SDO HMI 2014-12-06 00:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.81 | 0.00 | 8.61 | -14.84 | 34.66 | 0.23 | 180.79 | 0.2629 | -826.6 | -702.4 | |
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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 | -15.16 | 35.71 | 1.28 | 184.63 | 0.2684 | -745.0 | -615.5 | |
| 0.00 | 2.13 | 0.00 | 1.09 | -14.89 | 35.65 | 1.22 | 184.49 | 0.2637 | -811.0 | -837.2 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -13.21 | 35.46 | 1.03 | 184.29 | 0.2350 | -982.0 | -784.0 | |
| 0.00 | 1.11 | 0.00 | 0.56 | -13.06 | 35.40 | 0.97 | 184.08 | 0.2324 | -1044.0 | -817.9 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -15.38 | 35.07 | 0.64 | 182.28 | 0.2713 | -789.0 | -650.5 | |
| 0.00 | 1.37 | 0.00 | 0.70 | -15.04 | 34.82 | 0.39 | 181.44 | 0.2655 | -958.0 | -826.1 | |
| 0.00 | 2.05 | 0.00 | 1.05 | -15.25 | 34.79 | 0.36 | 181.31 | 0.2691 | -707.0 | -520.5 | |
| 0.00 | 2.05 | 0.00 | 1.05 | -14.86 | 34.61 | 0.18 | 180.66 | 0.2623 | -935.0 | -732.1 | |
| 0.00 | 2.47 | 0.00 | 1.27 | -15.10 | 34.58 | 0.15 | 180.54 | 0.2665 | -565.0 | -612.9 | |
| 0.00 | 0.60 | 0.00 | 0.31 | -16.24 | 34.52 | 0.09 | 180.29 | 0.2856 | -819.0 | -668.1 | |
| 0.00 | 0.85 | 0.00 | 0.44 | -17.35 | 34.45 | 0.02 | 180.08 | 0.3042 | -622.0 | -529.2 | |
| 0.00 | 1.28 | 0.00 | 0.65 | -13.08 | 30.82 | -3.61 | 165.13 | 0.2402 | -942.0 | -841.7 | |
| 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. | |