SDO HMI 2014-09-22 00:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.15 | 295.86 | 28.59 | 151.19 | 8.82 | 289.92 | -13.58 | 82.09 | 0.2406 | -580.3 | -369.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.59 | 0.00 | 0.80 | 15.70 | 296.56 | -6.94 | 37.65 | 0.1914 | -933.0 | -679.6 | |
| 0.00 | 1.24 | 0.00 | 0.62 | 11.27 | 293.86 | -9.64 | 65.52 | 0.1813 | -840.0 | -625.4 | |
| 0.00 | 1.77 | 0.00 | 0.89 | 10.02 | 293.53 | -9.97 | 72.66 | 0.1795 | -967.0 | -720.2 | |
| 0.00 | 1.42 | 0.00 | 0.72 | 10.88 | 292.75 | -10.75 | 69.50 | 0.1964 | -886.0 | -537.2 | |
| 0.00 | 1.42 | 0.00 | 0.71 | 4.86 | 292.69 | -10.81 | 101.05 | 0.1914 | 757.0 | 745.3 | |
| 0.00 | 1.42 | 0.00 | 0.71 | 7.20 | 292.58 | -10.92 | 88.65 | 0.1889 | -975.0 | -774.2 | |
| 0.00 | 2.13 | 0.00 | 1.08 | 10.90 | 292.25 | -11.25 | 70.18 | 0.2045 | -997.0 | -793.4 | |
| 0.00 | 1.24 | 0.00 | 0.63 | 5.43 | 292.40 | -11.10 | 97.88 | 0.1944 | -890.0 | -591.7 | |
| 0.00 | 1.33 | 0.00 | 0.67 | 9.78 | 291.89 | -11.61 | 75.96 | 0.2054 | -1040.0 | -751.2 | |
| 0.00 | 1.95 | 0.00 | 0.99 | 10.89 | 291.72 | -11.78 | 71.00 | 0.2130 | -868.0 | -649.4 | |
| 0.00 | 1.33 | 0.00 | 0.67 | 10.29 | 291.71 | -11.79 | 73.76 | 0.2103 | -725.0 | -517.6 | |
| 17.89 | 94.04 | 9.06 | 47.68 | 5.13 | 291.51 | -11.99 | 98.59 | 0.2102 | -1235.5 | -492.5 | |
| 1.95 | -12.00 | 0.99 | -12.00 | 5.46 | 291.44 | -12.06 | 96.98 | 0.2105 | -1113.5 | 999999 | |
| 2.66 | -12.00 | 1.35 | -12.00 | 5.64 | 291.41 | -12.09 | 96.11 | 0.2106 | -1024.8 | 999999 | |
| 0.00 | 1.06 | 0.00 | 0.54 | 3.95 | 291.04 | -12.47 | 103.50 | 0.2225 | 778.0 | 607.9 | |
| 0.00 | 1.42 | 0.00 | 0.73 | 18.61 | 290.39 | -13.11 | 46.65 | 0.2970 | -772.0 | -632.6 | |
| 0.00 | 0.62 | 0.00 | 0.32 | 17.66 | 290.33 | -13.17 | 49.31 | 0.2876 | -733.0 | -414.9 | |
| 29.84 | 156.11 | 15.23 | 79.72 | 10.96 | 289.93 | -13.57 | 72.83 | 0.2422 | -1275.7 | -446.9 | |
| 3.28 | -18.00 | 1.68 | -18.00 | 10.98 | 289.42 | -14.08 | 73.29 | 0.2505 | -900.7 | 999999 | |
| 0.00 | 1.51 | 0.00 | 0.77 | 9.29 | 289.31 | -14.19 | 80.08 | 0.2468 | 926.0 | 761.9 | |
| 0.00 | 2.04 | 0.00 | 1.04 | 11.24 | 289.09 | -14.41 | 72.61 | 0.2569 | -208.0 | -211.8 | |
| 0.53 | 2.39 | 0.28 | 1.24 | 5.12 | 286.07 | -17.43 | 95.46 | 0.3010 | 1063.2 | 840.8 | |
| 0.00 | 1.06 | 0.00 | 0.55 | 5.38 | 285.88 | -17.62 | 94.51 | 0.3037 | 660.0 | 563.5 | |
| 0.00 | 1.51 | 0.00 | 0.78 | 5.71 | 285.77 | -17.73 | 93.40 | 0.3049 | 756.0 | 630.6 | |
| 0.00 | 2.92 | 0.00 | 1.53 | 5.41 | 284.95 | -18.55 | 94.10 | 0.3189 | 902.0 | 818.8 | |
| 0.00 | 1.15 | 0.00 | 0.60 | 8.64 | 284.31 | -19.19 | 84.02 | 0.3282 | 858.0 | 671.6 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 5.76 | 283.95 | -19.55 | 92.73 | 0.3348 | 599.0 | 434.7 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 8.37 | 283.68 | -19.82 | 84.92 | 0.3383 | 735.0 | 593.0 | |
| 0.00 | 1.33 | 0.00 | 0.70 | 4.58 | 283.79 | -19.71 | 96.17 | 0.3396 | 740.0 | 452.4 | |
| 0.00 | 1.42 | 0.00 | 0.75 | 15.19 | 283.10 | -20.40 | 66.18 | 0.3694 | -923.0 | -737.6 | |
| 0.00 | 1.51 | 0.00 | 0.80 | 15.18 | 282.93 | -20.57 | 66.34 | 0.3718 | -753.0 | -602.4 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 4.14 | 283.29 | -20.21 | 97.22 | 0.3488 | 578.0 | 488.3 | |
| 0.00 | 1.06 | 0.00 | 0.56 | 8.43 | 282.99 | -20.51 | 84.82 | 0.3495 | 880.0 | 749.8 | |
| 0.00 | 1.86 | 0.00 | 0.99 | 8.30 | 281.89 | -21.61 | 85.31 | 0.3672 | 752.0 | 589.3 | |
| 0.00 | 1.42 | 0.00 | 0.85 | 0.53 | 269.90 | -33.60 | 99.58 | 0.5633 | 666.0 | 499.1 | |
| 0.00 | 1.68 | 0.00 | 1.02 | 9.08 | 268.09 | -35.41 | 84.26 | 0.5772 | 604.0 | 498.9 | |
| 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. | |