SDO HMI 2014-03-10 02:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.87 | 28.52 | 0.43 | 14.18 | -11.00 | 14.60 | 1.71 | 204.07 | 0.0883 | 235.9 | 343.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.82 | 0.00 | 0.91 | -9.44 | 19.51 | 6.62 | 251.00 | 0.1208 | 930.0 | 682.7 | |
| 0.00 | 2.34 | 0.00 | 1.16 | -9.43 | 17.96 | 5.07 | 246.13 | 0.0958 | 878.0 | 712.1 | |
| 0.00 | 1.13 | 0.00 | 0.56 | -9.17 | 17.60 | 4.70 | 247.28 | 0.0882 | 862.0 | 710.0 | |
| 0.87 | 4.68 | 0.43 | 2.33 | -10.82 | 16.19 | 3.30 | 222.15 | 0.0846 | 1150.9 | 851.6 | |
| 0.00 | 7.54 | 0.00 | 3.74 | -10.82 | 15.19 | 2.30 | 212.24 | 0.0741 | 895.0 | 725.6 | |
| 0.00 | 1.04 | 0.00 | 0.52 | -11.24 | 15.13 | 2.24 | 208.81 | 0.0799 | 810.0 | 674.7 | |
| 0.00 | 1.65 | 0.00 | 0.82 | -11.45 | 15.01 | 2.12 | 206.30 | 0.0822 | 857.0 | 641.5 | |
| 0.00 | 1.13 | 0.00 | 0.56 | -10.65 | 13.01 | 0.12 | 181.91 | 0.0596 | 660.0 | 449.2 | |
| 0.00 | 1.30 | 0.00 | 0.65 | -11.77 | 11.09 | -1.80 | 158.71 | 0.0851 | -967.0 | -774.7 | |
| 0.00 | 1.21 | 0.00 | 0.60 | -12.19 | 10.45 | -2.44 | 154.19 | 0.0962 | -1018.0 | -829.9 | |
| 0.00 | 2.25 | 0.00 | 1.12 | -12.43 | 10.35 | -2.54 | 154.42 | 0.1006 | -839.0 | -714.9 | |
| 0.00 | 1.13 | 0.00 | 0.56 | -12.66 | 10.29 | -2.60 | 154.89 | 0.1049 | -841.0 | -737.9 | |
| 0.00 | 1.30 | 0.00 | 0.65 | -13.07 | 8.85 | -4.04 | 145.97 | 0.1233 | -705.0 | -553.3 | |
| 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. | |