SDO HMI 2014-12-06 20:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.15 | 0.00 | 11.17 | -14.84 | 37.07 | 13.61 | 221.22 | 0.3461 | -311.1 | -313.9 | |
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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 | 0.53 | -20.99 | 43.64 | 20.18 | 221.74 | 0.4858 | -788.0 | -610.9 | |
| 0.00 | 1.53 | 0.00 | 0.85 | -19.91 | 40.81 | 17.35 | 219.23 | 0.4452 | 702.0 | 591.1 | |
| 0.00 | 1.28 | 0.00 | 0.68 | -14.83 | 39.78 | 16.32 | 226.39 | 0.3769 | 417.0 | 455.8 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -15.80 | 38.65 | 15.19 | 222.48 | 0.3749 | 778.0 | 645.1 | |
| 0.00 | 0.85 | 0.00 | 0.45 | -15.56 | 38.41 | 14.95 | 222.50 | 0.3694 | 806.0 | 705.2 | |
| 0.00 | 1.11 | 0.00 | 0.59 | -14.88 | 37.82 | 14.36 | 222.70 | 0.3551 | 771.0 | 586.5 | |
| 0.00 | 1.11 | 0.00 | 0.58 | -12.90 | 36.95 | 13.49 | 225.14 | 0.3222 | -826.0 | -672.8 | |
| 0.00 | 1.28 | 0.00 | 0.67 | -13.17 | 36.84 | 13.38 | 224.30 | 0.3241 | -809.0 | -584.7 | |
| 0.00 | 0.94 | 0.00 | 0.49 | -12.75 | 36.69 | 13.23 | 224.94 | 0.3175 | -785.0 | -549.9 | |
| 0.00 | 3.67 | 0.00 | 1.91 | -13.02 | 36.05 | 12.59 | 222.94 | 0.3133 | -829.0 | -735.4 | |
| 0.00 | 0.85 | 0.00 | 0.45 | -14.36 | 35.53 | 12.07 | 218.91 | 0.3240 | -953.0 | -810.7 | |
| 0.00 | 2.73 | 0.00 | 1.43 | -15.46 | 35.28 | 11.82 | 216.22 | 0.3356 | -608.0 | -648.6 | |
| 0.00 | 1.28 | 0.00 | 0.67 | -14.63 | 35.02 | 11.56 | 217.18 | 0.3222 | -905.0 | -658.6 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -14.88 | 34.91 | 11.45 | 216.44 | 0.3243 | -777.0 | -659.4 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -10.78 | 33.59 | 10.13 | 222.26 | 0.2581 | -861.0 | -674.9 | |
| 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. | |