SDO HMI 2014-07-09 22:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.82 | 40.86 | 5.20 | 30.93 | 7.79 | 251.95 | 49.24 | 277.04 | 0.7581 | 361.9 | 315.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.00 | 2.63 | 0.82 | 2.17 | 6.87 | 255.96 | 53.25 | 275.75 | 0.8017 | -526.8 | -368.1 | |
| 0.00 | 1.18 | 0.00 | 0.97 | 6.94 | 255.82 | 53.10 | 275.84 | 0.8002 | -398.0 | -405.9 | |
| 0.64 | 2.18 | 0.51 | 1.76 | 7.14 | 254.98 | 52.27 | 276.10 | 0.7914 | -708.4 | -597.1 | |
| 0.00 | 0.27 | 0.00 | 0.22 | 8.11 | 254.65 | 51.93 | 277.34 | 0.7881 | -542.0 | -625.0 | |
| 0.00 | 1.00 | 0.00 | 0.75 | 8.69 | 251.78 | 49.07 | 278.22 | 0.7568 | 391.0 | 315.7 | |
| 0.00 | 2.81 | 0.00 | 2.12 | 8.91 | 251.63 | 48.92 | 278.52 | 0.7553 | 696.0 | 562.9 | |
| 2.09 | 14.25 | 1.57 | 10.68 | 8.36 | 251.44 | 48.73 | 277.81 | 0.7528 | 658.8 | 402.5 | |
| 0.00 | 0.64 | 0.00 | 0.48 | 9.31 | 251.62 | 48.90 | 279.05 | 0.7553 | 369.0 | 450.3 | |
| 3.09 | 8.72 | 2.30 | 6.50 | 7.24 | 251.22 | 48.51 | 276.32 | 0.7499 | 672.7 | 482.2 | |
| 0.00 | 1.00 | 0.00 | 0.74 | 5.85 | 250.85 | 48.14 | 274.46 | 0.7454 | 471.0 | 322.0 | |
| 0.00 | 1.00 | 0.00 | 0.75 | 8.77 | 251.28 | 48.57 | 278.36 | 0.7512 | 558.0 | 503.8 | |
| 0.00 | 1.45 | 0.00 | 1.08 | 8.45 | 250.99 | 48.28 | 277.95 | 0.7477 | 649.0 | 486.7 | |
| 0.00 | 2.36 | 0.00 | 1.73 | 6.21 | 250.39 | 47.68 | 274.95 | 0.7400 | 669.0 | 529.3 | |
| 0.00 | 0.64 | 0.00 | 0.46 | 6.56 | 250.20 | 47.49 | 275.42 | 0.7379 | 611.0 | 507.3 | |
| 0.00 | 0.73 | 0.00 | 0.52 | 9.67 | 249.28 | 46.57 | 279.73 | 0.7286 | 601.0 | 479.8 | |
| 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. | |