SDO HMI 2014-08-01 13:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.68 | 0.00 | 9.51 | 14.00 | 257.50 | -5.90 | 185.09 | 0.2078 | 487.9 | 361.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.81 | 0.00 | 0.92 | 16.48 | 268.38 | 4.98 | 335.87 | 0.2044 | -747.0 | -624.0 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 16.15 | 267.42 | 4.01 | 339.51 | 0.1929 | -955.0 | -741.9 | |
| 0.00 | 1.45 | 0.00 | 0.73 | 15.84 | 267.22 | 3.82 | 339.85 | 0.1868 | -1000.0 | -803.2 | |
| 0.00 | 1.99 | 0.00 | 0.99 | 9.72 | 260.45 | -2.95 | 36.51 | 0.0857 | 942.0 | 805.4 | |
| 0.00 | 1.27 | 0.00 | 0.63 | 7.40 | 259.88 | -3.52 | 65.13 | 0.0674 | 1019.0 | 852.0 | |
| 0.00 | 1.63 | 0.00 | 0.81 | 8.98 | 259.38 | -4.03 | 51.16 | 0.0894 | 1008.0 | 799.4 | |
| 0.00 | 1.36 | 0.00 | 0.69 | 16.18 | 258.48 | -4.93 | 24.54 | 0.1995 | 915.0 | 689.8 | |
| 0.00 | 0.91 | 0.00 | 0.45 | 10.22 | 257.84 | -5.56 | 50.84 | 0.1235 | 876.0 | 638.1 | |
| 0.00 | 1.18 | 0.00 | 0.59 | 4.33 | 256.04 | -7.37 | 100.97 | 0.1308 | 942.0 | 743.5 | |
| 0.00 | 1.00 | 0.00 | 0.52 | 18.62 | 250.48 | -12.93 | 43.38 | 0.3100 | 764.0 | 635.4 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 18.73 | 249.68 | -13.73 | 44.78 | 0.3205 | 602.0 | 509.5 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 18.88 | 249.63 | -13.77 | 44.51 | 0.3227 | 817.0 | 726.7 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 21.07 | 247.89 | -15.52 | 43.09 | 0.3670 | 801.0 | 571.6 | |
| 0.00 | 1.00 | 0.00 | 0.54 | 13.56 | 239.85 | -23.55 | 69.74 | 0.4158 | 846.0 | 721.4 | |
| 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. | |