| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.28 | 270.55 | 81.33 | 490.69 | 15.94 | 228.01 | -73.87 | 74.03 | 0.9587 | -280.3 | -49.5 | |
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back to the solar disc SDO HMI 2011-11-20 16:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.63 | 138.79 | 22.15 | 187.85 | 14.23 | 233.81 | -68.06 | 75.56 | 0.9301 | -772.0 | -165.1 | |
| 5.74 | -1.00 | 7.88 | -1.00 | 14.30 | 233.18 | -68.70 | 75.52 | 0.9340 | -213.3 | 999999 | |
| 1.03 | -1.00 | 1.43 | -1.00 | 14.32 | 232.82 | -69.05 | 75.52 | 0.9361 | 116.0 | 999999 | |
| 4.29 | 7.97 | 5.88 | 10.97 | 12.65 | 233.02 | -68.86 | 77.30 | 0.9345 | -259.0 | -27.3 | |
| 0.26 | -4.00 | 0.35 | -4.00 | 12.35 | 233.10 | -68.77 | 77.61 | 0.9339 | 20.7 | 999999 | |
| 1.11 | -4.00 | 1.54 | -4.00 | 12.34 | 232.85 | -69.02 | 77.63 | 0.9354 | -89.4 | 999999 | |
| 1.03 | 39.78 | 2.05 | 81.66 | 16.39 | 226.28 | -75.59 | 73.65 | 0.9695 | 523.2 | -26.9 | |
| 0.00 | 0.69 | 0.00 | 1.49 | 17.45 | 224.93 | -76.95 | 72.59 | 0.9749 | 279.0 | 218.6 | |
| 0.00 | 0.77 | 0.00 | 1.49 | 15.76 | 226.74 | -75.13 | 74.28 | 0.9675 | 137.0 | 211.7 | |
| 6.52 | -7.00 | 13.12 | -7.00 | 16.04 | 226.05 | -75.83 | 74.01 | 0.9704 | 385.5 | 999999 | |
| 7.72 | 78.78 | 18.85 | 199.70 | 17.68 | 223.40 | -78.47 | 72.41 | 0.9803 | -411.3 | 36.6 | |
| 2.49 | -7.00 | 5.15 | -7.00 | 15.93 | 225.65 | -76.22 | 74.14 | 0.9720 | -343.4 | 999999 | |
| 1.46 | 3.77 | 2.93 | 7.53 | 15.12 | 226.06 | -75.81 | 74.96 | 0.9702 | -141.9 | 9.2 | |
| 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. | |