SDO HMI 2014-07-08 16:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.88 | 173.14 | 14.79 | 88.87 | 6.56 | 204.45 | -14.83 | 78.30 | 0.2613 | -742.9 | -406.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.54 | 0.00 | 1.30 | 10.49 | 206.10 | -13.18 | 61.72 | 0.2557 | -682.0 | -656.7 | |
| 0.00 | 1.45 | 0.00 | 0.74 | 6.33 | 206.14 | -13.14 | 77.94 | 0.2320 | -923.0 | -806.5 | |
| 0.00 | 2.09 | 0.00 | 1.07 | 10.98 | 205.76 | -13.52 | 60.64 | 0.2645 | -923.0 | -741.5 | |
| 2.91 | 4.81 | 1.48 | 2.46 | 7.12 | 205.55 | -13.72 | 75.22 | 0.2446 | -1076.8 | -832.2 | |
| 0.00 | 3.45 | 0.00 | 1.78 | 11.52 | 204.74 | -14.54 | 60.58 | 0.2836 | -913.0 | -544.7 | |
| 25.97 | 150.27 | 13.31 | 77.02 | 6.28 | 204.63 | -14.65 | 79.24 | 0.2570 | -1348.2 | -428.5 | |
| 0.00 | 1.73 | 0.00 | 0.89 | 5.55 | 202.61 | -16.67 | 82.89 | 0.2889 | -687.0 | -605.1 | |
| 0.00 | 0.91 | 0.00 | 0.47 | 6.95 | 202.44 | -16.84 | 78.20 | 0.2951 | -742.0 | -553.8 | |
| 0.00 | 1.36 | 0.00 | 0.71 | 6.06 | 202.18 | -17.10 | 81.32 | 0.2971 | 832.0 | 653.7 | |
| 0.00 | 0.54 | 0.00 | 0.29 | 7.56 | 197.86 | -21.42 | 78.69 | 0.3708 | 507.0 | 537.0 | |
| 0.00 | 0.27 | 0.00 | 0.14 | 5.64 | 197.91 | -21.37 | 83.88 | 0.3662 | 644.0 | 669.7 | |
| 0.00 | 1.45 | 0.00 | 0.78 | 8.83 | 197.22 | -22.06 | 75.68 | 0.3846 | 857.0 | 679.7 | |
| 0.00 | 1.45 | 0.00 | 0.78 | 6.23 | 197.19 | -22.09 | 82.45 | 0.3786 | 940.0 | 749.7 | |
| 0.00 | 0.82 | 0.00 | 0.44 | 8.58 | 196.94 | -22.34 | 76.46 | 0.3882 | 727.0 | 514.4 | |
| 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. | |