SDO HMI 2014-12-07 06:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 61.60 | 354.43 | 31.95 | 183.79 | -3.64 | 1.14 | -16.82 | 102.78 | 0.2976 | 1091.9 | 393.2 | |
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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 | 1.11 | 0.00 | 0.56 | -4.72 | 5.83 | -12.14 | 111.87 | 0.2268 | -833.0 | -704.7 | |
| 0.00 | 2.90 | 0.00 | 1.48 | -5.20 | 5.28 | -12.69 | 112.88 | 0.2386 | 973.0 | 799.9 | |
| 0.00 | 1.37 | 0.00 | 0.70 | -5.20 | 5.06 | -12.91 | 112.54 | 0.2419 | 869.0 | 655.5 | |
| 0.00 | 1.37 | 0.00 | 0.71 | -6.50 | 2.27 | -15.70 | 113.15 | 0.2937 | -931.0 | -843.8 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -6.29 | 2.06 | -15.91 | 112.23 | 0.2957 | -911.0 | -716.5 | |
| 30.54 | 341.71 | 15.82 | 177.22 | -3.77 | 1.42 | -16.55 | 103.36 | 0.2935 | 1479.4 | 407.7 | |
| 31.06 | -6.00 | 16.13 | -6.00 | -3.45 | 0.77 | -17.19 | 101.84 | 0.3029 | 1367.2 | 999999 | |
| 0.00 | 0.68 | 0.00 | 0.35 | -1.97 | 0.52 | -17.45 | 96.86 | 0.3032 | 492.0 | 554.1 | |
| 0.00 | 0.51 | 0.00 | 0.27 | -4.60 | 0.28 | -17.69 | 105.14 | 0.3151 | 57.0 | 152.7 | |
| 0.00 | 1.45 | 0.00 | 0.76 | -1.58 | 359.93 | -18.03 | 95.42 | 0.3123 | -925.0 | -734.9 | |
| 0.00 | 2.39 | 0.00 | 1.25 | -4.30 | 359.13 | -18.83 | 103.41 | 0.3324 | 466.0 | 391.5 | |
| 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. | |