SDO HMI 2014-08-12 12:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 75.44 | 429.91 | 39.10 | 222.47 | 14.63 | 133.33 | 14.83 | 300.65 | 0.2882 | -895.1 | -354.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.73 | 397.97 | 37.75 | 206.45 | 14.87 | 133.93 | 15.43 | 300.19 | 0.2988 | -1399.8 | -432.2 | |
| 0.00 | 1.99 | 0.00 | 1.02 | 14.69 | 132.49 | 13.99 | 301.97 | 0.2768 | -991.0 | -772.9 | |
| 0.00 | 1.17 | 0.00 | 0.60 | 14.14 | 131.39 | 12.89 | 302.13 | 0.2565 | -947.0 | -748.5 | |
| 0.00 | 1.53 | 0.00 | 0.79 | 17.67 | 129.54 | 11.04 | 317.02 | 0.2688 | -799.0 | -663.8 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 12.37 | 126.58 | 8.08 | 307.05 | 0.1727 | 734.0 | 620.7 | |
| 0.00 | 1.35 | 0.00 | 0.68 | 11.34 | 126.26 | 7.76 | 302.87 | 0.1584 | 808.0 | 570.5 | |
| 0.00 | 2.26 | 0.00 | 1.13 | 11.20 | 125.76 | 7.26 | 303.79 | 0.1498 | 804.0 | 620.8 | |
| 0.00 | 2.35 | 0.00 | 1.17 | 10.92 | 125.66 | 7.16 | 302.57 | 0.1459 | 1021.0 | 806.3 | |
| 0.00 | 1.62 | 0.00 | 0.81 | 11.75 | 125.68 | 7.18 | 307.08 | 0.1541 | 1013.0 | 750.8 | |
| 0.00 | 2.35 | 0.00 | 1.17 | 10.72 | 125.19 | 6.69 | 303.06 | 0.1371 | 1168.0 | 922.5 | |
| 0.00 | 4.06 | 0.00 | 2.03 | 10.94 | 124.48 | 5.98 | 307.42 | 0.1293 | 1078.0 | 893.1 | |
| 2.71 | 9.48 | 1.35 | 4.73 | 10.18 | 124.18 | 5.68 | 303.69 | 0.1176 | 1165.7 | 876.2 | |
| 0.00 | 1.44 | 0.00 | 0.72 | 10.50 | 122.67 | 4.17 | 314.52 | 0.1007 | 909.0 | 718.7 | |
| 0.00 | 0.99 | 0.00 | 0.49 | 11.28 | 119.92 | 1.42 | 343.79 | 0.0874 | 729.0 | 537.4 | |
| 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. | |