SDO HMI 2014-09-26 00:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.91 | 21.74 | 1.99 | 14.76 | 6.86 | 207.25 | -43.46 | 87.39 | 0.6856 | 6.9 | 63.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.97 | 0.00 | 0.62 | 7.04 | 211.21 | -39.50 | 87.36 | 0.6342 | -480.0 | -365.7 | |
| 0.00 | 1.94 | 0.00 | 1.27 | 6.29 | 209.65 | -41.06 | 88.41 | 0.6554 | -700.0 | -555.6 | |
| 0.00 | 1.68 | 0.00 | 1.10 | 7.05 | 209.37 | -41.34 | 87.23 | 0.6585 | -728.0 | -618.0 | |
| 1.24 | 2.03 | 0.81 | 1.34 | 6.45 | 209.35 | -41.35 | 88.15 | 0.6592 | -616.3 | -521.9 | |
| 0.00 | 1.59 | 0.00 | 1.05 | 5.81 | 208.97 | -41.74 | 89.07 | 0.6647 | -698.0 | -537.7 | |
| 0.00 | 0.80 | 0.00 | 0.53 | 6.61 | 208.77 | -41.94 | 87.85 | 0.6667 | -503.0 | -409.2 | |
| 0.00 | 0.97 | 0.00 | 0.65 | 6.90 | 208.25 | -42.46 | 87.38 | 0.6732 | -613.0 | -496.3 | |
| 0.00 | 1.33 | 0.00 | 0.91 | 6.49 | 206.49 | -44.21 | 87.85 | 0.6957 | 658.0 | 533.2 | |
| 0.35 | 2.65 | 0.25 | 1.84 | 6.67 | 205.83 | -44.87 | 87.53 | 0.7037 | 692.8 | 534.2 | |
| 0.35 | 5.39 | 0.25 | 3.77 | 7.16 | 205.52 | -45.19 | 86.82 | 0.7073 | 785.5 | 630.2 | |
| 0.97 | -10.00 | 0.68 | -10.00 | 6.97 | 205.41 | -45.30 | 87.08 | 0.7087 | 641.5 | 999999 | |
| 0.00 | 0.80 | 0.00 | 0.56 | 7.35 | 205.28 | -45.43 | 86.53 | 0.7102 | 261.0 | 301.0 | |
| 0.00 | 0.88 | 0.00 | 0.62 | 8.71 | 204.87 | -45.84 | 84.60 | 0.7146 | 648.0 | 493.2 | |
| 0.00 | 0.71 | 0.00 | 0.50 | 7.92 | 204.46 | -46.25 | 85.69 | 0.7198 | 467.0 | 383.8 | |
| 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. | |