SOHO MDI 2000-11-05 11:11:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 67 | 452 | 37 | 258 | 2.46 | 272.11 | 29.80 | 268.27 | 0.4985 | 1510.7 | 631.5 | |
|
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 |
| 30 | 394 | 17 | 226 | 2.24 | 273.49 | 31.18 | 268.00 | 0.5198 | 1502.4 | 709.0 | |
| -1 | -1 | -1 | -1 | 2.06 | 273.12 | 30.82 | 267.60 | 0.5146 | 999999 | 999999 | |
| 4 | -1 | 2 | -1 | 1.88 | 272.76 | 30.46 | 267.20 | 0.5093 | 1528.0 | 999999 | |
| 4 | -1 | 2 | -1 | 3.27 | 272.71 | 30.41 | 269.93 | 0.5074 | 977.2 | 999999 | |
| 0 | 6 | 0 | 3 | 3.88 | 272.73 | 30.43 | 271.15 | 0.5075 | 657.0 | 667.6 | |
| 4 | -1 | 2 | -1 | 2.23 | 272.54 | 30.24 | 267.87 | 0.5057 | 1496.0 | 999999 | |
| 25 | -1 | 14 | -1 | 2.74 | 272.33 | 30.03 | 268.85 | 0.5021 | 1804.9 | 999999 | |
| 0 | 3 | 0 | 2 | 1.57 | 271.64 | 29.34 | 266.40 | 0.4928 | 645.0 | 627.5 | |
| 0 | 5 | 0 | 3 | 3.53 | 271.56 | 29.26 | 270.40 | 0.4899 | 857.0 | 816.1 | |
| 0 | 3 | 0 | 2 | 0.85 | 271.19 | 28.89 | 264.85 | 0.4871 | 347.0 | 392.5 | |
| 0 | 7 | 0 | 4 | 0.88 | 270.14 | 27.84 | 264.67 | 0.4710 | 735.0 | 722.0 | |
| 0 | 9 | 0 | 5 | 3.85 | 265.96 | 23.66 | 270.87 | 0.4022 | 693.0 | 602.9 | |
| 0 | 8 | 0 | 4 | 2.15 | 263.47 | 21.17 | 266.07 | 0.3633 | -778.0 | -644.9 | |
| 0 | 3 | 0 | 2 | 3.31 | 263.16 | 20.86 | 269.25 | 0.3571 | -690.0 | -613.1 | |
| 0 | 8 | 0 | 4 | 3.16 | 262.87 | 20.57 | 268.80 | 0.3524 | -996.0 | -847.1 | |
| 0 | 6 | 0 | 3 | 2.82 | 260.86 | 18.56 | 267.47 | 0.3196 | -941.0 | -834.7 | |
| 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. | |