SDO HMI 2014-05-15 11:00:37 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.75 | 66.64 | 11.77 | 36.21 | 8.56 | 195.13 | -21.54 | 62.19 | 0.4119 | 109.5 | 186.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.43 | 19.22 | 5.04 | 10.28 | 8.09 | 197.37 | -19.30 | 60.73 | 0.3768 | -1065.8 | -715.9 | |
| 0.00 | 3.50 | 0.00 | 1.88 | 8.57 | 196.63 | -20.05 | 60.54 | 0.3909 | -878.0 | -712.7 | |
| 1.98 | 5.48 | 1.06 | 2.95 | 8.57 | 196.27 | -20.41 | 60.96 | 0.3960 | -734.0 | -554.3 | |
| 0.00 | 0.99 | 0.00 | 0.54 | 8.38 | 195.13 | -21.54 | 62.67 | 0.4107 | -616.0 | -440.2 | |
| 1.71 | 10.60 | 0.93 | 5.80 | 9.10 | 194.39 | -22.28 | 61.89 | 0.4262 | 1094.8 | 721.0 | |
| 0.00 | 0.90 | 0.00 | 0.49 | 9.82 | 194.14 | -22.53 | 60.67 | 0.4349 | 652.0 | 555.6 | |
| 0.00 | 2.60 | 0.00 | 1.43 | 9.27 | 194.02 | -22.66 | 61.95 | 0.4326 | 871.0 | 769.1 | |
| 0.90 | 4.85 | 0.49 | 2.66 | 9.02 | 193.97 | -22.71 | 62.51 | 0.4316 | 1064.2 | 824.5 | |
| 1.53 | -8.00 | 0.84 | -8.00 | 9.12 | 193.76 | -22.91 | 62.52 | 0.4351 | 829.8 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.44 | 8.38 | 193.51 | -23.17 | 64.31 | 0.4337 | 870.0 | 697.7 | |
| 0.00 | 1.44 | 0.00 | 0.79 | 8.72 | 193.45 | -23.22 | 63.64 | 0.4368 | 787.0 | 690.3 | |
| 4.85 | 16.25 | 2.67 | 8.95 | 8.35 | 193.21 | -23.47 | 64.64 | 0.4378 | 994.9 | 741.5 | |
| 1.35 | -12.00 | 0.74 | -12.00 | 8.57 | 193.06 | -23.61 | 64.32 | 0.4413 | 759.5 | 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. | |