SDO HMI 2014-08-22 01:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.84 | 150.89 | 14.11 | 92.60 | 16.51 | 27.99 | 35.63 | 288.68 | 0.5915 | -482.2 | -319.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.39 | 127.31 | 13.84 | 78.74 | 16.31 | 28.70 | 36.34 | 288.05 | 0.6004 | -1032.1 | -368.1 | |
| 0.00 | 1.08 | 0.00 | 0.65 | 17.12 | 26.81 | 34.45 | 290.03 | 0.5776 | -586.0 | -468.8 | |
| 0.00 | 2.70 | 0.00 | 1.63 | 17.79 | 26.69 | 34.33 | 291.19 | 0.5781 | -599.0 | -554.7 | |
| 0.45 | 1.71 | 0.27 | 1.03 | 17.60 | 26.61 | 34.25 | 290.92 | 0.5764 | -777.6 | -657.9 | |
| 0.00 | 1.35 | 0.00 | 0.81 | 17.68 | 26.36 | 33.99 | 291.15 | 0.5733 | -724.0 | -583.1 | |
| 0.00 | 3.15 | 0.00 | 1.89 | 17.12 | 25.89 | 33.53 | 290.37 | 0.5653 | -853.0 | -689.6 | |
| 0.00 | 3.15 | 0.00 | 1.89 | 17.44 | 25.81 | 33.44 | 290.95 | 0.5652 | -714.0 | -560.0 | |
| 0.00 | 0.81 | 0.00 | 0.47 | 16.45 | 22.37 | 30.01 | 290.64 | 0.5146 | 535.0 | 445.2 | |
| 0.00 | 1.17 | 0.00 | 0.67 | 17.12 | 21.39 | 29.03 | 292.42 | 0.5037 | 681.0 | 565.2 | |
| 0.00 | 0.99 | 0.00 | 0.57 | 18.27 | 21.41 | 29.05 | 294.57 | 0.5091 | 734.0 | 626.5 | |
| 0.00 | 2.43 | 0.00 | 1.39 | 18.86 | 20.90 | 28.54 | 295.99 | 0.5050 | 565.0 | 529.3 | |
| 0.00 | 2.07 | 0.00 | 1.18 | 18.31 | 20.76 | 28.40 | 295.03 | 0.5004 | 759.0 | 605.3 | |
| 0.00 | 1.26 | 0.00 | 0.71 | 17.30 | 20.44 | 28.08 | 293.28 | 0.4913 | 737.0 | 559.6 | |
| 0.00 | 0.63 | 0.00 | 0.36 | 18.92 | 20.37 | 28.01 | 296.45 | 0.4981 | 384.0 | 463.1 | |
| 0.00 | 1.08 | 0.00 | 0.61 | 16.82 | 19.72 | 27.36 | 292.75 | 0.4789 | 799.0 | 706.8 | |
| 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. | |