| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.81 | 42.63 | 4.60 | 24.90 | 14.82 | 241.67 | -30.92 | 69.69 | 0.5318 | 146.0 | 78.3 | |
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back to the solar disc SDO HMI 2011-10-26 14:59:00 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.13 | 0.00 | 0.63 | 12.86 | 245.74 | -26.85 | 71.55 | 0.4662 | 736.0 | 597.8 | |
| 0.00 | 4.69 | 0.00 | 2.65 | 15.11 | 245.21 | -27.38 | 67.28 | 0.4834 | -922.0 | -710.8 | |
| 0.00 | 0.87 | 0.00 | 0.50 | 15.43 | 244.01 | -28.59 | 67.38 | 0.5017 | -352.0 | -332.7 | |
| 0.00 | 0.95 | 0.00 | 0.54 | 14.21 | 243.83 | -28.76 | 69.83 | 0.4989 | -543.0 | -385.9 | |
| 0.00 | 1.22 | 0.00 | 0.70 | 16.17 | 242.83 | -29.77 | 66.67 | 0.5214 | -294.0 | -321.4 | |
| 0.00 | 1.22 | 0.00 | 0.70 | 15.18 | 242.48 | -30.11 | 68.67 | 0.5218 | -696.0 | -548.4 | |
| 1.65 | 7.46 | 0.97 | 4.38 | 16.52 | 241.72 | -30.87 | 66.64 | 0.5380 | -683.9 | -483.7 | |
| 0.00 | 2.86 | 0.00 | 1.67 | 14.05 | 241.55 | -31.05 | 71.20 | 0.5306 | 293.0 | 346.6 | |
| 0.00 | 1.22 | 0.00 | 0.71 | 12.37 | 241.72 | -30.88 | 74.27 | 0.5229 | -649.0 | -462.1 | |
| 3.99 | 7.38 | 2.35 | 4.34 | 14.14 | 240.92 | -31.67 | 71.29 | 0.5397 | 870.1 | 670.6 | |
| 1.91 | 6.42 | 1.13 | 3.80 | 14.45 | 240.36 | -32.23 | 70.97 | 0.5484 | 825.7 | 566.6 | |
| 0.26 | -11.00 | 0.15 | -11.00 | 14.33 | 240.38 | -32.21 | 71.17 | 0.5478 | 875.7 | 999999 | |
| 0.00 | 6.08 | 0.00 | 3.61 | 14.65 | 239.93 | -32.66 | 70.80 | 0.5551 | 720.0 | 647.5 | |
| 0.00 | 1.13 | 0.00 | 0.67 | 14.88 | 239.78 | -32.81 | 70.45 | 0.5579 | 663.0 | 565.6 | |
| 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. | |