SDO HMI 2014-12-02 16:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.56 | 17.77 | 1.65 | 11.93 | -15.29 | 38.63 | -39.75 | 114.03 | 0.6767 | -113.8 | -18.4 | |
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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 |
| 1.96 | 6.15 | 1.25 | 3.92 | -16.44 | 42.81 | -35.58 | 117.68 | 0.6324 | 939.4 | 704.1 | |
| 0.00 | 0.51 | 0.00 | 0.34 | -15.63 | 40.05 | -38.33 | 115.02 | 0.6615 | 548.0 | 571.7 | |
| 0.60 | 2.65 | 0.40 | 1.77 | -15.12 | 38.90 | -39.48 | 113.74 | 0.6729 | 782.4 | 702.1 | |
| 0.00 | 0.43 | 0.00 | 0.29 | -14.51 | 38.44 | -39.94 | 112.67 | 0.6760 | 554.0 | 465.2 | |
| 0.00 | 0.77 | 0.00 | 0.53 | -14.40 | 36.36 | -42.03 | 111.66 | 0.7001 | -600.0 | -586.2 | |
| 0.00 | 1.28 | 0.00 | 0.89 | -14.65 | 36.26 | -42.13 | 111.96 | 0.7021 | -818.0 | -693.6 | |
| 0.00 | 0.60 | 0.00 | 0.41 | -14.28 | 36.34 | -42.04 | 111.49 | 0.6998 | -723.0 | -588.4 | |
| 0.00 | 0.94 | 0.00 | 0.65 | -14.86 | 36.16 | -42.22 | 112.22 | 0.7040 | -731.0 | -681.6 | |
| 0.00 | 2.05 | 0.00 | 1.43 | -14.99 | 35.80 | -42.59 | 112.24 | 0.7086 | -631.0 | -574.5 | |
| 0.00 | 1.37 | 0.00 | 0.97 | -14.08 | 34.38 | -44.00 | 110.49 | 0.7217 | -667.0 | -618.6 | |
| 0.00 | 1.02 | 0.00 | 0.73 | -14.26 | 34.21 | -44.18 | 110.68 | 0.7243 | -528.0 | -429.6 | |
| 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. | |