SDO HMI 2011-01-01 08:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.79 | 73.65 | 11.00 | 50.61 | -13.61 | 207.37 | -43.06 | 106.60 | 0.6943 | -2.7 | 141.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.10 | 24.22 | 3.38 | 16.06 | -13.76 | 209.64 | -40.80 | 107.38 | 0.6674 | 911.4 | 718.2 | |
| 0.00 | 2.04 | 0.00 | 1.37 | -14.22 | 209.01 | -41.43 | 107.87 | 0.6763 | 609.0 | 491.1 | |
| 0.00 | 1.27 | 0.00 | 0.85 | -12.93 | 209.29 | -41.15 | 106.07 | 0.6698 | 589.0 | 485.2 | |
| 0.00 | 0.93 | 0.00 | 0.62 | -13.08 | 209.25 | -41.18 | 106.28 | 0.6705 | 577.0 | 462.7 | |
| 0.51 | 2.72 | 0.34 | 1.82 | -13.80 | 209.06 | -41.37 | 107.28 | 0.6746 | 680.8 | 484.8 | |
| 0.00 | 3.40 | 0.00 | 2.27 | -13.31 | 208.92 | -41.51 | 106.53 | 0.6751 | 557.0 | 470.5 | |
| 0.34 | 1.53 | 0.23 | 1.04 | -14.67 | 208.21 | -42.23 | 108.31 | 0.6872 | 605.8 | 492.5 | |
| 0.00 | 0.59 | 0.00 | 0.40 | -12.10 | 208.44 | -42.00 | 104.63 | 0.6786 | -513.0 | -404.6 | |
| 0.00 | 0.76 | 0.00 | 0.52 | -12.72 | 208.31 | -42.12 | 105.51 | 0.6814 | -499.0 | -399.2 | |
| 1.44 | 2.21 | 0.98 | 1.49 | -13.05 | 208.20 | -42.23 | 105.96 | 0.6834 | 542.2 | 274.2 | |
| 0.00 | 1.61 | 0.00 | 1.09 | -13.47 | 208.11 | -42.32 | 106.54 | 0.6854 | 361.0 | 240.0 | |
| 0.00 | 1.36 | 0.00 | 0.92 | -12.83 | 208.13 | -42.31 | 105.63 | 0.6839 | 562.0 | 418.4 | |
| 0.00 | 1.53 | 0.00 | 1.04 | -12.49 | 207.70 | -42.73 | 105.04 | 0.6884 | 648.0 | 477.1 | |
| 0.00 | 0.85 | 0.00 | 0.58 | -12.15 | 207.36 | -43.08 | 104.47 | 0.6919 | 515.0 | 328.8 | |
| 0.00 | 2.38 | 0.00 | 1.66 | -13.65 | 206.45 | -43.99 | 106.40 | 0.7059 | -475.0 | -417.8 | |
| 0.00 | 1.19 | 0.00 | 0.84 | -13.63 | 205.94 | -44.50 | 106.26 | 0.7119 | -737.0 | -675.7 | |
| 1.27 | 1.53 | 0.90 | 1.08 | -13.61 | 205.47 | -44.96 | 106.13 | 0.7173 | -644.2 | -612.0 | |
| 0.00 | 3.99 | 0.00 | 2.83 | -12.94 | 205.29 | -45.15 | 105.17 | 0.7183 | -729.0 | -684.2 | |
| 0.00 | 1.61 | 0.00 | 1.16 | -14.26 | 204.96 | -45.47 | 106.90 | 0.7245 | -732.0 | -634.5 | |
| 0.00 | 1.87 | 0.00 | 1.34 | -13.98 | 204.90 | -45.53 | 106.52 | 0.7247 | -668.0 | -555.1 | |
| 0.00 | 2.04 | 0.00 | 1.47 | -13.97 | 204.56 | -45.88 | 106.42 | 0.7286 | -757.0 | -589.2 | |
| 0.00 | 1.02 | 0.00 | 0.73 | -12.99 | 204.80 | -45.64 | 105.13 | 0.7240 | -564.0 | -526.1 | |
| 0.00 | 1.36 | 0.00 | 0.98 | -13.46 | 204.56 | -45.88 | 105.73 | 0.7277 | -779.0 | -664.4 | |
| 1.44 | 1.78 | 1.04 | 1.29 | -13.84 | 204.41 | -46.02 | 106.22 | 0.7300 | -722.9 | -634.0 | |
| 1.95 | 9.86 | 1.41 | 7.16 | -13.60 | 204.30 | -46.14 | 105.87 | 0.7309 | -535.8 | -447.2 | |
| 3.74 | -25.00 | 2.72 | -25.00 | -14.07 | 204.00 | -46.43 | 106.44 | 0.7352 | -452.3 | 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. | |