SDO HMI 2014-01-16 04:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.23 | 21.55 | 1.52 | 14.44 | 16.09 | 27.00 | 37.25 | 300.39 | 0.6749 | 293.7 | 71.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.43 | 5.10 | 0.30 | 3.63 | 15.89 | 31.37 | 41.62 | 297.41 | 0.7220 | -630.4 | -588.3 | |
| 0.43 | -1.00 | 0.30 | -1.00 | 15.78 | 31.18 | 41.43 | 297.38 | 0.7194 | -688.6 | 999999 | |
| 0.77 | 3.83 | 0.54 | 2.70 | 15.88 | 30.67 | 40.92 | 297.77 | 0.7145 | -796.7 | -557.9 | |
| 0.00 | 0.68 | 0.00 | 0.48 | 16.07 | 30.03 | 40.28 | 298.36 | 0.7084 | -504.0 | -485.0 | |
| 0.00 | 1.45 | 0.00 | 0.93 | 15.78 | 24.42 | 34.67 | 301.50 | 0.6444 | 672.0 | 622.3 | |
| 0.00 | 0.94 | 0.00 | 0.60 | 16.00 | 24.32 | 34.57 | 301.87 | 0.6445 | 525.0 | 473.5 | |
| 0.00 | 0.94 | 0.00 | 0.60 | 15.86 | 24.18 | 34.43 | 301.78 | 0.6421 | 744.0 | 616.5 | |
| 0.00 | 0.77 | 0.00 | 0.50 | 16.67 | 24.01 | 34.26 | 303.01 | 0.6454 | 412.0 | 413.8 | |
| 0.60 | 2.30 | 0.38 | 1.47 | 15.77 | 23.60 | 33.85 | 302.07 | 0.6350 | 771.0 | 647.1 | |
| 0.00 | 1.36 | 0.00 | 0.87 | 16.68 | 23.41 | 33.66 | 303.46 | 0.6388 | 676.0 | 548.3 | |
| 0.00 | 1.36 | 0.00 | 0.87 | 15.73 | 23.23 | 33.48 | 302.28 | 0.6303 | 738.0 | 607.8 | |
| 0.00 | 1.11 | 0.00 | 0.70 | 15.47 | 23.14 | 33.39 | 301.99 | 0.6277 | 688.0 | 523.0 | |
| 0.00 | 0.94 | 0.00 | 0.60 | 17.91 | 21.93 | 32.18 | 306.28 | 0.6310 | 682.0 | 530.9 | |
| 0.00 | 0.77 | 0.00 | 0.49 | 18.61 | 21.82 | 32.07 | 307.30 | 0.6349 | 712.0 | 620.2 | |
| 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. | |