SDO HMI 2014-07-18 06:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 18.25 | 72.55 | 9.62 | 38.25 | 6.93 | 112.44 | 20.00 | 277.52 | 0.3439 | 52.2 | 11.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.63 | 15.89 | 1.40 | 8.45 | 7.31 | 113.90 | 21.46 | 278.21 | 0.3682 | -974.9 | -750.5 | |
| 0.73 | -1.00 | 0.39 | -1.00 | 7.58 | 113.89 | 21.44 | 278.96 | 0.3684 | -892.8 | 999999 | |
| 3.09 | -1.00 | 1.64 | -1.00 | 7.22 | 113.70 | 21.26 | 278.03 | 0.3648 | -1118.2 | 999999 | |
| 0.00 | 12.80 | 0.00 | 6.79 | 6.93 | 113.46 | 21.01 | 277.28 | 0.3604 | -460.0 | -631.9 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 6.68 | 113.35 | 20.90 | 276.63 | 0.3582 | -706.0 | -563.4 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 7.03 | 112.87 | 20.42 | 277.74 | 0.3510 | 554.0 | 344.6 | |
| 0.00 | 1.09 | 0.00 | 0.58 | 7.95 | 112.79 | 20.34 | 280.37 | 0.3515 | -593.0 | -394.0 | |
| 0.00 | 1.82 | 0.00 | 0.96 | 7.78 | 112.51 | 20.07 | 279.98 | 0.3467 | -1083.0 | -895.8 | |
| 4.90 | 34.95 | 2.58 | 18.33 | 6.67 | 111.84 | 19.40 | 276.94 | 0.3337 | 996.5 | 663.3 | |
| 1.91 | -9.00 | 1.00 | -9.00 | 6.67 | 111.55 | 19.10 | 277.04 | 0.3290 | 995.1 | 999999 | |
| 3.99 | -9.00 | 2.09 | -9.00 | 6.89 | 111.46 | 19.02 | 277.73 | 0.3278 | 1005.2 | 999999 | |
| 1.00 | -9.00 | 0.52 | -9.00 | 6.57 | 111.09 | 18.65 | 276.83 | 0.3213 | 1181.3 | 999999 | |
| 0.00 | 3.09 | 0.00 | 1.61 | 6.78 | 111.00 | 18.56 | 277.53 | 0.3202 | 1033.0 | 905.4 | |
| 0.00 | 0.73 | 0.00 | 0.37 | 4.07 | 107.37 | 14.93 | 268.42 | 0.2582 | 333.0 | 252.6 | |
| 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. | |