SDO HMI 2014-03-10 18:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.98 | 79.44 | 14.38 | 40.83 | 6.60 | 10.83 | 6.71 | 334.27 | 0.2673 | 184.2 | 60.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.47 | 4.50 | 0.76 | 2.33 | 5.82 | 14.52 | 10.40 | 321.24 | 0.2881 | -1023.9 | -774.6 | |
| 0.00 | 0.87 | 0.00 | 0.45 | 6.11 | 13.92 | 9.80 | 323.53 | 0.2859 | -957.0 | -770.9 | |
| 0.00 | 1.21 | 0.00 | 0.63 | 6.38 | 13.71 | 9.59 | 324.67 | 0.2875 | -979.0 | -831.9 | |
| 0.00 | 0.95 | 0.00 | 0.49 | 6.06 | 12.94 | 8.82 | 326.25 | 0.2758 | -863.0 | -622.5 | |
| 7.62 | 20.27 | 3.94 | 10.46 | 6.85 | 12.50 | 8.38 | 329.10 | 0.2831 | -1113.9 | -750.4 | |
| 1.56 | -5.00 | 0.80 | -5.00 | 6.99 | 12.11 | 7.99 | 330.55 | 0.2820 | -849.6 | 999999 | |
| 0.00 | 2.17 | 0.00 | 1.12 | 7.26 | 11.82 | 7.70 | 331.93 | 0.2836 | -922.0 | -708.2 | |
| 0.00 | 1.82 | 0.00 | 0.93 | 5.29 | 10.52 | 6.40 | 332.80 | 0.2439 | 1092.0 | 904.0 | |
| 0.00 | 2.25 | 0.00 | 1.16 | 6.69 | 10.39 | 6.27 | 335.67 | 0.2644 | 934.0 | 638.6 | |
| 0.00 | 1.47 | 0.00 | 0.75 | 5.41 | 10.31 | 6.19 | 333.78 | 0.2441 | 1074.0 | 846.6 | |
| 2.34 | 4.33 | 1.20 | 2.23 | 7.33 | 10.09 | 5.97 | 337.62 | 0.2724 | -903.7 | -609.0 | |
| 0.00 | 3.38 | 0.00 | 1.73 | 6.81 | 9.94 | 5.82 | 337.41 | 0.2632 | 490.0 | 713.8 | |
| 0.95 | 4.33 | 0.49 | 2.21 | 5.83 | 9.77 | 5.65 | 336.49 | 0.2468 | 1086.1 | 881.2 | |
| 10.66 | 27.64 | 5.46 | 14.17 | 6.62 | 9.45 | 5.33 | 338.87 | 0.2572 | 1163.5 | 448.3 | |
| 2.69 | -14.00 | 1.38 | -14.00 | 6.89 | 9.43 | 5.31 | 339.34 | 0.2614 | 999.3 | 999999 | |
| 0.00 | 1.82 | 0.00 | 0.93 | 6.21 | 8.76 | 4.64 | 340.90 | 0.2467 | 1062.0 | 864.0 | |
| 0.69 | 2.43 | 0.35 | 1.24 | 6.49 | 8.70 | 4.58 | 341.48 | 0.2508 | 981.1 | 720.7 | |
| 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. | |