SDO HMI 2014-03-10 15:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.04 | 76.68 | 14.90 | 39.29 | 6.66 | 10.72 | 4.95 | 340.49 | 0.2566 | 61.9 | 136.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.30 | 2.77 | 0.67 | 1.43 | 5.85 | 14.35 | 8.58 | 326.58 | 0.2705 | -963.4 | -819.1 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 5.97 | 14.14 | 8.37 | 327.47 | 0.2703 | -835.0 | -620.0 | |
| 0.00 | 1.30 | 0.00 | 0.67 | 6.11 | 13.57 | 7.79 | 329.56 | 0.2674 | -1042.0 | -824.7 | |
| 0.00 | 0.69 | 0.00 | 0.36 | 6.57 | 13.48 | 7.71 | 330.67 | 0.2734 | -920.0 | -747.6 | |
| 4.51 | 19.50 | 2.32 | 10.03 | 7.01 | 12.25 | 6.48 | 335.44 | 0.2707 | -1050.2 | -647.0 | |
| 5.98 | -5.00 | 3.08 | -5.00 | 7.13 | 12.01 | 6.24 | 336.42 | 0.2709 | -1071.2 | 999999 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 7.40 | 11.44 | 5.67 | 338.74 | 0.2715 | -929.0 | -658.0 | |
| 0.35 | 2.17 | 0.18 | 1.10 | 5.31 | 10.55 | 4.78 | 339.05 | 0.2329 | 1163.0 | 883.3 | |
| 0.43 | 2.69 | 0.22 | 1.37 | 5.46 | 10.34 | 4.57 | 340.12 | 0.2341 | 984.0 | 726.5 | |
| 0.00 | 1.73 | 0.00 | 0.89 | 6.93 | 10.29 | 4.52 | 342.23 | 0.2575 | 678.0 | 466.1 | |
| 2.86 | 10.14 | 1.47 | 5.20 | 7.39 | 10.09 | 4.32 | 343.50 | 0.2639 | -751.6 | -200.7 | |
| 2.25 | 9.18 | 1.15 | 4.68 | 5.88 | 9.80 | 4.03 | 342.84 | 0.2381 | 1031.0 | 843.7 | |
| 5.81 | 18.98 | 2.97 | 9.71 | 6.68 | 9.60 | 3.83 | 344.55 | 0.2501 | 1177.3 | 628.6 | |
| 4.94 | -13.00 | 2.53 | -13.00 | 6.89 | 9.57 | 3.80 | 344.89 | 0.2535 | 1040.1 | 999999 | |
| 0.61 | 2.77 | 0.31 | 1.42 | 6.40 | 8.82 | 3.04 | 347.35 | 0.2422 | 902.3 | 713.5 | |
| 0.00 | 2.34 | 0.00 | 1.19 | 6.18 | 8.79 | 3.01 | 347.29 | 0.2386 | 945.0 | 697.1 | |
| 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. | |