SDO HMI 2014-12-06 05:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.34 | 0.00 | 9.45 | -14.43 | 36.70 | 5.01 | 197.68 | 0.2730 | -351.8 | -303.7 | |
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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 | 1.62 | 0.00 | 0.83 | -11.42 | 42.09 | 10.40 | 221.20 | 0.2698 | -899.0 | -610.4 | |
| 0.00 | 1.19 | 0.00 | 0.63 | -17.07 | 40.59 | 8.90 | 206.44 | 0.3337 | 889.0 | 726.6 | |
| 0.00 | 1.28 | 0.00 | 0.68 | -19.00 | 40.34 | 8.65 | 203.35 | 0.3604 | 1024.0 | 778.5 | |
| 0.00 | 1.62 | 0.00 | 0.83 | -12.48 | 39.55 | 7.86 | 211.25 | 0.2586 | 889.0 | 563.5 | |
| 0.00 | 1.54 | 0.00 | 0.80 | -15.34 | 38.51 | 6.81 | 203.08 | 0.2932 | 792.0 | 575.1 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -15.00 | 35.67 | 3.98 | 194.31 | 0.2724 | -868.0 | -632.2 | |
| 0.00 | 2.90 | 0.00 | 1.49 | -14.81 | 35.45 | 3.76 | 193.72 | 0.2685 | -1041.0 | -871.1 | |
| 0.00 | 1.02 | 0.00 | 0.53 | -15.24 | 35.37 | 3.68 | 193.05 | 0.2752 | -750.0 | -578.9 | |
| 0.00 | 1.37 | 0.00 | 0.70 | -15.30 | 35.03 | 3.34 | 191.85 | 0.2750 | -896.0 | -773.2 | |
| 0.00 | 1.19 | 0.00 | 0.61 | -13.04 | 34.88 | 3.19 | 193.27 | 0.2371 | -864.0 | -647.7 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -14.84 | 34.78 | 3.09 | 191.32 | 0.2665 | -888.0 | -708.5 | |
| 0.00 | 0.94 | 0.00 | 0.47 | -11.20 | 32.27 | 0.58 | 182.85 | 0.1994 | -871.0 | -651.1 | |
| 0.00 | 1.62 | 0.00 | 0.83 | -13.04 | 31.00 | -0.69 | 177.06 | 0.2310 | -1091.0 | -861.6 | |
| 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. | |