SOHO MDI 2000-11-05 22:23:32 UT
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27 | 198 | 44 | 327 | -23.17 | 305.08 | 68.93 | 244.19 | 0.9533 | -115.8 | -91.4 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-05 22:23:32 UT |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 4 | 0 | 7 | -19.84 | 305.39 | 69.24 | 247.70 | 0.9520 | -349.0 | -302.8 | |
| 0 | 14 | 0 | 27 | -22.73 | 307.99 | 71.84 | 245.22 | 0.9664 | -202.0 | -106.6 | |
| 2 | 10 | 3 | 16 | -20.44 | 305.04 | 68.89 | 247.02 | 0.9509 | -218.9 | -163.8 | |
| 0 | 3 | 0 | 5 | -20.55 | 304.01 | 67.86 | 246.71 | 0.9458 | -326.0 | -270.9 | |
| 0 | 4 | 0 | 6 | -20.00 | 303.30 | 67.15 | 247.13 | 0.9414 | -223.0 | -250.4 | |
| 9 | 117 | 17 | 204 | -24.13 | 306.63 | 70.48 | 243.54 | 0.9620 | 56.9 | -99.2 | |
| 0 | 10 | 0 | 15 | -21.41 | 303.19 | 67.04 | 245.63 | 0.9425 | -477.0 | -439.5 | |
| 9 | -6 | 16 | -6 | -24.03 | 305.62 | 69.47 | 243.45 | 0.9575 | -476.4 | 999999 | |
| 0 | 8 | 0 | 10 | -20.33 | 299.88 | 63.73 | 246.02 | 0.9220 | 219.0 | 162.1 | |
| 4 | 13 | 5 | 17 | -21.89 | 299.98 | 63.83 | 244.41 | 0.9251 | 203.0 | 57.8 | |
| 0 | 4 | 0 | 5 | -22.78 | 299.31 | 63.16 | 243.30 | 0.9225 | 313.0 | 239.8 | |
| 0 | 1 | 0 | 2 | -23.13 | 299.52 | 63.36 | 242.99 | 0.9244 | 372.0 | 245.9 | |
| 3 | 10 | 3 | 13 | -23.55 | 299.41 | 63.26 | 242.52 | 0.9245 | 384.3 | 239.1 | |
| 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. | |