| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.23 | 112.36 | 22.76 | 78.01 | -25.32 | 87.34 | 35.07 | 227.84 | 0.7016 | 85.2 | 124.7 | |
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back to the solar disc SDO HMI 2011-11-12 07:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.77 | 0.00 | 0.57 | -25.30 | 91.44 | 39.17 | 230.80 | 0.7392 | -654.0 | -529.8 | |
| 14.55 | 86.19 | 10.26 | 60.82 | -25.17 | 88.81 | 36.54 | 229.19 | 0.7142 | 906.1 | 245.5 | |
| 2.32 | -2.00 | 1.64 | -2.00 | -25.50 | 88.52 | 36.24 | 228.60 | 0.7137 | 893.2 | 999999 | |
| 4.48 | -2.00 | 3.16 | -2.00 | -25.79 | 88.29 | 36.02 | 228.10 | 0.7137 | 720.1 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.72 | -25.48 | 88.14 | 35.87 | 228.35 | 0.7102 | 408.0 | 398.5 | |
| 0.00 | 1.03 | 0.00 | 0.71 | -25.81 | 85.88 | 33.61 | 226.28 | 0.6919 | -428.0 | -373.3 | |
| 0.00 | 1.38 | 0.00 | 0.94 | -25.69 | 85.37 | 33.10 | 226.01 | 0.6863 | -447.0 | -323.8 | |
| 0.00 | 1.38 | 0.00 | 0.93 | -25.48 | 84.91 | 32.64 | 225.90 | 0.6804 | -559.0 | -401.8 | |
| 0.00 | 2.32 | 0.00 | 1.50 | -24.51 | 81.92 | 29.64 | 224.48 | 0.6447 | -812.0 | -620.9 | |
| 0.00 | 1.12 | 0.00 | 0.74 | -26.45 | 82.26 | 29.99 | 222.52 | 0.6644 | -619.0 | -483.3 | |
| 2.24 | 15.33 | 1.45 | 9.93 | -25.10 | 81.43 | 29.16 | 223.33 | 0.6453 | -828.5 | -661.3 | |
| 9.64 | -11.00 | 6.25 | -11.00 | -25.40 | 81.40 | 29.13 | 222.95 | 0.6476 | -885.2 | 999999 | |
| 0.00 | 1.81 | 0.00 | 1.15 | -24.10 | 80.40 | 28.13 | 223.55 | 0.6268 | -572.0 | -545.5 | |
| 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. | |