SDO HMI 2014-08-20 02:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 24.75 | 101.06 | 18.78 | 76.11 | -9.39 | 332.02 | -46.22 | 108.88 | 0.7550 | 702.5 | 348.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.53 | 0.00 | 1.04 | -9.14 | 337.71 | -40.53 | 111.09 | 0.6900 | 850.0 | 657.3 | |
| 0.00 | 1.08 | 0.00 | 0.74 | -8.46 | 337.60 | -40.64 | 110.10 | 0.6884 | 626.0 | 537.8 | |
| 0.00 | 0.72 | 0.00 | 0.51 | -9.22 | 335.89 | -42.36 | 110.33 | 0.7115 | 634.0 | 487.8 | |
| 0.00 | 0.63 | 0.00 | 0.44 | -6.50 | 334.82 | -43.42 | 106.22 | 0.7136 | 644.0 | 541.9 | |
| 0.00 | 1.44 | 0.00 | 1.00 | -2.69 | 334.95 | -43.29 | 101.03 | 0.7002 | 121.0 | 130.6 | |
| 0.00 | 1.26 | 0.00 | 0.97 | -12.28 | 332.02 | -46.23 | 112.48 | 0.7658 | -538.0 | -462.0 | |
| 16.02 | 77.93 | 12.05 | 58.65 | -9.45 | 332.10 | -46.14 | 108.99 | 0.7545 | 962.7 | 346.8 | |
| 1.89 | -7.00 | 1.43 | -7.00 | -9.33 | 331.76 | -46.48 | 108.70 | 0.7577 | 581.2 | 999999 | |
| 0.00 | 0.90 | 0.00 | 0.70 | -11.84 | 331.21 | -47.03 | 111.60 | 0.7725 | 477.0 | 309.0 | |
| 0.00 | 0.90 | 0.00 | 0.70 | -11.76 | 331.04 | -47.20 | 111.43 | 0.7739 | 411.0 | 354.7 | |
| 0.00 | 1.53 | 0.00 | 1.17 | -9.37 | 331.26 | -46.98 | 108.55 | 0.7632 | 504.0 | 457.6 | |
| 0.00 | 0.99 | 0.00 | 0.76 | -9.30 | 331.00 | -47.24 | 108.37 | 0.7657 | 606.0 | 468.0 | |
| 5.94 | 9.09 | 4.60 | 7.04 | -9.34 | 330.49 | -47.75 | 108.23 | 0.7713 | 668.0 | 432.9 | |
| 0.90 | 3.06 | 0.70 | 2.39 | -9.45 | 330.01 | -48.23 | 108.18 | 0.7767 | 541.6 | 380.8 | |
| 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. | |