SDO HMI 2014-08-12 16:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 31.20 | 76.83 | 23.12 | 56.82 | 13.57 | 164.51 | 48.22 | 282.44 | 0.7445 | -244.1 | -159.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.99 | 0.00 | 0.75 | 13.67 | 165.79 | 49.50 | 282.47 | 0.7589 | 270.0 | 194.7 | |
| 18.31 | 34.09 | 13.78 | 25.64 | 13.33 | 165.45 | 49.16 | 282.04 | 0.7550 | -834.2 | -494.5 | |
| 0.00 | 4.51 | 0.00 | 3.39 | 13.86 | 165.36 | 49.07 | 282.76 | 0.7543 | -487.0 | -468.8 | |
| 0.00 | 2.34 | 0.00 | 1.74 | 12.90 | 164.62 | 48.33 | 281.53 | 0.7454 | -325.0 | -331.7 | |
| 3.52 | 8.66 | 2.59 | 6.37 | 12.81 | 164.32 | 48.02 | 281.42 | 0.7419 | -680.5 | -288.7 | |
| 0.36 | 2.71 | 0.26 | 1.98 | 12.62 | 163.94 | 47.65 | 281.19 | 0.7375 | -782.5 | -630.7 | |
| 0.00 | 0.81 | 0.00 | 0.59 | 12.01 | 163.56 | 47.27 | 280.38 | 0.7328 | -649.0 | -498.1 | |
| 0.00 | 1.26 | 0.00 | 0.92 | 14.82 | 163.89 | 47.59 | 284.18 | 0.7386 | 317.0 | 338.5 | |
| 0.00 | 1.89 | 0.00 | 1.38 | 14.92 | 163.45 | 47.16 | 284.37 | 0.7337 | 524.0 | 395.6 | |
| 0.81 | 14.43 | 0.59 | 10.39 | 14.05 | 163.11 | 46.82 | 283.21 | 0.7289 | 632.7 | 534.3 | |
| 7.03 | -10.00 | 5.06 | -10.00 | 14.37 | 162.97 | 46.68 | 283.67 | 0.7276 | 726.5 | 999999 | |
| 0.00 | 0.81 | 0.00 | 0.58 | 13.86 | 162.74 | 46.45 | 282.99 | 0.7245 | 548.0 | 556.1 | |
| 0.00 | 0.72 | 0.00 | 0.52 | 13.98 | 162.77 | 46.48 | 283.16 | 0.7249 | 773.0 | 773.6 | |
| 1.17 | 2.44 | 0.84 | 1.74 | 14.77 | 162.58 | 46.29 | 284.27 | 0.7235 | 733.5 | 616.6 | |
| 0.00 | 1.17 | 0.00 | 0.83 | 14.03 | 161.83 | 45.54 | 283.32 | 0.7139 | 523.0 | 381.5 | |
| 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. | |