SDO HMI 2014-10-05 23:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 52.78 | 284.59 | 32.58 | 176.02 | -1.49 | 155.23 | 35.93 | 258.70 | 0.6004 | 820.3 | 349.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 37.77 | 255.51 | 23.43 | 158.52 | -1.52 | 155.52 | 36.22 | 258.76 | 0.6045 | 1108.6 | 357.8 | |
| 3.07 | -1.00 | 1.89 | -1.00 | -1.56 | 154.78 | 35.48 | 258.41 | 0.5945 | 1126.3 | 999999 | |
| 8.34 | 12.56 | 5.09 | 7.66 | -1.78 | 154.09 | 34.78 | 257.77 | 0.5857 | 916.5 | 716.6 | |
| 0.00 | 1.23 | 0.00 | 0.75 | -3.84 | 154.01 | 34.71 | 254.34 | 0.5922 | 679.0 | 543.9 | |
| 3.60 | 6.24 | 2.17 | 3.76 | -0.41 | 153.52 | 34.22 | 259.86 | 0.5735 | 874.3 | 664.9 | |
| 0.00 | 0.97 | 0.00 | 0.58 | -0.50 | 152.51 | 33.21 | 259.33 | 0.5595 | 746.0 | 569.3 | |
| 0.00 | 0.97 | 0.00 | 0.57 | -0.20 | 152.01 | 32.71 | 259.67 | 0.5514 | 580.0 | 566.6 | |
| 0.00 | 1.41 | 0.00 | 0.83 | -0.00 | 151.80 | 32.49 | 259.94 | 0.5477 | 754.0 | 575.9 | |
| 0.00 | 0.79 | 0.00 | 0.47 | -0.89 | 151.55 | 32.25 | 258.24 | 0.5471 | -592.0 | -496.1 | |
| 0.00 | 0.70 | 0.00 | 0.41 | -1.14 | 151.09 | 31.79 | 257.61 | 0.5414 | -624.0 | -569.2 | |
| 0.00 | 2.28 | 0.00 | 1.34 | -0.62 | 151.05 | 31.75 | 258.52 | 0.5390 | -783.0 | -675.4 | |
| 0.00 | 1.05 | 0.00 | 0.62 | -0.41 | 150.59 | 31.29 | 258.71 | 0.5317 | -654.0 | -545.8 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -0.27 | 150.28 | 30.98 | 258.84 | 0.5267 | -664.0 | -494.6 | |
| 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. | |