SDO HMI 2014-02-28 22:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 33.28 | 0.00 | 17.16 | 8.10 | 135.20 | 1.54 | 354.27 | 0.2795 | 284.4 | 244.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.07 | 0.00 | 1.08 | 8.14 | 143.19 | 9.53 | 328.09 | 0.3114 | -768.0 | -663.9 | |
| 0.00 | 1.03 | 0.00 | 0.53 | 4.98 | 142.73 | 9.07 | 323.17 | 0.2633 | -918.0 | -746.9 | |
| 0.00 | 2.50 | 0.00 | 1.29 | 6.50 | 142.52 | 8.86 | 327.02 | 0.2822 | -943.0 | -690.6 | |
| 0.00 | 3.62 | 0.00 | 1.86 | 6.90 | 140.77 | 7.11 | 333.16 | 0.2735 | -1007.0 | -836.0 | |
| 0.00 | 1.55 | 0.00 | 0.80 | 8.70 | 139.99 | 6.33 | 338.28 | 0.2958 | -818.0 | -659.8 | |
| 0.00 | 1.64 | 0.00 | 0.85 | 10.81 | 135.76 | 2.10 | 353.37 | 0.3129 | 963.0 | 782.8 | |
| 0.00 | 1.38 | 0.00 | 0.71 | 8.02 | 134.75 | 1.09 | 355.91 | 0.2647 | 814.0 | 637.9 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 7.83 | 134.60 | 0.94 | 356.43 | 0.2614 | 923.0 | 776.7 | |
| 0.00 | 2.07 | 0.00 | 1.06 | 7.12 | 134.57 | 0.91 | 356.38 | 0.2494 | 711.0 | 588.2 | |
| 0.00 | 0.86 | 0.00 | 0.44 | 7.92 | 133.16 | -0.50 | 1.90 | 0.2626 | 719.0 | 622.8 | |
| 0.00 | 1.90 | 0.00 | 0.97 | 7.52 | 132.92 | -0.74 | 2.88 | 0.2560 | 824.0 | 616.8 | |
| 0.00 | 2.41 | 0.00 | 1.25 | 9.81 | 132.32 | -1.34 | 4.51 | 0.2951 | 834.0 | 704.4 | |
| 0.00 | 1.12 | 0.00 | 0.58 | 8.36 | 131.90 | -1.76 | 6.46 | 0.2715 | 952.0 | 769.5 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 8.03 | 130.70 | -2.96 | 11.01 | 0.2690 | 791.0 | 591.4 | |
| 0.00 | 6.12 | 0.00 | 3.16 | 8.56 | 129.92 | -3.74 | 13.37 | 0.2805 | 574.0 | 801.9 | |
| 0.00 | 2.59 | 0.00 | 1.34 | 9.06 | 129.79 | -3.87 | 13.39 | 0.2891 | 900.0 | 718.4 | |
| 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. | |