SDO HMI 2014-08-22 00:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.83 | 143.48 | 14.02 | 87.56 | 16.47 | 28.10 | 35.18 | 288.73 | 0.5854 | -424.6 | -333.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.83 | 124.95 | 14.02 | 76.75 | 16.32 | 28.70 | 35.79 | 288.23 | 0.5931 | -1046.0 | -378.6 | |
| 0.00 | 4.67 | 0.00 | 2.81 | 17.66 | 26.67 | 33.76 | 291.21 | 0.5702 | -636.0 | -633.1 | |
| 0.00 | 0.90 | 0.00 | 0.54 | 17.65 | 26.36 | 33.45 | 291.32 | 0.5660 | -568.0 | -520.1 | |
| 0.00 | 0.90 | 0.00 | 0.54 | 17.39 | 26.08 | 33.17 | 290.98 | 0.5613 | -603.0 | -507.0 | |
| 0.00 | 2.16 | 0.00 | 1.29 | 17.16 | 25.88 | 32.97 | 290.65 | 0.5578 | -877.0 | -763.1 | |
| 0.00 | 0.90 | 0.00 | 0.54 | 17.38 | 25.77 | 32.86 | 291.09 | 0.5571 | -732.0 | -557.5 | |
| 0.00 | 0.81 | 0.00 | 0.46 | 18.52 | 21.86 | 28.95 | 295.11 | 0.5089 | 438.0 | 368.9 | |
| 0.00 | 1.08 | 0.00 | 0.61 | 17.12 | 21.43 | 28.52 | 292.68 | 0.4966 | 680.0 | 561.5 | |
| 0.00 | 1.53 | 0.00 | 0.87 | 16.87 | 21.36 | 28.44 | 292.25 | 0.4945 | 587.0 | 457.8 | |
| 0.00 | 0.81 | 0.00 | 0.46 | 17.28 | 21.39 | 28.48 | 293.01 | 0.4966 | 669.0 | 569.6 | |
| 0.00 | 1.08 | 0.00 | 0.61 | 18.10 | 21.02 | 28.11 | 294.82 | 0.4955 | 729.0 | 609.0 | |
| 0.00 | 1.53 | 0.00 | 0.87 | 18.33 | 20.85 | 27.94 | 295.37 | 0.4942 | 839.0 | 619.8 | |
| 0.00 | 0.63 | 0.00 | 0.36 | 17.30 | 20.45 | 27.54 | 293.60 | 0.4837 | 748.0 | 556.9 | |
| 0.00 | 0.63 | 0.00 | 0.35 | 16.74 | 19.94 | 27.02 | 292.79 | 0.4739 | 771.0 | 693.3 | |
| 0.00 | 0.90 | 0.00 | 0.50 | 16.81 | 19.73 | 26.82 | 293.06 | 0.4714 | 723.0 | 626.1 | |
| 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. | |