SDO HMI 2011-10-10 08:59:02 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.98 | 96.32 | 24.82 | 51.03 | 20.40 | 111.41 | -15.52 | 45.25 | 0.3549 | -19.8 | 176.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.75 | 0.00 | 0.94 | 22.51 | 111.80 | -15.13 | 40.32 | 0.3742 | 906.0 | 742.0 | |
| 31.47 | 80.37 | 16.59 | 42.49 | 20.03 | 111.93 | -15.00 | 45.11 | 0.3448 | -945.8 | -36.8 | |
| 1.40 | -2.00 | 0.74 | -2.00 | 20.33 | 111.86 | -15.06 | 44.56 | 0.3489 | 204.6 | 999999 | |
| 0.00 | 2.02 | 0.00 | 1.08 | 23.05 | 111.16 | -15.77 | 40.43 | 0.3872 | 878.0 | 551.5 | |
| 0.00 | 2.37 | 0.00 | 1.27 | 23.40 | 111.05 | -15.87 | 40.00 | 0.3923 | 888.0 | 602.0 | |
| 0.00 | 1.14 | 0.00 | 0.62 | 24.77 | 110.50 | -16.43 | 38.55 | 0.4138 | 722.0 | 613.7 | |
| 14.11 | -2.00 | 7.49 | -2.00 | 20.53 | 110.98 | -15.95 | 45.69 | 0.3611 | 921.4 | 999999 | |
| 0.00 | 0.96 | 0.00 | 0.51 | 19.32 | 110.84 | -16.09 | 48.57 | 0.3503 | 670.0 | 411.9 | |
| 0.00 | 0.79 | 0.00 | 0.42 | 19.62 | 109.65 | -17.28 | 49.79 | 0.3679 | 861.0 | 627.6 | |
| 0.00 | 1.14 | 0.00 | 0.61 | 20.08 | 109.53 | -17.40 | 48.97 | 0.3739 | 450.0 | 433.2 | |
| 0.00 | 0.96 | 0.00 | 0.51 | 19.89 | 109.45 | -17.48 | 49.50 | 0.3730 | 872.0 | 716.5 | |
| 0.00 | 0.88 | 0.00 | 0.47 | 19.70 | 109.31 | -17.62 | 50.12 | 0.3730 | 829.0 | 611.9 | |
| 0.00 | 3.94 | 0.00 | 2.11 | 19.95 | 109.14 | -17.78 | 49.84 | 0.3773 | 873.0 | 681.1 | |
| 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. | |