SDO HMI 2011-08-18 14:59:09 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.46 | 107.20 | 14.44 | 89.18 | -20.83 | 56.84 | -46.59 | 122.29 | 0.8052 | 442.8 | 205.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.05 | 94.78 | 10.75 | 78.39 | -20.90 | 57.35 | -46.08 | 122.62 | 0.8011 | 818.2 | 240.0 | |
| 2.88 | -1.00 | 2.41 | -1.00 | -21.16 | 56.72 | -46.71 | 122.59 | 0.8078 | 537.8 | 999999 | |
| 1.53 | -1.00 | 1.28 | -1.00 | -20.93 | 56.67 | -46.75 | 122.30 | 0.8071 | 402.4 | 999999 | |
| 0.00 | 1.17 | 0.00 | 0.98 | -20.77 | 56.21 | -47.21 | 121.89 | 0.8104 | -174.0 | -111.2 | |
| 0.00 | 1.35 | 0.00 | 1.10 | -18.43 | 56.87 | -46.55 | 119.57 | 0.7942 | 492.0 | 475.2 | |
| 0.00 | 0.90 | 0.00 | 0.73 | -18.58 | 56.63 | -46.80 | 119.63 | 0.7971 | 549.0 | 471.5 | |
| 0.00 | 1.26 | 0.00 | 1.05 | -19.49 | 56.15 | -47.28 | 120.43 | 0.8054 | 548.0 | 454.5 | |
| 0.00 | 0.99 | 0.00 | 0.83 | -19.93 | 55.83 | -47.59 | 120.76 | 0.8100 | 507.0 | 430.4 | |
| 0.00 | 0.90 | 0.00 | 0.75 | -19.13 | 55.76 | -47.66 | 119.83 | 0.8073 | 599.0 | 476.3 | |
| 0.00 | 0.99 | 0.00 | 0.84 | -19.63 | 55.08 | -48.34 | 120.07 | 0.8153 | 419.0 | 344.2 | |
| 0.00 | 0.90 | 0.00 | 0.82 | -20.40 | 52.60 | -50.83 | 119.79 | 0.8394 | -644.0 | -592.0 | |
| 0.00 | 0.45 | 0.00 | 0.41 | -20.81 | 52.20 | -51.23 | 120.06 | 0.8441 | -540.0 | -482.2 | |
| 0.00 | 1.35 | 0.00 | 1.26 | -20.99 | 51.74 | -51.68 | 120.06 | 0.8484 | -504.0 | -439.4 | |
| 0.00 | 2.16 | 0.00 | 2.02 | -20.75 | 51.44 | -51.99 | 119.67 | 0.8500 | -594.0 | -490.8 | |
| 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. | |