SDO HMI 2011-12-23 10:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.82 | 310.91 | 85.77 | 825.91 | 19.03 | 307.92 | 77.60 | 289.85 | 0.9809 | 3.7 | 1.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.88 | 140.10 | 35.82 | 491.92 | 19.05 | 310.51 | 80.19 | 289.60 | 0.9894 | -517.5 | -91.0 | |
| 2.30 | 6.97 | 4.98 | 15.33 | 16.47 | 305.96 | 75.63 | 287.41 | 0.9746 | 251.4 | 12.9 | |
| 0.00 | 0.94 | 0.00 | 1.98 | 16.76 | 305.55 | 75.23 | 287.75 | 0.9732 | 321.0 | 259.0 | |
| 0.00 | 1.02 | 0.00 | 2.81 | 19.77 | 308.62 | 78.29 | 290.50 | 0.9846 | -503.0 | -497.7 | |
| 0.00 | 0.94 | 0.00 | 2.05 | 18.11 | 305.96 | 75.64 | 289.09 | 0.9753 | 100.0 | 75.5 | |
| 0.00 | 1.19 | 0.00 | 2.58 | 17.98 | 305.79 | 75.47 | 288.97 | 0.9747 | 284.0 | 215.2 | |
| 0.00 | 6.38 | 0.00 | 17.43 | 20.21 | 308.45 | 78.12 | 290.96 | 0.9842 | -467.0 | -436.5 | |
| 4.08 | 149.71 | 8.01 | 284.63 | 18.52 | 304.18 | 73.86 | 289.71 | 0.9687 | -293.8 | 206.8 | |
| 11.82 | -8.00 | 22.59 | -8.00 | 18.51 | 303.83 | 73.50 | 289.74 | 0.9672 | 582.7 | 999999 | |
| 0.00 | 1.02 | 0.00 | 2.10 | 19.55 | 304.87 | 74.55 | 290.68 | 0.9719 | -327.0 | -267.8 | |
| 0.00 | 2.64 | 0.00 | 5.08 | 19.92 | 303.73 | 73.40 | 291.20 | 0.9676 | 357.0 | 260.3 | |
| 0.94 | -8.00 | 1.72 | -8.00 | 19.58 | 302.99 | 72.67 | 290.95 | 0.9643 | 675.0 | 999999 | |
| 6.80 | -8.00 | 12.65 | -8.00 | 20.31 | 303.11 | 72.78 | 291.69 | 0.9652 | 465.7 | 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. | |