SDO HMI 2011-01-01 21:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.60 | 165.34 | 31.10 | 113.28 | 34.00 | 267.56 | 24.28 | 330.42 | 0.6926 | -60.4 | -56.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.56 | 90.44 | 11.48 | 62.76 | 33.39 | 270.08 | 26.80 | 327.44 | 0.7018 | -1020.5 | -296.4 | |
| 0.00 | 0.93 | 0.00 | 0.64 | 33.62 | 269.13 | 25.85 | 328.53 | 0.6978 | -416.0 | -350.3 | |
| 5.86 | 7.05 | 4.00 | 4.82 | 33.35 | 268.53 | 25.25 | 328.85 | 0.6912 | -802.3 | -617.4 | |
| 0.34 | 1.44 | 0.23 | 0.99 | 33.57 | 268.44 | 25.16 | 329.13 | 0.6928 | -672.0 | -545.1 | |
| 0.00 | 1.53 | 0.00 | 1.02 | 33.50 | 265.75 | 22.47 | 331.72 | 0.6752 | -712.0 | -610.7 | |
| 0.00 | 1.19 | 0.00 | 0.81 | 35.45 | 264.60 | 21.31 | 334.47 | 0.6893 | 399.0 | 295.4 | |
| 1.27 | 34.31 | 0.86 | 23.22 | 34.77 | 264.37 | 21.09 | 334.17 | 0.6807 | 691.8 | 300.6 | |
| 0.00 | 0.85 | 0.00 | 0.56 | 33.21 | 263.97 | 20.69 | 333.35 | 0.6612 | 727.0 | 550.7 | |
| 0.00 | 1.53 | 0.00 | 1.04 | 35.22 | 264.46 | 21.17 | 334.43 | 0.6861 | 377.0 | 316.3 | |
| 1.44 | -7.00 | 0.98 | -7.00 | 34.99 | 264.35 | 21.07 | 334.36 | 0.6830 | 620.2 | 999999 | |
| 0.00 | 1.44 | 0.00 | 0.95 | 33.61 | 263.69 | 20.41 | 333.97 | 0.6640 | 855.0 | 685.4 | |
| 9.77 | -7.00 | 6.61 | -7.00 | 35.24 | 263.92 | 20.64 | 335.00 | 0.6834 | 732.4 | 999999 | |
| 6.03 | 24.63 | 4.03 | 16.47 | 34.67 | 263.39 | 20.10 | 335.12 | 0.6742 | 1061.5 | 664.8 | |
| 4.33 | -13.00 | 2.91 | -13.00 | 35.04 | 263.25 | 19.97 | 335.54 | 0.6776 | 651.8 | 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. | |