SDO HMI 2014-12-02 16:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 59.77 | 350.07 | 36.13 | 211.35 | 16.66 | 109.83 | 31.44 | 298.98 | 0.5735 | -892.9 | -303.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.54 | 334.71 | 0.93 | 202.40 | 17.19 | 110.20 | 31.81 | 299.55 | 0.5811 | -578.8 | -351.9 | |
| 58.23 | -1.00 | 35.20 | -1.00 | 16.60 | 110.01 | 31.62 | 298.75 | 0.5754 | -1433.4 | 999999 | |
| 0.00 | 0.68 | 0.00 | 0.40 | 16.53 | 108.02 | 29.64 | 300.04 | 0.5498 | 420.0 | 365.6 | |
| 0.00 | 1.37 | 0.00 | 0.81 | 17.95 | 106.85 | 28.47 | 303.30 | 0.5447 | 486.0 | 415.0 | |
| 0.00 | 1.02 | 0.00 | 0.61 | 18.20 | 106.90 | 28.51 | 303.66 | 0.5470 | 619.0 | 511.4 | |
| 0.00 | 1.88 | 0.00 | 1.10 | 17.55 | 106.68 | 28.29 | 302.80 | 0.5397 | 780.0 | 632.8 | |
| 0.00 | 1.02 | 0.00 | 0.60 | 17.64 | 106.55 | 28.17 | 303.05 | 0.5388 | 874.0 | 751.8 | |
| 0.00 | 0.77 | 0.00 | 0.45 | 17.89 | 106.56 | 28.17 | 303.45 | 0.5407 | 804.0 | 711.0 | |
| 0.00 | 2.05 | 0.00 | 1.20 | 17.83 | 106.34 | 27.95 | 303.54 | 0.5375 | 612.0 | 568.6 | |
| 0.00 | 0.85 | 0.00 | 0.49 | 17.69 | 104.71 | 26.32 | 304.77 | 0.5164 | 551.0 | 442.6 | |
| 0.00 | 1.20 | 0.00 | 0.69 | 17.23 | 104.46 | 26.08 | 304.22 | 0.5098 | 758.0 | 591.6 | |
| 0.00 | 2.82 | 0.00 | 1.63 | 17.81 | 104.49 | 26.10 | 305.19 | 0.5146 | 810.0 | 715.6 | |
| 0.00 | 0.68 | 0.00 | 0.39 | 16.27 | 104.22 | 25.83 | 302.80 | 0.4996 | 474.0 | 602.1 | |
| 0.00 | 1.02 | 0.00 | 0.58 | 17.02 | 103.03 | 24.64 | 305.26 | 0.4903 | 833.0 | 678.2 | |
| 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. | |