| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.68 | 25.57 | 6.65 | 14.67 | -25.27 | 76.65 | -16.56 | 149.16 | 0.5039 | 42.7 | -206.5 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-12-06 12:58:56 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 |
| 9.12 | 11.26 | 5.17 | 6.38 | -24.96 | 78.30 | -14.91 | 151.27 | 0.4872 | 905.5 | 685.7 | |
| 0.00 | 1.53 | 0.00 | 0.87 | -24.96 | 77.86 | -15.35 | 150.58 | 0.4905 | 650.0 | 437.0 | |
| 0.00 | 0.85 | 0.00 | 0.49 | -24.77 | 76.87 | -16.33 | 148.84 | 0.4956 | 660.0 | 598.3 | |
| 2.56 | 2.98 | 1.48 | 1.72 | -25.49 | 75.68 | -17.53 | 147.92 | 0.5140 | -898.2 | -801.2 | |
| 0.00 | 0.85 | 0.00 | 0.49 | -25.65 | 75.59 | -17.62 | 147.97 | 0.5168 | -518.0 | -527.6 | |
| 0.00 | 1.45 | 0.00 | 0.84 | -25.32 | 75.57 | -17.64 | 147.57 | 0.5129 | -790.0 | -586.2 | |
| 0.00 | 1.88 | 0.00 | 1.09 | -25.49 | 74.85 | -18.36 | 146.76 | 0.5207 | -879.0 | -659.9 | |
| 0.00 | 1.53 | 0.00 | 0.90 | -25.98 | 74.29 | -18.92 | 146.57 | 0.5312 | -491.0 | -484.2 | |
| 0.00 | 1.96 | 0.00 | 1.14 | -25.75 | 74.33 | -18.88 | 146.35 | 0.5282 | -785.0 | -612.9 | |
| 0.00 | 1.28 | 0.00 | 0.75 | -25.79 | 74.08 | -19.13 | 146.06 | 0.5306 | -574.0 | -475.9 | |
| 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. | |