SDO HMI 2014-05-27 21:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.69 | 42.09 | 9.45 | 24.80 | -10.36 | 83.78 | 31.38 | 252.07 | 0.5396 | 446.2 | 202.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.53 | 17.95 | 8.17 | 10.84 | -9.80 | 86.39 | 33.99 | 254.47 | 0.5740 | 943.8 | 590.4 | |
| 0.00 | 2.25 | 0.00 | 1.34 | -9.72 | 85.20 | 32.80 | 254.16 | 0.5572 | 791.0 | 648.6 | |
| 0.00 | 1.62 | 0.00 | 0.97 | -9.85 | 84.99 | 32.59 | 253.86 | 0.5547 | 474.0 | 404.4 | |
| 0.00 | 1.08 | 0.00 | 0.64 | -10.96 | 84.72 | 32.32 | 251.79 | 0.5547 | 510.0 | 439.1 | |
| 0.00 | 0.81 | 0.00 | 0.48 | -12.07 | 84.68 | 32.28 | 249.83 | 0.5585 | 568.0 | 404.8 | |
| 0.00 | 1.53 | 0.00 | 0.91 | -11.76 | 84.60 | 32.20 | 250.33 | 0.5562 | 573.0 | 467.5 | |
| 2.16 | 4.15 | 1.28 | 2.45 | -10.16 | 84.37 | 31.97 | 253.04 | 0.5470 | 785.4 | 604.5 | |
| 0.00 | 2.07 | 0.00 | 1.22 | -10.07 | 83.96 | 31.56 | 253.03 | 0.5409 | 861.0 | 723.5 | |
| 0.00 | 0.36 | 0.00 | 0.21 | -10.35 | 83.74 | 31.34 | 252.42 | 0.5388 | 629.0 | 562.0 | |
| 0.00 | 1.44 | 0.00 | 0.84 | -10.17 | 83.29 | 30.89 | 252.54 | 0.5317 | 735.0 | 639.6 | |
| 0.00 | 2.25 | 0.00 | 1.28 | -10.94 | 80.17 | 27.77 | 249.45 | 0.4905 | -764.0 | -670.2 | |
| 0.00 | 2.53 | 0.00 | 1.40 | -9.91 | 77.62 | 25.22 | 249.92 | 0.4488 | -927.0 | -678.8 | |
| 0.00 | 1.80 | 0.00 | 1.00 | -15.04 | 75.23 | 22.83 | 237.26 | 0.4472 | -718.0 | -500.7 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -14.45 | 74.55 | 22.15 | 237.70 | 0.4337 | -729.0 | -566.4 | |
| 0.00 | 1.35 | 0.00 | 0.72 | -9.21 | 72.53 | 20.13 | 247.52 | 0.3692 | -702.0 | -403.9 | |
| 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. | |