SDO HMI 2014-02-27 18:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.17 | 42.38 | 5.05 | 21.04 | -6.37 | 146.98 | -2.06 | 146.61 | 0.0431 | 49.6 | 409.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.45 | 13.44 | 1.71 | 6.66 | -6.83 | 149.42 | 0.38 | 313.64 | 0.0092 | 1228.6 | 950.8 | |
| 0.00 | 0.86 | 0.00 | 0.43 | -6.92 | 148.55 | -0.48 | 60.19 | 0.0097 | 873.0 | 751.6 | |
| 0.00 | 0.95 | 0.00 | 0.47 | -6.32 | 148.44 | -0.60 | 34.54 | 0.0185 | 954.0 | 778.2 | |
| 0.00 | 3.96 | 0.00 | 1.96 | -7.07 | 148.40 | -0.63 | 78.59 | 0.0112 | 768.0 | 819.5 | |
| 0.00 | 5.43 | 0.00 | 2.69 | -6.44 | 147.78 | -1.26 | 59.03 | 0.0256 | 676.0 | 592.8 | |
| 0.00 | 1.46 | 0.00 | 0.73 | -6.59 | 147.57 | -1.47 | 67.56 | 0.0277 | -60.0 | -54.2 | |
| 0.00 | 1.55 | 0.00 | 0.77 | -5.78 | 146.32 | -2.72 | 62.54 | 0.0534 | 912.0 | 644.8 | |
| 0.00 | 0.95 | 0.00 | 0.47 | -5.27 | 146.23 | -2.81 | 55.63 | 0.0593 | 1000.0 | 636.9 | |
| 0.00 | 0.86 | 0.00 | 0.43 | -6.19 | 145.78 | -3.26 | 72.99 | 0.0594 | -854.0 | -658.4 | |
| 0.00 | 1.29 | 0.00 | 0.64 | -6.45 | 144.91 | -4.13 | 79.98 | 0.0730 | -776.0 | -517.3 | |
| 1.64 | 11.63 | 0.81 | 5.79 | -5.90 | 143.54 | -5.50 | 77.01 | 0.0983 | -1180.2 | -895.7 | |
| 4.48 | -11.00 | 2.23 | -11.00 | -5.54 | 143.51 | -5.53 | 73.60 | 0.1004 | -1196.5 | 999999 | |
| 0.60 | -11.00 | 0.30 | -11.00 | -5.84 | 143.39 | -5.65 | 76.77 | 0.1011 | -941.3 | 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. | |