SDO HMI 2014-10-01 10:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.47 | 116.93 | 12.89 | 78.06 | -10.08 | 140.52 | -38.72 | 113.14 | 0.6720 | 454.8 | 235.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.88 | 0.00 | 0.61 | -16.76 | 141.76 | -37.48 | 122.77 | 0.6952 | 460.0 | 391.9 | |
| 18.50 | 103.53 | 12.25 | 68.56 | -9.67 | 140.88 | -38.36 | 112.78 | 0.6659 | 962.3 | 321.2 | |
| 0.97 | -2.00 | 0.64 | -2.00 | -9.23 | 140.86 | -38.38 | 112.16 | 0.6640 | 709.6 | 999999 | |
| 0.00 | 0.62 | 0.00 | 0.42 | -11.23 | 140.06 | -39.19 | 114.48 | 0.6833 | 652.0 | 546.3 | |
| 0.00 | 0.26 | 0.00 | 0.18 | -14.45 | 139.40 | -39.84 | 118.34 | 0.7072 | 560.0 | 511.0 | |
| 0.00 | 1.85 | 0.00 | 1.25 | -11.05 | 139.97 | -39.28 | 114.18 | 0.6834 | 450.0 | 327.2 | |
| 0.00 | 2.56 | 0.00 | 1.82 | -14.77 | 138.27 | -40.98 | 118.08 | 0.7210 | -727.0 | -611.5 | |
| 0.00 | 2.03 | 0.00 | 1.43 | -13.49 | 138.31 | -40.94 | 116.47 | 0.7141 | -553.0 | -551.7 | |
| 0.00 | 1.32 | 0.00 | 0.95 | -12.78 | 136.80 | -42.45 | 114.77 | 0.7272 | -674.0 | -578.9 | |
| 0.00 | 0.97 | 0.00 | 0.70 | -12.96 | 136.59 | -42.65 | 114.88 | 0.7302 | -389.0 | -311.0 | |
| 0.00 | 1.15 | 0.00 | 0.83 | -12.46 | 136.49 | -42.76 | 114.20 | 0.7291 | -302.0 | -408.1 | |
| 0.00 | 0.88 | 0.00 | 0.64 | -12.58 | 136.12 | -43.12 | 114.18 | 0.7336 | -538.0 | -459.0 | |
| 0.00 | 0.88 | 0.00 | 0.67 | -12.48 | 133.55 | -45.69 | 112.84 | 0.7604 | -316.0 | -296.4 | |
| 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. | |