| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.68 | 231.46 | 34.98 | 204.63 | 17.44 | 223.01 | -54.70 | 70.20 | 0.8297 | -429.4 | -149.3 | |
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back to the solar disc SDO HMI 2011-11-22 12:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.31 | 207.72 | 25.62 | 182.66 | 17.46 | 223.38 | -54.33 | 70.10 | 0.8264 | -810.9 | -209.2 | |
| 1.80 | -1.00 | 1.60 | -1.00 | 17.97 | 222.88 | -54.84 | 69.59 | 0.8319 | -508.5 | 999999 | |
| 3.34 | -1.00 | 3.00 | -1.00 | 18.02 | 222.37 | -55.35 | 69.64 | 0.8366 | -335.1 | 999999 | |
| 0.00 | 0.77 | 0.00 | 0.70 | 18.01 | 221.93 | -55.79 | 69.73 | 0.8405 | 248.0 | 211.3 | |
| 0.00 | 1.97 | 0.00 | 1.76 | 16.08 | 222.30 | -55.41 | 71.95 | 0.8342 | 217.0 | 237.3 | |
| 0.77 | 11.05 | 0.70 | 10.06 | 16.46 | 221.81 | -55.91 | 71.58 | 0.8393 | -173.6 | 263.4 | |
| 1.20 | -6.00 | 1.08 | -6.00 | 16.31 | 221.87 | -55.84 | 71.75 | 0.8384 | -203.6 | 999999 | |
| 3.26 | -6.00 | 2.98 | -6.00 | 16.51 | 221.45 | -56.27 | 71.58 | 0.8425 | 587.4 | 999999 | |
| 0.00 | 1.37 | 0.00 | 1.25 | 16.17 | 221.38 | -56.34 | 71.99 | 0.8427 | 433.0 | 357.2 | |
| 0.00 | 4.20 | 0.00 | 4.00 | 17.34 | 219.97 | -57.74 | 70.87 | 0.8565 | 686.0 | 566.0 | |
| 0.00 | 1.29 | 0.00 | 1.21 | 16.39 | 220.31 | -57.40 | 71.91 | 0.8524 | 607.0 | 552.5 | |
| 0.00 | 1.29 | 0.00 | 1.26 | 17.25 | 219.01 | -58.71 | 71.12 | 0.8645 | 490.0 | 442.4 | |
| 0.00 | 1.80 | 0.00 | 1.73 | 15.29 | 219.47 | -58.24 | 73.31 | 0.8584 | 481.0 | 383.2 | |
| 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. | |