| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.33 | 141.75 | 12.53 | 72.97 | 8.35 | 357.38 | 12.89 | 305.84 | 0.2735 | -907.2 | -411.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-12-14 18:58:55 UT
See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.45 | 0.00 | 0.75 | 9.33 | 359.68 | 15.19 | 304.18 | 0.3140 | -886.0 | -702.9 | |
| 24.33 | 128.55 | 12.53 | 66.23 | 8.31 | 357.61 | 13.12 | 305.14 | 0.2759 | -1443.9 | -432.8 | |
| 0.00 | 1.87 | 0.00 | 0.96 | 8.34 | 356.87 | 12.39 | 306.77 | 0.2662 | -1121.0 | -887.9 | |
| 0.00 | 2.30 | 0.00 | 1.18 | 8.04 | 356.41 | 11.92 | 306.88 | 0.2569 | -1215.0 | -902.7 | |
| 0.00 | 1.70 | 0.00 | 0.87 | 8.09 | 355.71 | 11.22 | 308.72 | 0.2481 | -1042.0 | -765.2 | |
| 0.00 | 1.02 | 0.00 | 0.53 | 10.97 | 354.89 | 10.40 | 319.00 | 0.2714 | -806.0 | -600.6 | |
| 0.00 | 1.28 | 0.00 | 0.65 | 8.54 | 353.48 | 8.99 | 316.37 | 0.2251 | 931.0 | 766.7 | |
| 0.00 | 1.11 | 0.00 | 0.56 | 8.72 | 353.30 | 8.82 | 317.49 | 0.2253 | 974.0 | 724.3 | |
| 0.00 | 1.70 | 0.00 | 0.86 | 9.70 | 352.00 | 7.51 | 324.74 | 0.2243 | 799.0 | 686.8 | |
| 0.00 | 0.77 | 0.00 | 0.38 | 6.65 | 350.12 | 5.63 | 323.09 | 0.1631 | 927.0 | 826.7 | |
| 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. | |