SDO HMI 2014-05-27 17:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.63 | 28.93 | 0.33 | 15.24 | -19.96 | 49.63 | -4.99 | 166.61 | 0.3362 | 498.0 | 425.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.35 | 0.00 | 0.70 | -17.89 | 53.01 | -1.61 | 174.69 | 0.2894 | 844.0 | 728.9 | |
| 0.00 | 1.53 | 0.00 | 0.80 | -18.90 | 52.62 | -2.00 | 173.79 | 0.3070 | 996.0 | 886.8 | |
| 0.00 | 0.81 | 0.00 | 0.42 | -18.68 | 52.56 | -2.06 | 173.52 | 0.3034 | 991.0 | 861.4 | |
| 0.63 | 8.57 | 0.33 | 4.46 | -18.93 | 51.85 | -2.77 | 171.45 | 0.3091 | 1122.4 | 844.9 | |
| 0.00 | 1.62 | 0.00 | 0.85 | -19.13 | 51.52 | -3.10 | 170.57 | 0.3131 | 889.0 | 758.9 | |
| 0.00 | 1.08 | 0.00 | 0.56 | -18.80 | 51.08 | -3.54 | 169.05 | 0.3092 | 778.0 | 656.2 | |
| 0.00 | 0.99 | 0.00 | 0.52 | -19.28 | 50.58 | -4.04 | 167.91 | 0.3186 | 691.0 | 399.4 | |
| 0.00 | 1.53 | 0.00 | 0.81 | -20.18 | 50.46 | -4.16 | 168.17 | 0.3335 | 768.0 | 663.1 | |
| 0.00 | 1.08 | 0.00 | 0.57 | -20.50 | 49.83 | -4.79 | 166.69 | 0.3409 | 651.0 | 520.8 | |
| 0.00 | 1.35 | 0.00 | 0.72 | -21.37 | 49.77 | -4.85 | 167.14 | 0.3550 | 783.0 | 667.9 | |
| 0.00 | 1.44 | 0.00 | 0.76 | -19.60 | 49.51 | -5.11 | 165.10 | 0.3279 | -918.0 | -752.6 | |
| 0.00 | 2.98 | 0.00 | 1.58 | -21.85 | 48.77 | -5.85 | 164.98 | 0.3666 | 844.0 | 697.8 | |
| 0.00 | 2.07 | 0.00 | 1.12 | -21.73 | 42.72 | -11.90 | 151.36 | 0.4015 | -754.0 | -647.8 | |
| 0.00 | 2.53 | 0.00 | 1.37 | -22.15 | 41.94 | -12.68 | 150.40 | 0.4132 | -919.0 | -775.0 | |
| 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. | |