| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33 | 208 | 41 | 264 | -23.43 | 305.19 | 62.89 | 242.51 | 0.9216 | -277.6 | -103.5 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-05 11:11:32 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 6 | 0 | 7 | -20.55 | 306.49 | 64.19 | 245.88 | 0.9253 | -76.0 | -64.7 | |
| 6 | 21 | 8 | 29 | -22.61 | 307.86 | 65.55 | 244.04 | 0.9362 | -397.5 | -182.8 | |
| 0 | 2 | 0 | 2 | -20.12 | 305.60 | 63.30 | 246.12 | 0.9191 | -553.0 | -450.5 | |
| 0 | 2 | 0 | 3 | -20.46 | 305.76 | 63.46 | 245.80 | 0.9207 | -392.0 | -423.9 | |
| 5 | 13 | 6 | 16 | -20.52 | 304.01 | 61.70 | 245.29 | 0.9095 | -400.2 | -320.0 | |
| 4 | 128 | 6 | 168 | -24.19 | 306.53 | 64.23 | 242.08 | 0.9313 | 24.7 | -138.6 | |
| 12 | -6 | 15 | -6 | -24.09 | 305.57 | 63.27 | 241.94 | 0.9256 | -608.6 | 999999 | |
| 0 | 2 | 0 | 2 | -20.74 | 302.78 | 60.48 | 244.73 | 0.9017 | -523.0 | -521.8 | |
| 0 | 4 | 0 | 5 | -25.59 | 306.12 | 63.82 | 240.52 | 0.9314 | 91.0 | 61.4 | |
| 0 | 2 | 0 | 2 | -20.03 | 300.62 | 58.32 | 244.89 | 0.8849 | 129.0 | 161.1 | |
| 0 | 3 | 0 | 4 | -22.55 | 299.85 | 57.55 | 241.93 | 0.8852 | 425.0 | 346.9 | |
| 4 | 17 | 4 | 18 | -23.10 | 299.91 | 57.61 | 241.35 | 0.8870 | 482.6 | 281.0 | |
| 2 | -12 | 2 | -12 | -23.26 | 299.62 | 57.32 | 241.09 | 0.8854 | 396.3 | 999999 | |
| 0 | 3 | 0 | 3 | -22.77 | 299.30 | 57.00 | 241.51 | 0.8818 | 284.0 | 402.2 | |
| 0 | 5 | 0 | 5 | -23.61 | 298.24 | 55.94 | 240.25 | 0.8763 | 407.0 | 351.4 | |
| 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. | |