SDO HMI 2014-01-02 13:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.71 | 41.86 | 15.80 | 34.22 | -12.04 | 116.79 | -52.41 | 102.75 | 0.7953 | 456.6 | 225.3 | |
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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 | 0.51 | 0.00 | 0.41 | -17.44 | 118.66 | -50.54 | 109.83 | 0.7853 | 575.0 | 551.5 | |
| 0.00 | 1.10 | 0.00 | 0.87 | -14.88 | 118.60 | -50.60 | 106.58 | 0.7815 | 546.0 | 427.8 | |
| 11.05 | 22.77 | 8.54 | 17.59 | -11.35 | 119.27 | -49.93 | 102.15 | 0.7698 | 819.7 | 505.7 | |
| 0.76 | -3.00 | 0.59 | -3.00 | -11.49 | 119.05 | -50.15 | 102.31 | 0.7724 | 380.1 | 999999 | |
| 6.63 | 9.26 | 5.39 | 7.53 | -12.33 | 116.94 | -52.26 | 103.12 | 0.7956 | 609.0 | 374.1 | |
| 0.00 | 1.95 | 0.00 | 1.72 | -12.57 | 113.56 | -55.64 | 103.05 | 0.8293 | 329.0 | 283.1 | |
| 0.59 | 1.70 | 0.55 | 1.57 | -12.67 | 111.81 | -57.39 | 103.01 | 0.8456 | -613.4 | -537.7 | |
| 0.00 | 0.76 | 0.00 | 0.71 | -13.68 | 111.44 | -57.76 | 104.16 | 0.8497 | -456.0 | -491.7 | |
| 0.00 | 0.59 | 0.00 | 0.56 | -13.64 | 111.17 | -58.03 | 104.09 | 0.8521 | -490.0 | -448.7 | |
| 0.00 | 1.61 | 0.00 | 1.52 | -11.70 | 110.90 | -58.30 | 101.79 | 0.8532 | -478.0 | -394.8 | |
| 0.68 | 1.61 | 0.73 | 1.74 | -12.91 | 106.60 | -62.60 | 102.90 | 0.8897 | -331.4 | -259.5 | |
| 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. | |