SDO HMI 2011-12-23 16:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.47 | 216.83 | 123.90 | 815.00 | 18.96 | 307.81 | 80.78 | 289.49 | 0.9893 | -21.7 | -12.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.87 | 85.48 | 8.89 | 492.05 | 17.68 | 310.09 | 83.06 | 288.00 | 0.9950 | -559.5 | -84.5 | |
| 1.36 | -1.00 | 6.41 | -1.00 | 18.48 | 309.93 | 82.90 | 288.82 | 0.9948 | -645.2 | 999999 | |
| 0.68 | 4.25 | 1.91 | 12.06 | 16.48 | 305.88 | 78.85 | 287.11 | 0.9852 | 234.2 | 84.9 | |
| 0.00 | 1.95 | 0.00 | 5.33 | 16.68 | 305.55 | 78.52 | 287.35 | 0.9843 | -326.0 | -140.3 | |
| 1.95 | -1.00 | 11.69 | -1.00 | 19.34 | 311.18 | 84.16 | 289.60 | 0.9968 | 323.6 | 999999 | |
| 7.90 | -1.00 | 39.33 | -1.00 | 19.06 | 310.25 | 83.22 | 289.38 | 0.9954 | -378.8 | 999999 | |
| 0.00 | 1.53 | 0.00 | 4.36 | 18.00 | 305.87 | 78.85 | 288.65 | 0.9856 | 82.0 | 41.9 | |
| 0.00 | 5.44 | 0.00 | 21.20 | 20.19 | 308.49 | 81.46 | 290.64 | 0.9924 | -441.0 | -387.5 | |
| 4.08 | 114.88 | 10.04 | 271.99 | 18.50 | 304.07 | 77.05 | 289.33 | 0.9804 | -371.2 | 156.8 | |
| 8.24 | -9.00 | 19.61 | -9.00 | 18.51 | 303.68 | 76.65 | 289.39 | 0.9791 | 455.5 | 999999 | |
| 0.00 | 1.78 | 0.00 | 4.36 | 20.03 | 303.89 | 76.86 | 290.91 | 0.9803 | 73.0 | 108.7 | |
| 6.97 | -9.00 | 15.89 | -9.00 | 19.68 | 302.95 | 75.92 | 290.66 | 0.9771 | 482.9 | 999999 | |
| 4.42 | -9.00 | 10.13 | -9.00 | 20.25 | 303.00 | 75.98 | 291.23 | 0.9775 | 397.3 | 999999 | |
| 0.00 | 0.59 | 0.00 | 1.41 | 21.02 | 303.26 | 76.23 | 291.99 | 0.9787 | 323.0 | 294.3 | |
| 0.00 | 0.93 | 0.00 | 2.24 | 21.22 | 303.44 | 76.42 | 292.17 | 0.9794 | 346.0 | 314.8 | |
| 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. | |