SDO HMI 2014-12-06 09:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.08 | 0.00 | 9.48 | -16.37 | 37.80 | 8.29 | 204.39 | 0.3199 | -287.5 | -375.2 | |
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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 | 0.94 | 0.00 | 0.51 | -19.44 | 44.40 | 14.89 | 215.77 | 0.4163 | 788.0 | 624.8 | |
| 0.00 | 2.47 | 0.00 | 1.35 | -20.73 | 43.42 | 13.90 | 212.16 | 0.4240 | -976.0 | -690.6 | |
| 0.00 | 0.94 | 0.00 | 0.50 | -17.19 | 40.59 | 11.08 | 211.54 | 0.3524 | 867.0 | 663.3 | |
| 0.00 | 1.79 | 0.00 | 0.96 | -19.37 | 40.57 | 11.06 | 208.36 | 0.3825 | 855.0 | 745.4 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -19.03 | 40.39 | 10.87 | 208.43 | 0.3763 | 970.0 | 746.0 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -13.13 | 35.78 | 6.27 | 204.72 | 0.2553 | -890.0 | -766.5 | |
| 0.00 | 2.30 | 0.00 | 1.18 | -13.44 | 35.63 | 6.12 | 203.72 | 0.2590 | -920.0 | -787.7 | |
| 0.00 | 2.56 | 0.00 | 1.32 | -14.69 | 35.45 | 5.94 | 201.26 | 0.2772 | -1049.0 | -900.8 | |
| 0.00 | 2.13 | 0.00 | 1.10 | -15.21 | 35.12 | 5.61 | 199.54 | 0.2835 | -923.0 | -766.2 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -14.96 | 34.93 | 5.42 | 199.23 | 0.2785 | -884.0 | -736.5 | |
| 0.00 | 1.45 | 0.00 | 0.74 | -13.04 | 31.09 | 1.58 | 186.70 | 0.2319 | -1000.0 | -735.5 | |
| 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. | |