| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 9.55 | 48.47 | 9.78 | 49.74 | 16.74 | 178.44 | -56.78 | 66.32 | 0.8764 | -116.7 | 86.4 | |
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back to the solar disc SDO HMI 2011-02-26 04:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 3.53 | 0.00 | 3.51 | 17.34 | 179.69 | -55.53 | 65.23 | 0.8688 | -593.0 | -390.4 | |
| 2.24 | 18.52 | 2.17 | 18.08 | 15.53 | 179.87 | -55.35 | 67.14 | 0.8622 | 779.1 | 490.7 | |
| 0.00 | 0.60 | 0.00 | 0.61 | 17.45 | 178.97 | -56.25 | 65.37 | 0.8747 | -468.0 | -440.1 | |
| 2.15 | 3.10 | 2.13 | 3.06 | 16.02 | 179.44 | -55.78 | 66.75 | 0.8670 | 382.9 | 312.3 | |
| 0.00 | 0.43 | 0.00 | 0.46 | 19.00 | 177.84 | -57.39 | 64.11 | 0.8873 | -438.0 | -416.4 | |
| 0.00 | 0.60 | 0.00 | 0.62 | 17.06 | 178.41 | -56.81 | 65.98 | 0.8778 | -262.0 | -237.1 | |
| 3.70 | 8.27 | 3.86 | 8.65 | 17.37 | 177.98 | -57.24 | 65.80 | 0.8819 | -528.0 | -286.1 | |
| 0.00 | 1.72 | 0.00 | 1.88 | 18.95 | 177.09 | -58.13 | 64.42 | 0.8924 | -397.0 | -348.6 | |
| 0.00 | 0.86 | 0.00 | 0.99 | 20.42 | 175.91 | -59.31 | 63.27 | 0.9042 | -219.0 | -224.9 | |
| 0.00 | 1.89 | 0.00 | 1.95 | 15.90 | 177.98 | -57.25 | 67.40 | 0.8781 | 581.0 | 515.8 | |
| 1.46 | 3.27 | 1.62 | 3.63 | 18.79 | 176.45 | -58.77 | 64.80 | 0.8965 | -407.6 | -382.5 | |
| 0.00 | 1.46 | 0.00 | 1.53 | 16.01 | 177.52 | -57.70 | 67.42 | 0.8819 | 281.0 | 245.7 | |
| 0.00 | 0.34 | 0.00 | 0.39 | 17.64 | 175.49 | -59.73 | 66.33 | 0.9004 | -202.0 | -263.0 | |
| 0.00 | 3.88 | 0.00 | 4.38 | 17.22 | 175.29 | -59.93 | 66.85 | 0.9009 | -399.0 | -212.4 | |
| 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. | |