SDO HMI 2011-01-01 20:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.86 | 173.14 | 31.18 | 117.94 | 34.08 | 267.27 | 23.44 | 331.29 | 0.6883 | -126.0 | 8.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.28 | 85.51 | 13.29 | 59.06 | 33.42 | 270.04 | 26.21 | 328.00 | 0.6981 | -997.0 | -276.3 | |
| 0.00 | 1.10 | 0.00 | 0.76 | 33.61 | 269.12 | 25.29 | 329.04 | 0.6940 | -467.0 | -358.0 | |
| 4.42 | 11.46 | 3.00 | 7.80 | 33.38 | 268.58 | 24.75 | 329.35 | 0.6881 | -836.1 | -576.4 | |
| 1.87 | -3.00 | 1.27 | -3.00 | 33.60 | 268.46 | 24.62 | 329.67 | 0.6895 | -570.0 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.57 | 33.57 | 265.79 | 21.95 | 332.31 | 0.6727 | -700.0 | -643.0 | |
| 0.00 | 1.02 | 0.00 | 0.69 | 35.44 | 264.60 | 20.77 | 335.01 | 0.6862 | 305.0 | 279.5 | |
| 0.00 | 1.19 | 0.00 | 0.78 | 33.20 | 263.99 | 20.15 | 333.92 | 0.6580 | 667.0 | 552.6 | |
| 0.00 | 2.29 | 0.00 | 1.55 | 35.25 | 264.43 | 20.60 | 335.04 | 0.6832 | 361.0 | 366.5 | |
| 1.78 | 36.09 | 1.20 | 24.34 | 35.06 | 264.23 | 20.39 | 335.11 | 0.6800 | 728.5 | 281.5 | |
| 0.00 | 2.38 | 0.00 | 1.57 | 33.75 | 263.82 | 19.99 | 334.53 | 0.6632 | 614.0 | 627.2 | |
| 9.94 | -9.00 | 6.70 | -9.00 | 35.28 | 263.98 | 20.14 | 335.53 | 0.6811 | 705.5 | 999999 | |
| 6.28 | 31.25 | 4.19 | 20.82 | 34.71 | 263.45 | 19.61 | 335.66 | 0.6719 | 1006.1 | 612.8 | |
| 2.29 | -12.00 | 1.53 | -12.00 | 34.97 | 263.32 | 19.49 | 335.99 | 0.6741 | 786.2 | 999999 | |
| 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. | |