SDO HMI 2014-02-25 20:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.89 | 129.74 | 25.15 | 90.42 | 8.42 | 132.41 | -41.87 | 70.21 | 0.7036 | 520.5 | 216.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.64 | 0.00 | 0.99 | 7.28 | 142.37 | -31.90 | 66.24 | 0.5750 | -808.0 | -571.7 | |
| 0.00 | 1.64 | 0.00 | 1.00 | 7.41 | 141.05 | -33.23 | 66.94 | 0.5929 | -696.0 | -534.4 | |
| 0.00 | 1.21 | 0.00 | 0.75 | 8.09 | 140.12 | -34.16 | 66.50 | 0.6084 | -679.0 | -508.4 | |
| 0.00 | 1.55 | 0.00 | 0.97 | 8.26 | 139.85 | -34.43 | 66.41 | 0.6128 | -680.0 | -561.5 | |
| 0.00 | 0.95 | 0.00 | 0.60 | 8.92 | 139.71 | -34.57 | 65.52 | 0.6182 | -700.0 | -551.0 | |
| 0.00 | 1.38 | 0.00 | 0.91 | 7.57 | 135.27 | -39.01 | 70.02 | 0.6662 | -762.0 | -610.4 | |
| 0.00 | 1.21 | 0.00 | 0.82 | 6.82 | 133.27 | -41.00 | 72.02 | 0.6872 | -407.0 | -418.1 | |
| 0.00 | 1.03 | 0.00 | 0.71 | 7.29 | 132.78 | -41.49 | 71.60 | 0.6949 | 671.0 | 511.4 | |
| 9.38 | 32.54 | 6.52 | 22.64 | 8.70 | 132.49 | -41.79 | 69.83 | 0.7041 | 1004.1 | 404.1 | |
| 0.00 | 1.12 | 0.00 | 0.78 | 8.98 | 132.13 | -42.15 | 69.63 | 0.7094 | 221.0 | 230.2 | |
| 0.00 | 1.81 | 0.00 | 1.25 | 7.32 | 132.14 | -42.14 | 71.85 | 0.7027 | 602.0 | 524.3 | |
| 0.00 | 0.86 | 0.00 | 0.60 | 7.61 | 131.98 | -42.30 | 71.53 | 0.7056 | 537.0 | 424.5 | |
| 26.51 | 80.65 | 18.63 | 56.87 | 8.40 | 131.72 | -42.56 | 70.59 | 0.7118 | 810.0 | 231.3 | |
| 0.00 | 2.15 | 0.00 | 1.53 | 9.25 | 131.47 | -42.80 | 69.57 | 0.7180 | 400.0 | 351.4 | |
| 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. | |