SDO HMI 2014-01-11 01:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.35 | 91.40 | 17.13 | 57.24 | 16.43 | 25.29 | -31.94 | 56.09 | 0.6133 | 84.5 | 53.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.06 | 7.39 | 1.83 | 4.43 | 16.03 | 29.12 | -28.11 | 53.39 | 0.5663 | -919.8 | -742.5 | |
| 0.00 | 1.36 | 0.00 | 0.82 | 15.40 | 28.24 | -28.99 | 55.12 | 0.5718 | -709.0 | -640.1 | |
| 0.00 | 1.78 | 0.00 | 1.08 | 15.32 | 27.97 | -29.26 | 55.49 | 0.5743 | -731.0 | -616.2 | |
| 1.36 | 4.33 | 0.82 | 2.63 | 15.57 | 27.83 | -29.40 | 55.24 | 0.5779 | -889.1 | -663.9 | |
| 0.00 | 1.19 | 0.00 | 0.72 | 15.92 | 27.77 | -29.46 | 54.77 | 0.5812 | -542.0 | -466.5 | |
| 0.00 | 1.02 | 0.00 | 0.62 | 15.61 | 27.57 | -29.66 | 55.40 | 0.5812 | -616.0 | -537.6 | |
| 0.00 | 0.76 | 0.00 | 0.47 | 15.93 | 27.49 | -29.74 | 55.01 | 0.5846 | -438.0 | -364.7 | |
| 0.76 | 20.22 | 0.47 | 12.54 | 15.26 | 25.49 | -31.74 | 57.63 | 0.6031 | -888.1 | -332.0 | |
| 5.44 | -8.00 | 3.38 | -8.00 | 15.51 | 25.42 | -31.81 | 57.33 | 0.6057 | -876.7 | 999999 | |
| 0.00 | 2.29 | 0.00 | 1.45 | 17.29 | 24.94 | -32.29 | 55.19 | 0.6235 | 815.0 | 705.8 | |
| 14.02 | 40.28 | 8.91 | 25.62 | 17.16 | 24.34 | -32.89 | 55.84 | 0.6293 | 937.7 | 418.0 | |
| 0.00 | 1.44 | 0.00 | 0.91 | 16.52 | 24.47 | -32.76 | 56.63 | 0.6236 | 873.0 | 749.4 | |
| 2.12 | 3.57 | 1.33 | 2.24 | 15.21 | 24.38 | -32.85 | 58.55 | 0.6159 | -785.2 | -558.4 | |
| 0.00 | 1.61 | 0.00 | 1.03 | 16.42 | 23.97 | -33.26 | 57.15 | 0.6285 | 703.0 | 604.5 | |
| 0.00 | 0.85 | 0.00 | 0.54 | 16.72 | 23.43 | -33.80 | 57.12 | 0.6367 | 716.0 | 617.0 | |
| 0.00 | 1.10 | 0.00 | 0.71 | 17.33 | 23.16 | -34.07 | 56.49 | 0.6437 | 730.0 | 559.3 | |
| 0.59 | 2.21 | 0.39 | 1.43 | 17.28 | 22.91 | -34.32 | 56.74 | 0.6462 | 742.7 | 609.7 | |
| 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. | |