SDO HMI 2014-12-06 07:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.77 | 0.00 | 11.22 | -14.91 | 35.78 | 5.18 | 197.83 | 0.2778 | -461.0 | -433.5 | |
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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 | 0.49 | -17.02 | 40.56 | 9.96 | 209.16 | 0.3410 | 912.0 | 731.9 | |
| 0.00 | 1.79 | 0.00 | 0.96 | -19.32 | 40.44 | 9.84 | 205.73 | 0.3730 | 863.0 | 630.8 | |
| 0.00 | 1.62 | 0.00 | 0.84 | -15.38 | 38.59 | 7.99 | 206.48 | 0.3019 | 952.0 | 728.7 | |
| 0.00 | 1.45 | 0.00 | 0.74 | -13.15 | 35.73 | 5.13 | 200.64 | 0.2483 | -951.0 | -715.2 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -15.19 | 35.53 | 4.93 | 197.33 | 0.2798 | -709.0 | -531.3 | |
| 0.00 | 2.90 | 0.00 | 1.49 | -14.77 | 35.46 | 4.86 | 197.58 | 0.2726 | -931.0 | -861.3 | |
| 0.00 | 2.05 | 0.00 | 1.06 | -15.22 | 35.26 | 4.66 | 196.39 | 0.2789 | -688.0 | -614.1 | |
| 0.00 | 2.73 | 0.00 | 1.41 | -15.29 | 35.04 | 4.44 | 195.61 | 0.2789 | -891.0 | -744.9 | |
| 0.00 | 1.54 | 0.00 | 0.79 | -14.98 | 34.91 | 4.31 | 195.49 | 0.2734 | -992.0 | -793.9 | |
| 0.00 | 1.88 | 0.00 | 0.97 | -14.79 | 34.82 | 4.22 | 195.35 | 0.2700 | -955.0 | -756.4 | |
| 0.00 | 1.11 | 0.00 | 0.56 | -10.64 | 34.15 | 3.55 | 197.90 | 0.1990 | -779.0 | -575.7 | |
| 0.00 | 1.11 | 0.00 | 0.56 | -12.30 | 33.90 | 3.30 | 194.53 | 0.2251 | -866.0 | -587.5 | |
| 0.00 | 1.37 | 0.00 | 0.69 | -13.02 | 31.03 | 0.43 | 181.81 | 0.2303 | -958.0 | -818.0 | |
| 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. | |