| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 51.04 | 302.57 | 45.79 | 269.03 | 9.51 | 55.54 | -56.06 | 81.02 | 0.8294 | -599.7 | -243.2 | |
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back to the solar disc SDO HMI 2011-11-07 19:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.54 | 249.54 | 24.38 | 215.15 | 9.28 | 56.95 | -54.66 | 81.25 | 0.8167 | -987.2 | -234.6 | |
| 4.40 | 10.26 | 3.85 | 9.00 | 12.01 | 56.10 | -55.50 | 77.98 | 0.8264 | 453.5 | -67.2 | |
| 0.00 | 0.60 | 0.00 | 0.52 | 10.34 | 56.42 | -55.18 | 79.99 | 0.8223 | -481.0 | -393.3 | |
| 4.14 | -1.00 | 3.60 | -1.00 | 9.69 | 56.16 | -55.44 | 80.79 | 0.8246 | -390.0 | 999999 | |
| 1.72 | -1.00 | 1.50 | -1.00 | 9.39 | 56.18 | -55.42 | 81.15 | 0.8243 | -404.7 | 999999 | |
| 1.72 | -1.00 | 1.49 | -1.00 | 8.77 | 56.32 | -55.28 | 81.90 | 0.8227 | -283.9 | 999999 | |
| 0.00 | 0.60 | 0.00 | 0.54 | 11.19 | 54.87 | -56.73 | 79.05 | 0.8375 | -551.0 | -571.1 | |
| 7.50 | 35.53 | 7.67 | 36.17 | 9.49 | 50.37 | -61.23 | 81.20 | 0.8769 | -677.3 | -462.8 | |
| 2.16 | -8.00 | 2.21 | -8.00 | 9.07 | 50.24 | -61.36 | 81.69 | 0.8778 | -419.6 | 999999 | |
| 0.00 | 0.86 | 0.00 | 1.07 | 12.39 | 44.97 | -66.63 | 78.10 | 0.9180 | 373.0 | 315.2 | |
| 0.00 | 1.12 | 0.00 | 1.41 | 12.88 | 44.48 | -67.13 | 77.58 | 0.9214 | 425.0 | 425.0 | |
| 0.86 | 1.90 | 1.09 | 2.40 | 12.66 | 44.43 | -67.17 | 77.82 | 0.9216 | 350.0 | 464.0 | |
| 0.00 | 2.16 | 0.00 | 2.77 | 12.85 | 44.09 | -67.51 | 77.62 | 0.9239 | 274.0 | 142.9 | |
| 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. | |