| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 10.41 | 0.00 | 6.03 | 13.34 | 17.48 | -28.48 | 64.04 | 0.5185 | -511.8 | -497.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-12-05 03:00:25 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 | 0.85 | 0.00 | 0.47 | 15.12 | 23.76 | -22.20 | 55.06 | 0.4469 | -665.0 | -529.5 | |
| 0.00 | 1.11 | 0.00 | 0.63 | 16.62 | 20.55 | -25.41 | 55.73 | 0.4997 | -628.0 | -520.5 | |
| 0.00 | 0.85 | 0.00 | 0.47 | 7.38 | 19.87 | -26.09 | 74.32 | 0.4549 | -696.0 | -576.1 | |
| 0.00 | 1.02 | 0.00 | 0.59 | 13.41 | 18.51 | -27.45 | 63.24 | 0.5043 | -694.0 | -563.1 | |
| 0.00 | 1.54 | 0.00 | 0.89 | 13.26 | 17.74 | -28.22 | 64.10 | 0.5138 | -768.0 | -647.9 | |
| 0.00 | 1.28 | 0.00 | 0.74 | 13.59 | 17.18 | -28.79 | 63.90 | 0.5233 | -593.0 | -523.5 | |
| 0.00 | 0.77 | 0.00 | 0.44 | 9.10 | 17.36 | -28.61 | 72.13 | 0.4988 | -550.0 | -514.4 | |
| 0.00 | 0.68 | 0.00 | 0.41 | 15.45 | 15.50 | -30.47 | 61.92 | 0.5561 | -575.0 | -489.0 | |
| 0.00 | 0.94 | 0.00 | 0.55 | 13.53 | 15.57 | -30.39 | 65.10 | 0.5444 | -507.0 | -417.0 | |
| 0.00 | 1.11 | 0.00 | 0.67 | 13.64 | 13.67 | -32.29 | 66.07 | 0.5702 | -577.0 | -454.8 | |
| 0.00 | 0.26 | 0.00 | 0.17 | 15.76 | 4.96 | -41.00 | 67.10 | 0.6878 | 623.0 | 589.0 | |
| 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. | |