SDO HMI 2011-11-06 18:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.00 | 236.64 | 43.95 | 275.56 | 17.79 | 60.58 | -64.76 | 72.12 | 0.9046 | -152.0 | -109.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.86 | 171.07 | 0.89 | 181.09 | 16.64 | 64.11 | -61.23 | 73.12 | 0.8796 | -992.1 | -282.9 | |
| 4.83 | -1.00 | 5.03 | -1.00 | 16.81 | 63.89 | -61.45 | 72.94 | 0.8815 | -927.2 | 999999 | |
| 1.64 | -1.00 | 1.70 | -1.00 | 16.51 | 64.05 | -61.29 | 73.27 | 0.8800 | -840.6 | 999999 | |
| 1.98 | -1.00 | 2.10 | -1.00 | 17.22 | 63.46 | -61.88 | 72.52 | 0.8852 | -568.9 | 999999 | |
| 3.71 | -1.00 | 3.95 | -1.00 | 16.96 | 63.21 | -62.13 | 72.84 | 0.8869 | -564.3 | 999999 | |
| 2.33 | -1.00 | 2.47 | -1.00 | 16.62 | 63.33 | -62.01 | 73.20 | 0.8857 | -589.3 | 999999 | |
| 3.19 | -1.00 | 3.45 | -1.00 | 16.83 | 62.67 | -62.67 | 73.03 | 0.8909 | -340.8 | 999999 | |
| 1.47 | -1.00 | 1.61 | -1.00 | 16.99 | 62.23 | -63.11 | 72.88 | 0.8943 | -100.4 | 999999 | |
| 2.07 | -1.00 | 2.26 | -1.00 | 16.60 | 62.40 | -62.94 | 73.31 | 0.8929 | -310.9 | 999999 | |
| 0.00 | 0.95 | 0.00 | 1.01 | 15.05 | 63.19 | -62.15 | 74.99 | 0.8860 | 255.0 | 280.3 | |
| 3.71 | 5.09 | 4.21 | 5.79 | 17.46 | 61.30 | -64.04 | 72.43 | 0.9014 | -455.6 | -282.9 | |
| 2.50 | 34.25 | 3.50 | 49.21 | 19.64 | 55.98 | -69.36 | 70.44 | 0.9369 | 643.6 | 439.2 | |
| 6.47 | -12.00 | 9.40 | -12.00 | 19.84 | 55.13 | -70.21 | 70.27 | 0.9418 | 604.4 | 999999 | |
| 0.95 | 25.28 | 1.42 | 38.46 | 20.13 | 54.64 | -70.70 | 70.00 | 0.9445 | 236.0 | 101.5 | |
| 1.29 | -14.00 | 1.96 | -14.00 | 19.79 | 54.31 | -71.03 | 70.37 | 0.9462 | 233.8 | 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. | |