| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.94 | 132.18 | 25.37 | 93.91 | 33.90 | 267.75 | 28.30 | 326.69 | 0.7183 | -8.7 | -51.9 | |
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back to the solar disc SDO HMI 2011-01-02 04:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.87 | 78.59 | 10.72 | 56.77 | 33.36 | 270.20 | 30.75 | 324.02 | 0.7293 | -957.9 | -279.0 | |
| 0.00 | 0.59 | 0.00 | 0.43 | 33.48 | 269.30 | 29.85 | 324.88 | 0.7241 | -563.0 | -483.0 | |
| 2.89 | 5.86 | 2.05 | 4.15 | 33.31 | 268.55 | 29.10 | 325.36 | 0.7173 | -725.6 | -492.4 | |
| 0.00 | 1.02 | 0.00 | 0.71 | 33.03 | 267.88 | 28.44 | 325.67 | 0.7103 | -704.0 | -540.2 | |
| 0.00 | 1.27 | 0.00 | 0.89 | 35.12 | 264.37 | 24.92 | 330.73 | 0.7073 | 459.0 | 344.6 | |
| 3.48 | 4.08 | 2.42 | 2.83 | 34.85 | 264.08 | 24.63 | 330.77 | 0.7029 | 625.4 | 580.9 | |
| 0.00 | 2.89 | 0.00 | 1.96 | 33.57 | 263.30 | 23.85 | 330.43 | 0.6850 | 862.0 | 728.2 | |
| 8.84 | 17.42 | 6.14 | 12.11 | 35.21 | 263.52 | 24.08 | 331.60 | 0.7032 | 683.4 | 367.0 | |
| 0.00 | 1.78 | 0.00 | 1.22 | 34.46 | 263.13 | 23.68 | 331.35 | 0.6931 | 882.0 | 686.4 | |
| 0.00 | 1.44 | 0.00 | 0.99 | 34.60 | 262.98 | 23.53 | 331.61 | 0.6937 | 973.0 | 798.1 | |
| 0.00 | 1.10 | 0.00 | 0.76 | 34.71 | 262.86 | 23.41 | 331.83 | 0.6941 | 826.0 | 730.1 | |
| 2.21 | 16.14 | 1.52 | 11.09 | 34.89 | 262.72 | 23.27 | 332.11 | 0.6952 | 954.3 | 647.9 | |
| 3.65 | -12.00 | 2.52 | -12.00 | 35.12 | 262.66 | 23.22 | 332.35 | 0.6972 | 626.1 | 999999 | |
| 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. | |