SDO HMI 2014-10-02 13:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.40 | 81.94 | 8.72 | 46.65 | -10.29 | 140.23 | -24.17 | 124.87 | 0.4934 | 523.2 | 405.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.58 | 0.00 | 0.91 | -12.13 | 140.42 | -23.99 | 128.14 | 0.5073 | 789.0 | 632.1 | |
| 2.20 | 55.10 | 1.25 | 31.23 | -9.80 | 140.52 | -23.88 | 124.41 | 0.4855 | 1108.7 | 450.2 | |
| 2.99 | -2.00 | 1.69 | -2.00 | -9.55 | 140.54 | -23.86 | 124.00 | 0.4831 | 1107.3 | 999999 | |
| 5.72 | 13.47 | 3.23 | 7.59 | -9.17 | 140.54 | -23.87 | 123.34 | 0.4801 | 973.6 | 668.4 | |
| 0.00 | 1.94 | 0.00 | 1.11 | -11.95 | 140.27 | -24.14 | 127.67 | 0.5074 | 724.0 | 542.2 | |
| 4.49 | -2.00 | 2.55 | -2.00 | -10.02 | 140.40 | -24.00 | 124.66 | 0.4889 | 852.3 | 999999 | |
| 0.00 | 1.41 | 0.00 | 0.84 | -16.76 | 139.66 | -24.74 | 134.00 | 0.5592 | 523.0 | 474.0 | |
| 0.00 | 1.23 | 0.00 | 0.73 | -16.53 | 139.56 | -24.85 | 133.58 | 0.5582 | 642.0 | 539.6 | |
| 0.00 | 1.14 | 0.00 | 0.66 | -11.58 | 139.93 | -24.47 | 126.71 | 0.5082 | 781.0 | 640.5 | |
| 0.00 | 0.97 | 0.00 | 0.56 | -11.75 | 139.78 | -24.62 | 126.80 | 0.5115 | 648.0 | 573.9 | |
| 0.00 | 1.41 | 0.00 | 0.84 | -13.92 | 137.76 | -26.64 | 127.94 | 0.5540 | -724.0 | -603.2 | |
| 0.00 | 1.67 | 0.00 | 0.98 | -12.79 | 137.90 | -26.51 | 126.40 | 0.5428 | -825.0 | -678.7 | |
| 0.00 | 0.79 | 0.00 | 0.47 | -12.28 | 136.92 | -27.48 | 124.64 | 0.5502 | -591.0 | -442.1 | |
| 0.00 | 1.23 | 0.00 | 0.73 | -12.48 | 136.69 | -27.71 | 124.72 | 0.5546 | -749.0 | -644.8 | |
| 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. | |