SDO HMI 2014-08-22 12:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 21.49 | 127.78 | 14.43 | 84.98 | 16.52 | 27.88 | 41.56 | 287.17 | 0.6674 | -461.8 | -238.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.41 | 110.59 | 13.71 | 74.37 | 16.38 | 28.71 | 42.39 | 286.72 | 0.6776 | -1028.0 | -320.6 | |
| 1.08 | -1.00 | 0.72 | -1.00 | 16.35 | 28.28 | 41.95 | 286.77 | 0.6722 | -946.3 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.82 | 17.63 | 26.64 | 40.31 | 289.05 | 0.6545 | -747.0 | -614.3 | |
| 0.00 | 1.26 | 0.00 | 0.82 | 17.91 | 26.63 | 40.30 | 289.47 | 0.6551 | -654.0 | -540.5 | |
| 0.00 | 1.26 | 0.00 | 0.82 | 17.01 | 26.14 | 39.81 | 288.24 | 0.6469 | -748.0 | -623.9 | |
| 0.00 | 1.17 | 0.00 | 0.75 | 16.92 | 24.97 | 38.64 | 288.39 | 0.6318 | -727.0 | -633.8 | |
| 0.00 | 1.17 | 0.00 | 0.72 | 17.08 | 21.74 | 35.41 | 289.63 | 0.5903 | 593.0 | 566.2 | |
| 0.00 | 1.71 | 0.00 | 1.04 | 16.76 | 21.05 | 34.72 | 289.32 | 0.5801 | 624.0 | 540.6 | |
| 0.00 | 0.72 | 0.00 | 0.44 | 19.09 | 21.54 | 35.22 | 293.01 | 0.5943 | 530.0 | 420.8 | |
| 0.00 | 1.26 | 0.00 | 0.76 | 18.21 | 20.71 | 34.38 | 291.89 | 0.5803 | 668.0 | 610.4 | |
| 0.00 | 1.89 | 0.00 | 1.14 | 16.94 | 20.28 | 33.95 | 289.89 | 0.5703 | 636.0 | 484.5 | |
| 0.00 | 2.25 | 0.00 | 1.36 | 18.88 | 20.48 | 34.15 | 293.11 | 0.5797 | 830.0 | 613.6 | |
| 0.00 | 1.08 | 0.00 | 0.65 | 17.14 | 19.98 | 33.65 | 290.36 | 0.5669 | 757.0 | 645.6 | |
| 0.00 | 2.16 | 0.00 | 1.29 | 17.28 | 19.74 | 33.41 | 290.69 | 0.5642 | 807.0 | 724.6 | |
| 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. | |