SDO HMI 2011-11-14 08:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.49 | 323.52 | 27.56 | 209.32 | 16.16 | 63.83 | 38.47 | 291.82 | 0.6460 | -775.6 | -316.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 41.72 | 311.65 | 27.06 | 202.00 | 16.06 | 64.03 | 38.67 | 291.57 | 0.6481 | -1198.9 | -340.2 | |
| 0.00 | 1.20 | 0.00 | 0.80 | 19.12 | 64.62 | 39.26 | 295.81 | 0.6666 | -617.0 | -550.3 | |
| 0.77 | -1.00 | 0.50 | -1.00 | 15.77 | 63.42 | 38.06 | 291.38 | 0.6394 | -1198.8 | 999999 | |
| 0.00 | 0.77 | 0.00 | 0.51 | 19.10 | 64.05 | 38.69 | 296.05 | 0.6598 | -424.0 | -374.2 | |
| 0.00 | 1.03 | 0.00 | 0.65 | 14.98 | 62.43 | 37.07 | 290.55 | 0.6242 | -785.0 | -548.2 | |
| 0.00 | 0.95 | 0.00 | 0.58 | 18.34 | 58.51 | 33.15 | 297.75 | 0.5888 | 574.0 | 478.2 | |
| 0.00 | 0.86 | 0.00 | 0.53 | 19.48 | 58.77 | 33.41 | 299.38 | 0.5980 | 692.0 | 522.4 | |
| 0.00 | 1.12 | 0.00 | 0.69 | 19.88 | 58.71 | 33.35 | 300.04 | 0.5995 | 610.0 | 442.7 | |
| 0.00 | 1.46 | 0.00 | 0.88 | 18.71 | 57.14 | 31.78 | 299.20 | 0.5737 | 673.0 | 517.9 | |
| 0.00 | 1.12 | 0.00 | 0.67 | 18.16 | 56.88 | 31.52 | 298.48 | 0.5674 | 797.0 | 703.0 | |
| 0.00 | 1.12 | 0.00 | 0.67 | 17.95 | 56.66 | 31.30 | 298.28 | 0.5633 | 806.0 | 592.0 | |
| 0.00 | 1.55 | 0.00 | 0.93 | 22.39 | 54.90 | 29.54 | 306.62 | 0.5702 | 514.0 | 529.2 | |
| 0.00 | 0.69 | 0.00 | 0.41 | 21.73 | 54.71 | 29.35 | 305.77 | 0.5634 | 718.0 | 561.2 | |
| 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. | |