| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.57 | 92.11 | 18.19 | 81.22 | -16.95 | 340.84 | 53.25 | 247.81 | 0.8298 | 299.9 | 195.2 | |
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back to the solar disc SDO HMI 2011-11-21 18:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.37 | 2.06 | 1.33 | 2.00 | -16.96 | 344.56 | 56.97 | 248.83 | 0.8621 | 508.1 | 426.8 | |
| 0.00 | 2.74 | 0.00 | 2.59 | -16.49 | 343.62 | 56.03 | 249.12 | 0.8532 | 676.0 | 516.5 | |
| 0.00 | 3.08 | 0.00 | 2.91 | -16.77 | 343.52 | 55.93 | 248.78 | 0.8529 | 696.0 | 584.6 | |
| 3.94 | 21.42 | 3.53 | 19.17 | -16.61 | 341.55 | 53.96 | 248.43 | 0.8354 | -660.8 | -304.4 | |
| 1.46 | 2.23 | 1.32 | 2.02 | -17.96 | 341.77 | 54.18 | 246.92 | 0.8405 | -364.5 | -244.0 | |
| 0.00 | 0.77 | 0.00 | 0.69 | -18.04 | 341.11 | 53.52 | 246.64 | 0.8350 | -337.0 | -273.8 | |
| 12.77 | 50.04 | 11.13 | 43.51 | -16.76 | 340.36 | 52.77 | 247.91 | 0.8250 | 683.5 | 379.9 | |
| 0.00 | 2.83 | 0.00 | 2.45 | -18.52 | 339.56 | 51.97 | 245.59 | 0.8224 | 592.0 | 438.8 | |
| 1.03 | 1.71 | 0.88 | 1.47 | -18.20 | 339.12 | 51.53 | 245.83 | 0.8174 | 623.3 | 616.0 | |
| 0.00 | 1.80 | 0.00 | 1.55 | -18.71 | 339.28 | 51.69 | 245.29 | 0.8204 | 643.0 | 578.4 | |
| 0.00 | 0.77 | 0.00 | 0.66 | -18.42 | 339.11 | 51.52 | 245.57 | 0.8180 | 628.0 | 507.3 | |
| 0.00 | 1.29 | 0.00 | 1.07 | -18.93 | 337.44 | 49.85 | 244.39 | 0.8041 | -511.0 | -413.3 | |
| 0.00 | 1.37 | 0.00 | 1.13 | -19.12 | 337.27 | 49.68 | 244.10 | 0.8031 | -550.0 | -374.6 | |
| 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. | |