| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.79 | 162.63 | 41.14 | 270.64 | 17.94 | 60.10 | -72.92 | 72.40 | 0.9540 | -100.0 | -24.4 | |
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back to the solar disc SDO HMI 2011-11-06 04:58:59 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.33 | 119.11 | 3.30 | 178.21 | 16.97 | 63.32 | -69.70 | 73.32 | 0.9380 | -608.8 | -146.3 | |
| 2.59 | -1.00 | 3.66 | -1.00 | 16.60 | 63.27 | -69.75 | 73.72 | 0.9382 | -657.8 | 999999 | |
| 5.10 | -1.00 | 7.38 | -1.00 | 17.00 | 62.74 | -70.27 | 73.32 | 0.9413 | -598.8 | 999999 | |
| 2.50 | -1.00 | 3.76 | -1.00 | 16.92 | 61.96 | -71.06 | 73.43 | 0.9456 | -394.6 | 999999 | |
| 2.42 | -1.00 | 3.75 | -1.00 | 17.47 | 61.35 | -71.67 | 72.86 | 0.9490 | -236.1 | 999999 | |
| 0.86 | -1.00 | 1.35 | -1.00 | 17.46 | 61.16 | -71.86 | 72.88 | 0.9500 | 91.6 | 999999 | |
| 3.20 | -1.00 | 5.20 | -1.00 | 17.88 | 60.42 | -72.60 | 72.46 | 0.9538 | -169.2 | 999999 | |
| 0.00 | 3.97 | 0.00 | 6.31 | 17.32 | 60.88 | -72.14 | 73.04 | 0.9514 | 93.0 | -6.8 | |
| 0.00 | 0.95 | 0.00 | 1.71 | 18.70 | 58.59 | -74.43 | 71.65 | 0.9626 | -93.0 | -17.9 | |
| 0.00 | 4.58 | 0.00 | 7.59 | 17.26 | 59.99 | -73.03 | 73.12 | 0.9558 | 454.0 | 372.6 | |
| 0.00 | 1.12 | 0.00 | 2.29 | 19.61 | 56.59 | -76.43 | 70.75 | 0.9711 | 496.0 | 506.2 | |
| 0.00 | 1.55 | 0.00 | 3.21 | 19.40 | 56.34 | -76.68 | 70.96 | 0.9720 | 592.0 | 553.4 | |
| 5.79 | 31.35 | 12.74 | 71.32 | 19.82 | 55.40 | -77.62 | 70.55 | 0.9756 | 455.7 | 181.2 | |
| 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. | |