SDO HMI 2014-01-14 10:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 90.39 | 462.77 | 45.77 | 234.36 | -16.46 | 12.87 | 0.05 | 180.24 | 0.2093 | 1117.1 | 411.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.19 | 277.55 | 0.60 | 140.61 | -16.97 | 13.82 | 1.01 | 184.46 | 0.2180 | 1010.4 | 471.6 | |
| 46.09 | -1.00 | 23.35 | -1.00 | -16.61 | 13.67 | 0.86 | 183.89 | 0.2116 | 1456.3 | 999999 | |
| 7.14 | -1.00 | 3.62 | -1.00 | -16.64 | 13.05 | 0.24 | 181.09 | 0.2116 | 1193.7 | 999999 | |
| 0.00 | 1.28 | 0.00 | 0.65 | -18.85 | 12.84 | 0.02 | 180.08 | 0.2493 | 709.0 | 578.9 | |
| 0.00 | 1.62 | 0.00 | 0.82 | -16.76 | 12.62 | -0.19 | 179.14 | 0.2137 | 880.0 | 640.5 | |
| 0.00 | 1.19 | 0.00 | 0.60 | -15.83 | 12.53 | -0.28 | 178.63 | 0.1977 | 578.0 | 572.5 | |
| 0.00 | 1.45 | 0.00 | 0.73 | -16.88 | 12.50 | -0.31 | 178.60 | 0.2158 | 714.0 | 542.6 | |
| 0.00 | 3.06 | 0.00 | 1.54 | -15.47 | 12.47 | -0.34 | 178.27 | 0.1915 | 892.0 | 675.8 | |
| 0.00 | 1.36 | 0.00 | 0.69 | -15.38 | 12.29 | -0.52 | 177.33 | 0.1901 | 640.0 | 440.0 | |
| 0.00 | 2.55 | 0.00 | 1.28 | -14.92 | 12.11 | -0.71 | 176.24 | 0.1825 | -861.0 | -433.0 | |
| 35.97 | 166.84 | 18.20 | 84.44 | -16.19 | 11.95 | -0.87 | 175.91 | 0.2044 | 1342.9 | 359.1 | |
| 0.00 | 1.19 | 0.00 | 0.60 | -15.71 | 7.50 | -5.31 | 155.45 | 0.2155 | -867.0 | -701.3 | |
| 0.00 | 1.70 | 0.00 | 0.86 | -15.83 | 6.98 | -5.84 | 153.60 | 0.2211 | -811.0 | -736.0 | |
| 0.00 | 1.70 | 0.00 | 0.88 | -19.10 | 4.35 | -8.46 | 151.22 | 0.2902 | -862.0 | -560.2 | |
| 0.00 | 1.28 | 0.00 | 0.66 | -17.58 | 4.15 | -8.67 | 147.72 | 0.2703 | -967.0 | -693.0 | |
| 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. | |