SDO HMI 2014-12-07 10:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.73 | 0.00 | 9.88 | -14.72 | 38.79 | 23.01 | 236.09 | 0.4584 | 220.2 | 248.7 | |
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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 | 0.68 | 0.00 | 0.40 | -14.89 | 45.71 | 29.92 | 241.83 | 0.5491 | 504.0 | 446.2 | |
| 0.00 | 0.85 | 0.00 | 0.48 | -12.45 | 40.67 | 24.88 | 242.18 | 0.4665 | 543.0 | 523.6 | |
| 0.00 | 2.39 | 0.00 | 1.39 | -19.37 | 41.22 | 25.43 | 230.59 | 0.5265 | 718.0 | 659.0 | |
| 0.00 | 0.85 | 0.00 | 0.49 | -19.46 | 40.72 | 24.93 | 229.92 | 0.5215 | 752.0 | 612.7 | |
| 0.00 | 1.62 | 0.00 | 0.90 | -12.81 | 39.54 | 23.76 | 240.42 | 0.4536 | 899.0 | 663.8 | |
| 0.00 | 2.30 | 0.00 | 1.29 | -15.64 | 38.82 | 23.04 | 234.29 | 0.4660 | 798.0 | 680.6 | |
| 0.00 | 1.28 | 0.00 | 0.71 | -15.52 | 38.68 | 22.89 | 234.34 | 0.4631 | 853.0 | 698.1 | |
| 0.00 | 1.88 | 0.00 | 1.02 | -10.99 | 37.55 | 21.76 | 242.19 | 0.4133 | 804.0 | 653.4 | |
| 0.00 | 1.19 | 0.00 | 0.65 | -12.74 | 37.05 | 21.26 | 237.89 | 0.4193 | -840.0 | -777.5 | |
| 0.00 | 0.60 | 0.00 | 0.33 | -15.52 | 37.05 | 21.26 | 232.43 | 0.4428 | 170.0 | 187.0 | |
| 0.00 | 2.05 | 0.00 | 1.11 | -12.92 | 36.74 | 20.95 | 237.15 | 0.4166 | -841.0 | -651.8 | |
| 0.00 | 1.19 | 0.00 | 0.65 | -14.05 | 36.12 | 20.33 | 234.10 | 0.4179 | -648.0 | -539.1 | |
| 0.00 | 0.85 | 0.00 | 0.46 | -13.53 | 35.30 | 19.51 | 234.08 | 0.4027 | -849.0 | -660.5 | |
| 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. | |