SDO HMI 2011-12-23 14:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 38.06 | 243.12 | 113.22 | 802.11 | 19.05 | 307.93 | 79.80 | 289.66 | 0.9869 | -22.4 | -0.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.44 | 101.04 | 5.85 | 480.90 | 18.52 | 310.17 | 82.04 | 288.92 | 0.9933 | -683.3 | -86.9 | |
| 0.68 | 8.84 | 1.78 | 22.47 | 16.54 | 306.16 | 78.03 | 287.25 | 0.9828 | -137.6 | 85.2 | |
| 2.72 | -1.00 | 13.79 | -1.00 | 19.31 | 311.33 | 83.20 | 289.63 | 0.9954 | 328.7 | 999999 | |
| 9.43 | -1.00 | 40.09 | -1.00 | 19.06 | 310.36 | 82.23 | 289.44 | 0.9937 | -447.2 | 999999 | |
| 0.00 | 2.12 | 0.00 | 5.47 | 17.99 | 305.89 | 77.76 | 288.75 | 0.9825 | 149.0 | 69.5 | |
| 0.00 | 1.02 | 0.00 | 3.49 | 19.94 | 308.61 | 80.48 | 290.47 | 0.9903 | -495.0 | -473.1 | |
| 0.00 | 3.31 | 0.00 | 11.41 | 20.25 | 308.53 | 80.40 | 290.79 | 0.9901 | -455.0 | -414.9 | |
| 0.00 | 0.85 | 0.00 | 2.98 | 20.57 | 308.68 | 80.55 | 291.10 | 0.9905 | -296.0 | -277.9 | |
| 3.99 | 123.65 | 9.05 | 270.06 | 18.49 | 304.10 | 75.97 | 289.44 | 0.9767 | -340.0 | 190.7 | |
| 8.92 | -9.00 | 19.62 | -9.00 | 18.51 | 303.74 | 75.61 | 289.50 | 0.9754 | 474.5 | 999999 | |
| 0.00 | 1.10 | 0.00 | 2.67 | 19.71 | 304.79 | 76.66 | 290.61 | 0.9795 | -266.0 | -229.0 | |
| 0.00 | 1.19 | 0.00 | 2.66 | 19.93 | 303.78 | 75.65 | 290.94 | 0.9762 | 286.0 | 243.9 | |
| 6.12 | -9.00 | 12.90 | -9.00 | 19.74 | 302.89 | 74.76 | 290.85 | 0.9728 | 461.1 | 999999 | |
| 4.76 | -9.00 | 10.14 | -9.00 | 20.28 | 303.02 | 74.89 | 291.39 | 0.9736 | 380.6 | 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. | |