| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.98 | 52.23 | 11.51 | 30.47 | 7.43 | 265.31 | -31.60 | 79.40 | 0.5303 | -895.0 | -598.4 | |
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back to the solar disc SDO HMI 2011-11-21 01:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.98 | 35.34 | 11.51 | 20.33 | 7.50 | 266.57 | -30.34 | 78.95 | 0.5123 | -1118.1 | -625.7 | |
| 0.00 | 0.94 | 0.00 | 0.55 | 7.83 | 265.53 | -31.38 | 78.60 | 0.5283 | -631.0 | -441.9 | |
| 0.00 | 2.49 | 0.00 | 1.46 | 5.88 | 264.62 | -32.29 | 82.45 | 0.5381 | -879.0 | -678.4 | |
| 0.00 | 1.37 | 0.00 | 0.81 | 6.13 | 263.61 | -33.30 | 82.17 | 0.5531 | -759.0 | -570.1 | |
| 0.00 | 1.37 | 0.00 | 0.82 | 6.45 | 263.52 | -33.39 | 81.60 | 0.5550 | -742.0 | -628.4 | |
| 0.00 | 1.03 | 0.00 | 0.61 | 6.60 | 263.36 | -33.55 | 81.37 | 0.5574 | -594.0 | -457.9 | |
| 0.00 | 1.03 | 0.00 | 0.62 | 7.31 | 263.05 | -33.86 | 80.17 | 0.5630 | -740.0 | -568.8 | |
| 0.00 | 1.20 | 0.00 | 0.72 | 8.64 | 262.60 | -34.31 | 77.95 | 0.5720 | -764.0 | -674.7 | |
| 0.00 | 1.46 | 0.00 | 0.88 | 8.91 | 262.57 | -34.34 | 77.49 | 0.5730 | -707.0 | -581.0 | |
| 0.00 | 1.12 | 0.00 | 0.67 | 7.92 | 262.60 | -34.31 | 79.19 | 0.5706 | -675.0 | -622.8 | |
| 0.00 | 0.51 | 0.00 | 0.31 | 7.77 | 262.47 | -34.44 | 79.49 | 0.5721 | -631.0 | -633.2 | |
| 0.00 | 1.20 | 0.00 | 0.73 | 7.93 | 261.69 | -35.22 | 79.38 | 0.5834 | -507.0 | -414.0 | |
| 0.00 | 1.80 | 0.00 | 1.11 | 8.42 | 260.64 | -36.27 | 78.80 | 0.5988 | -765.0 | -603.4 | |
| 0.00 | 1.37 | 0.00 | 0.85 | 6.09 | 260.30 | -36.61 | 82.74 | 0.6000 | -672.0 | -471.9 | |
| 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. | |