SDO HMI 2013-01-05 20:58:54 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.28 | 306.03 | 25.00 | 165.69 | -24.20 | 250.72 | -12.13 | 151.61 | 0.4043 | 759.9 | 316.2 | |
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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 | 0.44 | -20.54 | 256.09 | -6.76 | 159.30 | 0.3135 | -786.0 | -595.0 | |
| 46.28 | 284.80 | 25.00 | 153.96 | -24.22 | 251.12 | -11.73 | 152.32 | 0.4011 | 1499.7 | 404.2 | |
| 0.00 | 2.55 | 0.00 | 1.43 | -26.82 | 246.53 | -16.33 | 147.70 | 0.4714 | -692.0 | -535.7 | |
| 0.00 | 1.53 | 0.00 | 0.84 | -23.73 | 246.02 | -16.84 | 142.60 | 0.4385 | -755.0 | -737.1 | |
| 0.00 | 1.53 | 0.00 | 0.84 | -23.48 | 245.92 | -16.94 | 142.06 | 0.4365 | -795.0 | -700.7 | |
| 0.00 | 1.70 | 0.00 | 0.94 | -24.43 | 244.90 | -17.95 | 141.96 | 0.4574 | -771.0 | -553.2 | |
| 0.00 | 2.80 | 0.00 | 1.56 | -24.09 | 244.92 | -17.94 | 141.47 | 0.4532 | -885.0 | -716.8 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -24.78 | 244.81 | -18.04 | 142.34 | 0.4622 | -631.0 | -422.7 | |
| 0.00 | 1.02 | 0.00 | 0.57 | -24.75 | 244.65 | -18.21 | 142.05 | 0.4634 | -633.0 | -559.3 | |
| 0.00 | 1.36 | 0.00 | 0.75 | -23.17 | 244.71 | -18.14 | 139.75 | 0.4449 | -730.0 | -668.2 | |
| 0.00 | 2.97 | 0.00 | 1.64 | -23.39 | 244.61 | -18.24 | 139.94 | 0.4483 | -861.0 | -771.3 | |
| 0.00 | 2.21 | 0.00 | 1.21 | -22.23 | 244.51 | -18.35 | 137.92 | 0.4366 | -913.0 | -634.2 | |
| 0.00 | 1.44 | 0.00 | 0.80 | -23.35 | 244.18 | -18.68 | 139.25 | 0.4523 | -922.0 | -757.7 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
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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. |
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| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
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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. |
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| 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. | |