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 |
| 23.27 | 75.19 | 12.00 | 38.63 | -6.94 | 149.01 | 15.35 | 270.21 | 0.2645 | 325.2 | 127.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.47 | 0.00 | 0.76 | -8.22 | 150.76 | 17.10 | 265.48 | 0.2932 | -794.0 | -593.8 | |
| 11.64 | 27.33 | 6.02 | 14.15 | -7.37 | 150.66 | 17.00 | 268.42 | 0.2914 | 1010.0 | 568.2 | |
| 7.24 | 16.73 | 3.74 | 8.63 | -7.12 | 150.06 | 16.40 | 269.32 | 0.2814 | 1150.2 | 808.8 | |
| 0.00 | 1.55 | 0.00 | 0.80 | -6.72 | 149.51 | 15.85 | 270.84 | 0.2726 | 750.0 | 587.4 | |
| 0.60 | 3.36 | 0.31 | 1.73 | -6.47 | 149.01 | 15.35 | 271.88 | 0.2644 | 1029.4 | 816.5 | |
| 0.52 | 1.47 | 0.27 | 0.75 | -6.36 | 148.76 | 15.10 | 272.37 | 0.2603 | 917.5 | 766.0 | |
| 0.00 | 1.38 | 0.00 | 0.70 | -4.72 | 146.88 | 13.22 | 280.02 | 0.2324 | -938.0 | -766.2 | |
| 0.00 | 9.22 | 0.00 | 4.69 | -5.26 | 146.79 | 13.13 | 277.79 | 0.2294 | -876.0 | -768.7 | |
| 1.98 | 4.40 | 1.01 | 2.24 | -5.74 | 146.74 | 13.08 | 275.75 | 0.2274 | -1010.8 | -752.3 | |
| 1.29 | 2.59 | 0.65 | 1.31 | -8.56 | 145.68 | 12.02 | 262.80 | 0.2086 | 796.3 | 592.5 | |
| 0.00 | 1.81 | 0.00 | 0.91 | -8.19 | 144.78 | 11.12 | 264.24 | 0.1928 | -1008.0 | -866.0 | |
| 0.00 | 1.64 | 0.00 | 0.83 | -8.96 | 144.75 | 11.09 | 260.22 | 0.1936 | -762.0 | -616.1 | |
| 0.00 | 1.21 | 0.00 | 0.61 | -8.31 | 144.60 | 10.94 | 263.52 | 0.1899 | -935.0 | -717.5 | |
| 0.00 | 1.03 | 0.00 | 0.52 | -5.59 | 144.42 | 10.76 | 278.07 | 0.1886 | -675.0 | -613.8 | |
| 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. | |