SDO HMI 2014-12-05 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 | 20.56 | 0.00 | 10.55 | -14.64 | 35.46 | -1.18 | 175.27 | 0.2614 | -526.2 | -497.3 | |
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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 | 1.36 | 0.00 | 0.69 | -12.61 | 39.81 | 3.17 | 193.59 | 0.2310 | 1012.0 | 845.0 | |
| 0.00 | 1.71 | 0.00 | 0.90 | -19.38 | 37.82 | 1.18 | 183.29 | 0.3389 | 765.0 | 467.7 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -14.09 | 36.42 | -0.22 | 179.15 | 0.2499 | -915.0 | -737.2 | |
| 0.00 | 4.78 | 0.00 | 2.45 | -14.82 | 35.63 | -1.01 | 176.25 | 0.2628 | -876.0 | -799.2 | |
| 0.00 | 1.36 | 0.00 | 0.70 | -13.57 | 35.39 | -1.25 | 174.95 | 0.2419 | -798.0 | -669.6 | |
| 0.00 | 2.73 | 0.00 | 1.40 | -15.16 | 35.07 | -1.57 | 174.35 | 0.2692 | -689.0 | -626.5 | |
| 0.00 | 1.19 | 0.00 | 0.61 | -15.07 | 34.74 | -1.90 | 173.11 | 0.2683 | -858.0 | -681.9 | |
| 0.00 | 1.54 | 0.00 | 0.79 | -16.30 | 34.39 | -2.25 | 172.47 | 0.2896 | -789.0 | -659.3 | |
| 0.00 | 1.11 | 0.00 | 0.57 | -15.16 | 34.40 | -2.24 | 171.95 | 0.2706 | -719.0 | -622.8 | |
| 0.00 | 1.62 | 0.00 | 0.83 | -12.96 | 34.36 | -2.28 | 170.43 | 0.2339 | -652.0 | -623.0 | |
| 0.00 | 1.11 | 0.00 | 0.56 | -10.49 | 33.33 | -3.31 | 163.16 | 0.1966 | -878.0 | -674.6 | |
| 0.00 | 0.94 | 0.00 | 0.48 | -12.20 | 32.34 | -4.30 | 161.33 | 0.2297 | -917.0 | -716.3 | |
| 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. | |