SDO HMI 2014-08-08 00:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.26 | 18.13 | 1.20 | 14.55 | -7.82 | 227.68 | 49.71 | 254.65 | 0.7837 | 245.4 | 266.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.26 | 2.98 | 1.20 | 2.82 | -7.81 | 234.85 | 56.87 | 256.84 | 0.8541 | 611.9 | 479.9 | |
| 0.00 | 0.90 | 0.00 | 0.85 | -7.94 | 234.54 | 56.56 | 256.62 | 0.8516 | 617.0 | 557.4 | |
| 0.00 | 1.08 | 0.00 | 0.91 | -8.26 | 229.89 | 51.92 | 254.96 | 0.8088 | 544.0 | 470.7 | |
| 0.00 | 0.90 | 0.00 | 0.73 | -5.27 | 229.05 | 51.08 | 258.38 | 0.7931 | 608.0 | 493.5 | |
| 0.00 | 1.08 | 0.00 | 0.87 | -5.24 | 228.70 | 50.73 | 258.33 | 0.7895 | 536.0 | 431.2 | |
| 0.00 | 1.08 | 0.00 | 0.86 | -5.96 | 227.78 | 49.81 | 257.17 | 0.7815 | 618.0 | 519.1 | |
| 0.00 | 1.26 | 0.00 | 1.01 | -8.24 | 227.88 | 49.91 | 254.37 | 0.7884 | 374.0 | 325.7 | |
| 0.00 | 1.45 | 0.00 | 1.15 | -8.00 | 227.65 | 49.67 | 254.59 | 0.7854 | 525.0 | 482.4 | |
| 0.00 | 1.99 | 0.00 | 1.53 | -7.45 | 226.24 | 48.27 | 254.83 | 0.7690 | 630.0 | 429.5 | |
| 0.00 | 1.17 | 0.00 | 0.91 | -7.63 | 226.23 | 48.25 | 254.59 | 0.7693 | 335.0 | 401.3 | |
| 0.00 | 0.99 | 0.00 | 0.68 | -4.51 | 220.09 | 42.12 | 256.66 | 0.6895 | -593.0 | -491.5 | |
| 0.00 | 0.45 | 0.00 | 0.30 | -4.00 | 218.67 | 40.70 | 256.88 | 0.6703 | -432.0 | -479.2 | |
| 0.00 | 0.99 | 0.00 | 0.65 | -2.94 | 218.06 | 40.09 | 258.22 | 0.6592 | -738.0 | -649.4 | |
| 0.00 | 1.81 | 0.00 | 1.28 | -17.13 | 217.89 | 39.92 | 238.72 | 0.7198 | -274.0 | -242.1 | |
| 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. | |