| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.87 | 57.68 | 11.20 | 43.37 | 18.30 | 223.62 | 46.42 | 293.73 | 0.7536 | -288.1 | -203.5 | |
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back to the solar disc SDO HMI 2011-11-30 03:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.28 | 0.00 | 1.01 | 15.43 | 226.64 | 49.45 | 289.17 | 0.7777 | 614.0 | 489.0 | |
| 0.00 | 1.11 | 0.00 | 0.83 | 14.24 | 224.39 | 47.19 | 288.21 | 0.7510 | 474.0 | 364.6 | |
| 0.00 | 1.28 | 0.00 | 1.00 | 19.53 | 225.33 | 48.14 | 294.70 | 0.7749 | -289.0 | -290.3 | |
| 2.22 | 8.12 | 1.69 | 6.20 | 17.95 | 224.55 | 47.36 | 292.96 | 0.7623 | -674.5 | -478.9 | |
| 0.00 | 0.94 | 0.00 | 0.71 | 17.59 | 223.92 | 46.73 | 292.69 | 0.7547 | -571.0 | -506.6 | |
| 0.00 | 0.94 | 0.00 | 0.71 | 17.96 | 224.01 | 46.81 | 293.14 | 0.7566 | -616.0 | -583.5 | |
| 0.00 | 1.28 | 0.00 | 0.95 | 16.12 | 223.23 | 46.03 | 291.00 | 0.7430 | 393.0 | 254.5 | |
| 12.65 | 36.67 | 9.51 | 27.59 | 18.33 | 223.73 | 46.53 | 293.71 | 0.7548 | -818.8 | -304.6 | |
| 0.00 | 1.28 | 0.00 | 0.97 | 21.03 | 223.15 | 45.95 | 297.35 | 0.7577 | -614.0 | -518.7 | |
| 0.00 | 1.20 | 0.00 | 0.88 | 20.23 | 221.58 | 44.39 | 296.94 | 0.7386 | 456.0 | 401.6 | |
| 0.00 | 1.03 | 0.00 | 0.73 | 19.28 | 220.25 | 43.05 | 296.23 | 0.7207 | 521.0 | 447.4 | |
| 0.00 | 0.85 | 0.00 | 0.60 | 18.82 | 219.42 | 42.22 | 295.97 | 0.7099 | 686.0 | 621.0 | |
| 0.00 | 0.85 | 0.00 | 0.59 | 20.47 | 217.30 | 40.10 | 299.15 | 0.6934 | 594.0 | 487.2 | |
| 0.00 | 0.85 | 0.00 | 0.60 | 22.27 | 217.69 | 40.50 | 301.35 | 0.7060 | 594.0 | 531.7 | |
| 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. | |