SDO HMI 2011-02-27 23:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 70.22 | 300.16 | 65.06 | 282.83 | 26.55 | 162.49 | -49.12 | 52.61 | 0.8531 | -11.7 | -130.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.46 | 8.53 | 5.22 | 6.88 | 25.26 | 169.67 | -41.94 | 49.97 | 0.7917 | -679.2 | -421.7 | |
| 0.00 | 0.69 | 0.00 | 0.56 | 24.60 | 168.93 | -42.68 | 51.13 | 0.7940 | -578.0 | -396.6 | |
| 0.00 | 1.81 | 0.00 | 1.47 | 24.04 | 168.27 | -43.34 | 52.13 | 0.7963 | -653.0 | -494.0 | |
| 0.00 | 0.95 | 0.00 | 0.79 | 24.40 | 167.30 | -44.31 | 52.30 | 0.8063 | -484.0 | -389.9 | |
| 0.00 | 0.60 | 0.00 | 0.53 | 26.52 | 165.48 | -46.13 | 51.09 | 0.8313 | 175.0 | 187.9 | |
| 0.00 | 1.29 | 0.00 | 1.08 | 22.99 | 166.41 | -45.21 | 54.33 | 0.8064 | 504.0 | 518.7 | |
| 0.00 | 0.60 | 0.00 | 0.56 | 26.92 | 163.89 | -47.72 | 51.51 | 0.8449 | -736.0 | -615.0 | |
| 0.69 | 92.62 | 0.67 | 89.73 | 28.37 | 162.58 | -49.04 | 50.70 | 0.8606 | -736.9 | -269.9 | |
| 0.00 | 0.78 | 0.00 | 0.73 | 27.21 | 163.12 | -48.49 | 51.61 | 0.8517 | -590.0 | -525.1 | |
| 10.77 | -8.00 | 10.44 | -8.00 | 28.12 | 162.22 | -49.40 | 51.14 | 0.8621 | -755.4 | 999999 | |
| 11.11 | 41.27 | 10.30 | 38.23 | 26.17 | 163.07 | -48.55 | 52.72 | 0.8475 | 679.5 | 492.0 | |
| 0.00 | 0.95 | 0.00 | 0.83 | 23.64 | 164.23 | -47.38 | 54.79 | 0.8272 | 848.0 | 817.5 | |
| 1.81 | -11.00 | 1.69 | -11.00 | 26.07 | 162.67 | -48.94 | 53.02 | 0.8500 | 576.9 | 999999 | |
| 1.46 | 83.91 | 1.38 | 80.72 | 26.33 | 162.47 | -49.15 | 52.85 | 0.8526 | 234.1 | -384.9 | |
| 1.90 | 11.89 | 1.87 | 11.77 | 27.89 | 161.31 | -50.30 | 51.81 | 0.8673 | -121.5 | -5.2 | |
| 2.67 | -11.00 | 2.50 | -11.00 | 25.78 | 162.37 | -49.24 | 53.47 | 0.8509 | 617.4 | 999999 | |
| 4.14 | 53.67 | 3.66 | 48.38 | 23.43 | 163.61 | -48.01 | 55.34 | 0.8313 | 720.8 | 242.0 | |
| 8.79 | -14.00 | 8.55 | -14.00 | 27.13 | 161.47 | -50.14 | 52.51 | 0.8630 | -697.4 | 999999 | |
| 9.91 | -17.00 | 8.89 | -17.00 | 23.77 | 163.24 | -48.37 | 55.16 | 0.8356 | 560.4 | 999999 | |
| 1.12 | -17.00 | 1.00 | -17.00 | 23.43 | 163.21 | -48.40 | 55.53 | 0.8344 | 515.2 | 999999 | |
| 0.86 | -14.00 | 0.82 | -14.00 | 25.94 | 161.88 | -49.74 | 53.55 | 0.8552 | 315.0 | 999999 | |
| 1.98 | -14.00 | 1.92 | -14.00 | 26.46 | 161.20 | -50.41 | 53.33 | 0.8622 | -576.8 | 999999 | |
| 2.41 | -14.00 | 2.34 | -14.00 | 26.32 | 161.18 | -50.43 | 53.48 | 0.8618 | 292.2 | 999999 | |
| 2.07 | -17.00 | 1.89 | -17.00 | 23.76 | 162.36 | -49.26 | 55.61 | 0.8425 | -380.6 | 999999 | |
| 2.07 | -17.00 | 1.92 | -17.00 | 24.19 | 161.78 | -49.84 | 55.43 | 0.8487 | 612.0 | 999999 | |
| 0.00 | 0.60 | 0.00 | 0.57 | 24.32 | 161.20 | -50.42 | 55.57 | 0.8536 | 495.0 | 471.1 | |
| 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. | |