| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 78 | 603 | 45 | 341 | -23.32 | 305.83 | 9.44 | 198.03 | 0.4884 | -1347.1 | -595.7 | |
|
previous
or next observation for the same group /
back to the solar disc SOHO MDI 2000-11-01 08:40:32 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0 | 3 | 0 | 2 | -25.26 | 312.87 | 16.48 | 207.63 | 0.5553 | -724.0 | -682.2 | |
| 0 | 5 | 0 | 3 | -22.72 | 310.24 | 13.85 | 206.06 | 0.5048 | -842.0 | -716.6 | |
| 4 | 10 | 2 | 6 | -23.19 | 310.12 | 13.73 | 205.42 | 0.5103 | -854.4 | -708.1 | |
| 8 | 21 | 5 | 12 | -23.37 | 308.20 | 11.81 | 202.12 | 0.5011 | -891.3 | -571.8 | |
| 25 | 131 | 14 | 74 | -22.41 | 307.31 | 10.92 | 201.37 | 0.4826 | -1682.8 | -764.3 | |
| 3 | 13 | 2 | 7 | -22.52 | 306.18 | 9.79 | 199.25 | 0.4782 | -1385.4 | -1008.2 | |
| 17 | 355 | 10 | 201 | -23.86 | 305.59 | 9.20 | 197.27 | 0.4946 | -1502.9 | -609.9 | |
| 18 | -7 | 10 | -7 | -23.59 | 305.06 | 8.67 | 196.50 | 0.4884 | -1639.6 | 999999 | |
| 0 | 16 | 0 | 9 | -25.08 | 305.04 | 8.65 | 195.55 | 0.5099 | -393.0 | -248.1 | |
| 0 | 6 | 0 | 3 | -21.05 | 304.78 | 8.39 | 197.70 | 0.4498 | -23.0 | 109.7 | |
| 0 | 16 | 0 | 9 | -25.53 | 304.94 | 8.55 | 195.14 | 0.5159 | 647.0 | 596.9 | |
| 0 | 6 | 0 | 4 | -25.21 | 304.44 | 8.05 | 194.47 | 0.5094 | -370.0 | -288.6 | |
| 0 | 3 | 0 | 1 | -21.68 | 303.81 | 7.42 | 195.37 | 0.4549 | 349.0 | 248.5 | |
| 0 | 10 | 0 | 6 | -21.29 | 303.21 | 6.82 | 194.40 | 0.4466 | -870.0 | -763.4 | |
| 3 | -7 | 2 | -7 | -22.14 | 303.21 | 6.82 | 193.90 | 0.4595 | 525.1 | 999999 | |
| 0 | 4 | 0 | 2 | -23.09 | 303.00 | 6.61 | 193.00 | 0.4730 | 573.0 | 492.6 | |
| 0 | 4 | 0 | 2 | -21.36 | 302.55 | 6.16 | 193.02 | 0.4453 | -571.0 | -636.5 | |
| 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. | |