SDO HMI 2011-12-23 08:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.15 | 332.79 | 103.29 | 804.76 | 19.19 | 307.81 | 76.40 | 290.14 | 0.9770 | 38.5 | 4.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.37 | 152.11 | 30.76 | 474.21 | 19.02 | 310.49 | 79.08 | 289.66 | 0.9865 | -592.8 | -90.9 | |
| 2.30 | -1.00 | 6.78 | -1.00 | 19.46 | 310.46 | 79.04 | 290.11 | 0.9866 | -400.4 | 999999 | |
| 3.40 | 7.40 | 6.87 | 15.06 | 16.46 | 305.97 | 74.55 | 287.52 | 0.9704 | 293.5 | 18.1 | |
| 0.00 | 1.87 | 0.00 | 3.67 | 16.79 | 305.51 | 74.09 | 287.91 | 0.9687 | 237.0 | 161.9 | |
| 0.00 | 1.11 | 0.00 | 2.34 | 17.70 | 306.54 | 75.13 | 288.72 | 0.9732 | -191.0 | -188.5 | |
| 0.00 | 1.87 | 0.00 | 3.92 | 18.03 | 306.35 | 74.93 | 289.08 | 0.9726 | -21.0 | -61.5 | |
| 0.00 | 1.36 | 0.00 | 3.39 | 19.71 | 308.56 | 77.14 | 290.55 | 0.9811 | -583.0 | -542.0 | |
| 0.00 | 5.27 | 0.00 | 13.23 | 20.15 | 308.56 | 77.14 | 291.00 | 0.9812 | -587.0 | -483.9 | |
| 4.25 | 161.29 | 7.84 | 288.10 | 18.55 | 304.22 | 72.80 | 289.87 | 0.9642 | -342.6 | 224.2 | |
| 12.41 | -9.00 | 22.30 | -9.00 | 18.51 | 303.86 | 72.44 | 289.88 | 0.9626 | 594.9 | 999999 | |
| 0.00 | 0.51 | 0.00 | 0.84 | 17.59 | 302.33 | 70.91 | 289.12 | 0.9548 | -223.0 | -212.8 | |
| 4.34 | -9.00 | 7.48 | -9.00 | 19.77 | 302.96 | 71.55 | 291.30 | 0.9594 | 513.2 | 999999 | |
| 6.89 | -9.00 | 12.06 | -9.00 | 20.38 | 303.13 | 71.72 | 291.90 | 0.9606 | 523.6 | 999999 | |
| 5.19 | -9.00 | 9.20 | -9.00 | 21.30 | 303.19 | 71.78 | 292.84 | 0.9615 | 410.1 | 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. | |