| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 36.19 | 146.87 | 25.15 | 102.79 | 33.90 | 267.89 | 26.81 | 327.99 | 0.7082 | -7.6 | -92.9 | |
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back to the solar disc SDO HMI 2011-01-02 01:58:55 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.55 | 90.39 | 11.01 | 64.11 | 33.39 | 270.13 | 29.05 | 325.47 | 0.7175 | -956.0 | -276.2 | |
| 2.29 | 5.95 | 1.60 | 4.14 | 33.31 | 268.62 | 27.53 | 326.72 | 0.7064 | -735.3 | -679.0 | |
| 0.00 | 1.19 | 0.00 | 0.83 | 33.49 | 268.44 | 27.35 | 327.05 | 0.7069 | -665.0 | -506.6 | |
| 0.00 | 1.27 | 0.00 | 0.87 | 33.53 | 265.62 | 24.53 | 329.71 | 0.6887 | -669.0 | -535.3 | |
| 0.00 | 1.78 | 0.00 | 1.23 | 35.13 | 264.42 | 23.34 | 332.23 | 0.6978 | 446.0 | 281.2 | |
| 1.53 | 4.67 | 1.05 | 3.20 | 34.79 | 264.20 | 23.12 | 332.17 | 0.6929 | 705.9 | 555.6 | |
| 0.00 | 1.95 | 0.00 | 1.31 | 33.59 | 263.47 | 22.39 | 331.90 | 0.6759 | 780.0 | 669.0 | |
| 9.34 | 18.94 | 6.41 | 13.02 | 35.23 | 263.67 | 22.58 | 333.05 | 0.6944 | 736.2 | 269.4 | |
| 0.00 | 1.19 | 0.00 | 0.80 | 34.36 | 263.42 | 22.33 | 332.59 | 0.6838 | 747.0 | 580.9 | |
| 0.00 | 2.04 | 0.00 | 1.38 | 34.43 | 263.24 | 22.16 | 332.83 | 0.6836 | 936.0 | 736.7 | |
| 0.00 | 1.61 | 0.00 | 1.11 | 35.45 | 263.38 | 22.29 | 333.50 | 0.6951 | 561.0 | 436.6 | |
| 3.23 | 15.89 | 2.19 | 10.79 | 34.87 | 263.02 | 21.93 | 333.41 | 0.6870 | 930.2 | 683.4 | |
| 4.25 | -12.00 | 2.89 | -12.00 | 35.10 | 262.97 | 21.88 | 333.64 | 0.6891 | 631.6 | 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. | |