SOHO MDI 2000-11-05 10:28:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34 | 233 | 42 | 287 | -23.30 | 304.94 | 62.25 | 242.47 | 0.9173 | -275.9 | -85.1 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-05 10:28:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1 | 8 | 1 | 10 | -20.49 | 306.55 | 63.85 | 245.86 | 0.9231 | -25.0 | -20.5 | |
| 7 | 23 | 9 | 32 | -22.68 | 307.90 | 65.20 | 243.89 | 0.9344 | -382.5 | -197.7 | |
| 0 | 3 | 0 | 4 | -20.48 | 305.70 | 63.01 | 245.67 | 0.9179 | -392.0 | -394.8 | |
| 0 | 2 | 0 | 2 | -20.13 | 305.45 | 62.75 | 245.98 | 0.9157 | -354.0 | -453.5 | |
| 6 | 16 | 7 | 18 | -20.53 | 303.88 | 61.19 | 245.15 | 0.9061 | -388.5 | -308.8 | |
| 5 | 130 | 7 | 168 | -24.21 | 306.55 | 63.86 | 241.96 | 0.9292 | 80.8 | -113.0 | |
| 11 | -6 | 14 | -6 | -24.11 | 305.60 | 62.91 | 241.82 | 0.9236 | -579.1 | 999999 | |
| 0 | 6 | 0 | 6 | -20.71 | 302.65 | 59.95 | 244.62 | 0.8981 | -523.0 | -482.2 | |
| 0 | 3 | 0 | 3 | -25.57 | 306.10 | 63.40 | 240.43 | 0.9290 | 74.0 | 71.3 | |
| 0 | 3 | 0 | 3 | -19.99 | 300.45 | 57.75 | 244.76 | 0.8806 | 63.0 | 105.4 | |
| 0 | 4 | 0 | 4 | -21.94 | 300.09 | 57.39 | 242.53 | 0.8826 | 147.0 | 88.5 | |
| 4 | 18 | 4 | 19 | -23.08 | 299.89 | 57.20 | 241.24 | 0.8840 | 403.4 | 226.8 | |
| 0 | 3 | 0 | 3 | -22.74 | 299.29 | 56.59 | 241.40 | 0.8788 | 540.0 | 394.7 | |
| 0 | 5 | 0 | 6 | -23.67 | 298.30 | 55.60 | 240.07 | 0.8741 | 466.0 | 386.3 | |
| 0 | 9 | 0 | 9 | -23.39 | 297.82 | 55.12 | 240.21 | 0.8697 | 138.0 | 368.9 | |
| 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. | |