SDO HMI 2014-02-27 19:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.98 | 36.02 | 3.73 | 19.01 | 7.73 | 135.26 | -13.22 | 40.33 | 0.3446 | 138.1 | 55.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.29 | 0.00 | 0.66 | 6.59 | 141.88 | -6.60 | 25.69 | 0.2647 | -948.0 | -797.1 | |
| 0.00 | 2.93 | 0.00 | 1.50 | 6.41 | 141.55 | -6.93 | 27.10 | 0.2645 | -926.0 | -831.6 | |
| 0.00 | 2.76 | 0.00 | 1.42 | 6.23 | 141.29 | -7.20 | 28.31 | 0.2639 | -862.0 | -630.2 | |
| 0.69 | 3.70 | 0.36 | 1.91 | 6.84 | 140.01 | -8.48 | 31.25 | 0.2833 | -1206.2 | -914.4 | |
| 0.00 | 1.21 | 0.00 | 0.62 | 7.08 | 139.89 | -8.60 | 31.18 | 0.2880 | -742.0 | -610.1 | |
| 0.00 | 1.38 | 0.00 | 0.71 | 6.29 | 139.84 | -8.65 | 32.81 | 0.2771 | -743.0 | -643.1 | |
| 0.00 | 2.50 | 0.00 | 1.32 | 7.10 | 133.68 | -14.80 | 46.24 | 0.3526 | 909.0 | 776.7 | |
| 0.00 | 0.69 | 0.00 | 0.36 | 7.05 | 133.40 | -15.08 | 46.88 | 0.3553 | 787.0 | 677.6 | |
| 3.45 | 5.69 | 1.84 | 3.04 | 8.76 | 132.94 | -15.55 | 44.42 | 0.3802 | 1056.8 | 854.4 | |
| 0.00 | 3.36 | 0.00 | 1.79 | 7.64 | 132.45 | -16.03 | 47.47 | 0.3732 | 818.0 | 709.4 | |
| 0.00 | 2.15 | 0.00 | 1.16 | 8.80 | 131.81 | -16.68 | 46.37 | 0.3935 | 513.0 | 398.8 | |
| 2.84 | 4.31 | 1.53 | 2.32 | 8.43 | 131.67 | -16.82 | 47.30 | 0.3911 | 1043.1 | 783.9 | |
| 0.00 | 2.84 | 0.00 | 1.54 | 9.48 | 130.89 | -17.59 | 46.67 | 0.4116 | 601.0 | 453.8 | |
| 0.00 | 1.21 | 0.00 | 0.66 | 8.48 | 129.74 | -18.74 | 50.32 | 0.4147 | 866.0 | 652.8 | |
| 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. | |