| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.43 | 238.06 | 48.75 | 369.08 | -13.78 | 120.17 | -69.44 | 106.19 | 0.9476 | 368.2 | 129.2 | |
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back to the solar disc SDO HMI 2011-11-01 21:58:59 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.58 | 142.82 | 6.25 | 200.56 | -14.69 | 123.01 | -66.60 | 107.63 | 0.9331 | 827.0 | 190.7 | |
| 13.15 | -1.00 | 18.51 | -1.00 | -15.02 | 122.32 | -67.29 | 107.84 | 0.9375 | 513.3 | 999999 | |
| 0.95 | -1.00 | 1.34 | -1.00 | -14.51 | 122.17 | -67.44 | 107.27 | 0.9378 | 454.5 | 999999 | |
| 1.99 | -1.00 | 2.80 | -1.00 | -14.26 | 122.16 | -67.45 | 107.00 | 0.9376 | 457.0 | 999999 | |
| 1.12 | -1.00 | 1.66 | -1.00 | -15.01 | 121.26 | -68.35 | 107.62 | 0.9435 | -344.5 | 999999 | |
| 1.90 | 3.11 | 2.81 | 4.60 | -13.45 | 120.92 | -68.69 | 105.93 | 0.9438 | 124.6 | 47.4 | |
| 0.00 | 1.04 | 0.00 | 1.87 | -15.96 | 117.66 | -71.96 | 107.98 | 0.9624 | -305.0 | -231.2 | |
| 0.00 | 3.37 | 0.00 | 6.00 | -15.61 | 117.76 | -71.85 | 107.64 | 0.9616 | -491.0 | -465.3 | |
| 0.00 | 0.52 | 0.00 | 0.85 | -13.59 | 118.95 | -70.66 | 105.75 | 0.9543 | -484.0 | -414.8 | |
| 0.00 | 3.20 | 0.00 | 5.15 | -13.14 | 119.16 | -70.45 | 105.32 | 0.9529 | -518.0 | -448.0 | |
| 1.12 | 22.06 | 2.08 | 40.89 | -15.41 | 117.01 | -72.60 | 107.32 | 0.9648 | 336.7 | 24.0 | |
| 1.21 | 1.90 | 2.19 | 3.44 | -14.85 | 117.39 | -72.22 | 106.81 | 0.9627 | -314.4 | -357.9 | |
| 0.00 | 0.35 | 0.00 | 0.59 | -13.48 | 117.97 | -71.64 | 105.48 | 0.9590 | -238.0 | -286.0 | |
| 0.00 | 0.95 | 0.00 | 1.65 | -13.00 | 117.72 | -71.89 | 104.95 | 0.9598 | -217.0 | -206.8 | |
| 0.00 | 0.52 | 0.00 | 1.17 | -15.67 | 114.00 | -75.61 | 107.13 | 0.9769 | 140.0 | 0.5 | |
| 5.80 | 55.80 | 10.01 | 97.91 | -10.95 | 117.58 | -72.03 | 102.81 | 0.9590 | 594.2 | 161.0 | |
| 0.61 | 2.42 | 1.10 | 4.40 | -9.41 | 116.53 | -73.08 | 101.08 | 0.9630 | 312.7 | 194.4 | |
| 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. | |