SDO HMI 2014-07-07 11:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.36 | 42.33 | 4.86 | 21.98 | 7.33 | 252.35 | 17.08 | 283.34 | 0.3008 | 372.3 | 350.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.45 | 0.00 | 1.83 | 6.33 | 255.67 | 20.40 | 278.60 | 0.3518 | -776.0 | -583.2 | |
| 0.00 | 0.73 | 0.00 | 0.38 | 6.40 | 255.28 | 20.01 | 278.94 | 0.3457 | -621.0 | -591.1 | |
| 0.91 | 2.09 | 0.48 | 1.09 | 7.34 | 253.96 | 18.68 | 282.34 | 0.3266 | -1037.2 | -856.2 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 7.11 | 253.27 | 17.99 | 282.01 | 0.3147 | -746.0 | -490.5 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 7.12 | 253.07 | 17.80 | 282.14 | 0.3116 | -946.0 | -740.2 | |
| 4.54 | 8.90 | 2.36 | 4.63 | 7.95 | 252.56 | 17.28 | 285.14 | 0.3062 | 890.3 | 270.6 | |
| 0.00 | 1.54 | 0.00 | 0.80 | 7.38 | 252.34 | 17.07 | 283.43 | 0.3005 | 751.0 | 583.4 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 8.66 | 252.11 | 16.83 | 287.79 | 0.3020 | 812.0 | 737.6 | |
| 0.00 | 2.54 | 0.00 | 1.32 | 8.51 | 252.07 | 16.79 | 287.33 | 0.3007 | 1065.0 | 795.1 | |
| 0.00 | 2.18 | 0.00 | 1.13 | 8.02 | 252.02 | 16.74 | 285.79 | 0.2977 | 1132.0 | 906.2 | |
| 3.91 | 10.45 | 2.02 | 5.40 | 7.27 | 251.44 | 16.16 | 283.71 | 0.2855 | 1065.8 | 850.1 | |
| 0.00 | 1.73 | 0.00 | 0.89 | 7.03 | 251.11 | 15.84 | 283.12 | 0.2793 | 829.0 | 649.6 | |
| 0.00 | 2.00 | 0.00 | 1.03 | 5.88 | 250.91 | 15.64 | 279.10 | 0.2728 | 672.0 | 667.5 | |
| 0.00 | 0.82 | 0.00 | 0.42 | 6.89 | 250.76 | 15.48 | 282.86 | 0.2730 | 838.0 | 669.8 | |
| 0.00 | 2.18 | 0.00 | 1.12 | 6.40 | 250.58 | 15.30 | 281.21 | 0.2686 | 920.0 | 718.5 | |
| 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. | |