SDO HMI 2011-11-06 10:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 49.80 | 176.63 | 71.13 | 249.57 | 17.85 | 60.40 | -69.34 | 72.35 | 0.9342 | -162.3 | -10.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.51 | 124.58 | 23.96 | 157.97 | 16.85 | 63.44 | -66.30 | 73.27 | 0.9168 | -649.1 | -110.2 | |
| 0.69 | -1.00 | 0.88 | -1.00 | 17.22 | 62.37 | -67.37 | 72.93 | 0.9239 | -449.0 | 999999 | |
| 6.13 | -1.00 | 7.86 | -1.00 | 16.88 | 62.38 | -67.36 | 73.30 | 0.9237 | -457.7 | 999999 | |
| 2.76 | -1.00 | 3.59 | -1.00 | 17.23 | 62.04 | -67.71 | 72.94 | 0.9261 | -274.9 | 999999 | |
| 0.00 | 0.60 | 0.00 | 0.83 | 18.21 | 60.81 | -68.93 | 71.95 | 0.9339 | 295.0 | 283.7 | |
| 0.86 | -1.00 | 1.13 | -1.00 | 16.69 | 61.86 | -67.88 | 73.53 | 0.9270 | -220.0 | 999999 | |
| 5.18 | 8.12 | 7.07 | 11.13 | 17.56 | 60.83 | -68.91 | 72.64 | 0.9335 | -311.4 | 9.3 | |
| 2.16 | 42.30 | 3.69 | 77.71 | 19.47 | 56.27 | -73.47 | 70.81 | 0.9583 | 562.7 | 213.2 | |
| 8.37 | -8.00 | 15.08 | -8.00 | 19.78 | 55.29 | -74.45 | 70.51 | 0.9628 | 497.4 | 999999 | |
| 0.00 | 0.43 | 0.00 | 0.77 | 19.29 | 55.45 | -74.29 | 71.02 | 0.9621 | 153.0 | 208.0 | |
| 3.28 | -8.00 | 6.21 | -8.00 | 19.92 | 54.49 | -75.25 | 70.39 | 0.9663 | 180.5 | 999999 | |
| 0.86 | -8.00 | 1.66 | -8.00 | 19.94 | 54.21 | -75.53 | 70.38 | 0.9675 | -124.8 | 999999 | |
| 0.00 | 0.60 | 0.00 | 1.16 | 19.53 | 54.27 | -75.47 | 70.80 | 0.9672 | 10.0 | 58.7 | |
| 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. | |