SDO HMI 2014-12-06 10:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.77 | 0.00 | 11.90 | -15.83 | 37.30 | 8.34 | 205.67 | 0.3123 | -373.0 | -264.8 | |
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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 | 1.11 | 0.00 | 0.61 | -19.42 | 44.44 | 15.47 | 216.84 | 0.4214 | 722.0 | 576.5 | |
| 0.00 | 1.79 | 0.00 | 0.98 | -20.74 | 43.43 | 14.46 | 213.16 | 0.4288 | -960.0 | -734.7 | |
| 0.00 | 1.45 | 0.00 | 0.78 | -19.28 | 40.59 | 11.63 | 209.69 | 0.3857 | 887.0 | 714.5 | |
| 0.00 | 1.19 | 0.00 | 0.64 | -18.56 | 39.30 | 10.34 | 207.87 | 0.3655 | 785.0 | 553.6 | |
| 0.00 | 3.84 | 0.00 | 2.00 | -15.40 | 38.70 | 9.73 | 211.20 | 0.3160 | 863.0 | 665.0 | |
| 0.00 | 1.54 | 0.00 | 0.79 | -12.99 | 37.00 | 8.04 | 210.82 | 0.2671 | -788.0 | -543.6 | |
| 0.00 | 1.02 | 0.00 | 0.52 | -13.14 | 35.81 | 6.85 | 206.70 | 0.2596 | -911.0 | -777.1 | |
| 0.00 | 2.65 | 0.00 | 1.36 | -14.63 | 35.43 | 6.46 | 203.03 | 0.2796 | -1087.0 | -873.0 | |
| 0.00 | 1.19 | 0.00 | 0.62 | -15.12 | 35.35 | 6.38 | 202.09 | 0.2866 | -863.0 | -688.6 | |
| 0.00 | 2.47 | 0.00 | 1.28 | -15.21 | 35.13 | 6.17 | 201.30 | 0.2867 | -965.0 | -776.7 | |
| 0.00 | 1.45 | 0.00 | 0.75 | -14.72 | 34.84 | 5.88 | 201.03 | 0.2773 | -828.0 | -685.9 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -15.00 | 34.79 | 5.82 | 200.49 | 0.2813 | -817.0 | -688.2 | |
| 0.00 | 1.96 | 0.00 | 1.00 | -13.04 | 31.13 | 2.16 | 189.10 | 0.2332 | -887.0 | -666.1 | |
| 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. | |