SDO HMI 2014-08-02 23:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 23.71 | 169.88 | 37.09 | 265.13 | 9.07 | 172.63 | -72.02 | 82.39 | 0.9483 | 196.4 | 82.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.90 | 0.00 | 1.11 | 10.69 | 177.80 | -66.85 | 80.90 | 0.9167 | -315.0 | -292.1 | |
| 4.07 | 25.15 | 4.98 | 30.72 | 10.05 | 177.91 | -66.73 | 81.60 | 0.9161 | -738.8 | -503.4 | |
| 0.00 | 1.54 | 0.00 | 1.92 | 9.85 | 177.35 | -67.29 | 81.80 | 0.9199 | -254.0 | -197.3 | |
| 0.00 | 0.36 | 0.00 | 0.47 | 9.91 | 176.42 | -68.22 | 81.69 | 0.9261 | -276.0 | -306.0 | |
| 0.00 | 0.54 | 0.00 | 0.78 | 11.20 | 173.99 | -70.65 | 80.21 | 0.9407 | 235.0 | 230.2 | |
| 0.00 | 1.00 | 0.00 | 1.43 | 10.81 | 174.11 | -70.53 | 80.63 | 0.9401 | 335.0 | 344.9 | |
| 0.00 | 1.63 | 0.00 | 2.40 | 11.18 | 173.52 | -71.12 | 80.20 | 0.9434 | 286.0 | 336.3 | |
| 0.00 | 2.80 | 0.00 | 4.25 | 11.23 | 173.00 | -71.64 | 80.14 | 0.9463 | -265.0 | -163.4 | |
| 0.00 | 9.23 | 0.00 | 13.37 | 9.25 | 173.96 | -70.69 | 82.28 | 0.9414 | 686.0 | 485.1 | |
| 0.00 | 0.63 | 0.00 | 0.92 | 8.67 | 174.03 | -70.61 | 82.90 | 0.9412 | 393.0 | 367.9 | |
| 1.00 | 62.51 | 1.54 | 103.91 | 9.13 | 172.75 | -71.90 | 82.34 | 0.9483 | 605.5 | 90.8 | |
| 0.00 | 0.81 | 0.00 | 1.32 | 10.60 | 171.62 | -73.02 | 80.73 | 0.9538 | 472.0 | 454.2 | |
| 5.34 | 62.78 | 8.48 | 102.53 | 8.61 | 172.18 | -72.46 | 82.85 | 0.9515 | 572.7 | 190.9 | |
| 1.45 | -11.00 | 2.31 | -11.00 | 9.02 | 171.98 | -72.67 | 82.41 | 0.9525 | 571.6 | 999999 | |
| 4.07 | -11.00 | 6.61 | -11.00 | 9.19 | 171.78 | -72.86 | 82.22 | 0.9534 | 566.2 | 999999 | |
| 5.16 | -13.00 | 8.66 | -13.00 | 8.42 | 171.21 | -73.44 | 82.99 | 0.9566 | 176.6 | 999999 | |
| 2.62 | -11.00 | 4.51 | -11.00 | 8.90 | 170.73 | -73.91 | 82.46 | 0.9588 | -166.6 | 999999 | |
| 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. | |