| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.94 | 181.15 | 35.27 | 181.89 | 19.21 | 193.25 | -59.20 | 68.82 | 0.8707 | -297.3 | -132.0 | |
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back to the solar disc SDO HMI 2011-11-24 10:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.03 | 153.14 | 1.00 | 148.08 | 19.40 | 194.47 | -57.98 | 68.40 | 0.8622 | -287.8 | -212.3 | |
| 25.78 | -1.00 | 24.90 | -1.00 | 18.74 | 194.53 | -57.92 | 69.14 | 0.8607 | -740.3 | 999999 | |
| 1.80 | -1.00 | 1.77 | -1.00 | 19.07 | 193.93 | -58.52 | 68.87 | 0.8661 | 309.9 | 999999 | |
| 1.54 | 3.17 | 1.56 | 3.21 | 18.64 | 192.83 | -59.62 | 69.55 | 0.8744 | -224.3 | -341.5 | |
| 0.00 | 2.74 | 0.00 | 2.82 | 19.16 | 192.46 | -59.99 | 69.02 | 0.8780 | -277.0 | -207.2 | |
| 0.00 | 0.86 | 0.00 | 0.92 | 19.72 | 191.20 | -61.25 | 68.60 | 0.8884 | 343.0 | 385.7 | |
| 1.54 | 5.65 | 1.85 | 6.76 | 21.37 | 188.02 | -64.43 | 67.26 | 0.9125 | 489.8 | 407.9 | |
| 1.11 | 1.71 | 1.37 | 2.11 | 21.77 | 187.39 | -65.06 | 66.93 | 0.9171 | 563.1 | 525.0 | |
| 0.00 | 0.86 | 0.00 | 1.09 | 22.19 | 186.54 | -65.91 | 66.59 | 0.9228 | 380.0 | 337.5 | |
| 0.00 | 1.20 | 0.00 | 1.51 | 21.69 | 186.76 | -65.69 | 67.10 | 0.9210 | 542.0 | 483.0 | |
| 0.00 | 2.06 | 0.00 | 2.57 | 21.41 | 186.93 | -65.52 | 67.38 | 0.9196 | 534.0 | 489.2 | |
| 0.00 | 0.86 | 0.00 | 1.11 | 22.18 | 185.99 | -66.46 | 66.68 | 0.9261 | 434.0 | 337.4 | |
| 2.14 | 5.65 | 2.82 | 7.48 | 21.98 | 185.53 | -66.92 | 66.95 | 0.9287 | 272.3 | 138.8 | |
| 0.00 | 1.03 | 0.00 | 1.28 | 20.21 | 186.86 | -65.59 | 68.69 | 0.9190 | 517.0 | 422.2 | |
| 0.00 | 1.11 | 0.00 | 1.47 | 21.59 | 185.48 | -66.97 | 67.37 | 0.9287 | 265.0 | 289.2 | |
| 0.00 | 1.11 | 0.00 | 1.48 | 21.40 | 185.26 | -67.19 | 67.61 | 0.9299 | 180.0 | 190.5 | |
| 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. | |