| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r |
| 76 | 474 | 40 | 252 | 20.90 | 282.54 | -3.10 | 8.49 | 0.3474 | |
|
previous
or next day for the same group /
back to the solar disc Gyula 2000-11-29 11:42:42 UT ![]() |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r |
| 43 | 344 | 23 | 182 | 21.53 | 284.15 | -1.49 | 3.95 | 0.3525 | |
| 5 | -1 | 3 | -1 | 20.69 | 283.64 | -2.00 | 5.56 | 0.3395 | |
| 9 | -1 | 5 | -1 | 20.63 | 283.23 | -2.41 | 6.70 | 0.3393 | |
| 0 | 1 | 0 | 1 | 19.55 | 281.92 | -3.72 | 10.90 | 0.3249 | |
| 0 | 3 | 0 | 1 | 16.78 | 281.15 | -4.49 | 15.45 | 0.2830 | |
| 0 | 1 | 0 | 1 | 16.47 | 280.69 | -4.95 | 17.26 | 0.2800 | |
| 0 | 2 | 0 | 1 | 17.21 | 280.82 | -4.82 | 16.06 | 0.2913 | |
| 0 | 0 | 0 | 0 | 16.24 | 280.57 | -5.05 | 17.84 | 0.2770 | |
| 0 | 1 | 0 | 1 | 16.82 | 280.66 | -4.96 | 16.91 | 0.2857 | |
| 0 | 1 | 0 | 1 | 16.32 | 280.08 | -5.54 | 19.34 | 0.2809 | |
| 8 | 45 | 4 | 24 | 18.95 | 280.26 | -5.38 | 16.09 | 0.3217 | |
| 0 | 1 | 0 | 0 | 19.09 | 279.74 | -5.90 | 17.39 | 0.3264 | |
| 0 | 1 | 0 | 1 | 19.56 | 278.61 | -7.01 | 19.88 | 0.3396 | |
| 0 | 1 | 0 | 0 | 20.62 | 278.78 | -6.85 | 18.41 | 0.3551 | |
| 1 | 73 | 0 | 39 | 20.61 | 278.52 | -7.12 | 19.08 | 0.3563 | |
| 3 | -15 | 2 | -15 | 20.75 | 278.27 | -7.37 | 19.56 | 0.3598 | |
| 1 | -15 | 0 | -15 | 20.43 | 278.21 | -7.43 | 20.04 | 0.3553 | |
| 2 | -15 | 1 | -15 | 20.98 | 277.59 | -8.03 | 20.92 | 0.3670 | |
| 1 | -15 | 0 | -15 | 20.94 | 277.43 | -8.20 | 21.36 | 0.3674 | |
| 3 | -15 | 2 | -15 | 21.13 | 277.29 | -8.33 | 21.46 | 0.3711 | |
| 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 | |