 | 757 | 58 | 413 | 2.65 | 271.65 | -24.24 | 93.04 | 0.4124 | 1605.4 | 610.6 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-01 09:35:32 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34 | 705 | 18 | 382 | 2.26 | 272.87 | -23.02 | 94.23 | 0.3935 | 2042.2 | 639.1 | |
| 13 | -1 | 7 | -1 | 2.13 | 272.37 | -23.52 | 94.43 | 0.4017 | 1461.0 | 999999 | |
| 12 | -1 | 7 | -1 | 3.43 | 271.92 | -23.97 | 91.14 | 0.4073 | 1563.8 | 999999 | |
| 6 | -1 | 3 | -1 | 2.30 | 271.61 | -24.28 | 93.83 | 0.4136 | 1235.1 | 999999 | |
| 31 | -1 | 17 | -1 | 2.87 | 271.47 | -24.42 | 92.42 | 0.4150 | 1609.5 | 999999 | |
| 7 | -1 | 4 | -1 | 2.90 | 271.13 | -24.76 | 92.30 | 0.4204 | 1143.8 | 999999 | |
| 4 | 16 | 2 | 9 | 4.57 | 270.22 | -25.66 | 88.30 | 0.4338 | 870.2 | 661.2 | |
| 0 | 4 | 0 | 2 | 4.02 | 268.91 | -26.98 | 89.49 | 0.4545 | -446.0 | -310.0 | |
| 0 | 3 | 0 | 2 | 2.16 | 268.35 | -27.54 | 93.49 | 0.4648 | -500.0 | -432.4 | |
| 0 | 5 | 0 | 3 | 4.04 | 268.25 | -27.63 | 89.41 | 0.4646 | 655.0 | 499.2 | |
| 0 | 5 | 0 | 3 | -3.23 | 267.01 | -28.88 | 104.08 | 0.4992 | 607.0 | 480.8 | |
| 0 | 4 | 0 | 2 | 0.54 | 266.35 | -29.54 | 96.38 | 0.4981 | 839.0 | 666.2 | |
| 0 | 4 | 0 | 3 | 2.10 | 264.72 | -31.17 | 92.97 | 0.5200 | 452.0 | 368.4 | |
| 0 | 3 | 0 | 2 | 1.55 | 263.51 | -32.38 | 93.80 | 0.5387 | 624.0 | 473.5 | |
| 0 | 8 | 0 | 5 | 5.09 | 258.60 | -37.28 | 87.19 | 0.6064 | -406.0 | -548.2 | |
| 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. | |