SDO HMI 2014-07-20 02:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.18 | 136.66 | 23.90 | 75.65 | -21.58 | 67.93 | -0.25 | 179.54 | 0.4471 | 291.0 | 28.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.87 | 82.30 | 10.98 | 45.47 | -21.42 | 69.43 | 1.25 | 182.63 | 0.4440 | 1104.8 | 390.3 | |
| 0.82 | -1.00 | 0.45 | -1.00 | -21.02 | 69.26 | 1.08 | 182.32 | 0.4375 | 1052.8 | 999999 | |
| 0.00 | 1.63 | 0.00 | 0.90 | -20.81 | 69.23 | 1.05 | 182.27 | 0.4343 | 687.0 | 567.8 | |
| 5.08 | -1.00 | 2.80 | -1.00 | -21.15 | 68.97 | 0.79 | 181.68 | 0.4395 | 927.2 | 999999 | |
| 0.36 | 2.90 | 0.20 | 1.60 | -21.08 | 68.44 | 0.27 | 180.57 | 0.4382 | 865.2 | 683.4 | |
| 1.45 | 3.09 | 0.80 | 1.70 | -20.98 | 67.99 | -0.19 | 179.59 | 0.4366 | 751.1 | 599.0 | |
| 1.45 | 10.53 | 0.80 | 5.82 | -21.39 | 66.02 | -2.16 | 175.46 | 0.4444 | -903.2 | -734.8 | |
| 3.99 | -7.00 | 2.21 | -7.00 | -21.63 | 65.92 | -2.26 | 175.29 | 0.4482 | -1006.5 | 999999 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -22.04 | 65.81 | -2.36 | 175.16 | 0.4547 | -704.0 | -506.1 | |
| 1.72 | 30.49 | 0.96 | 16.98 | -22.17 | 65.58 | -2.60 | 174.71 | 0.4572 | -1048.6 | -789.7 | |
| 0.82 | 2.18 | 0.45 | 1.21 | -21.76 | 65.59 | -2.59 | 174.64 | 0.4508 | -953.8 | -687.9 | |
| 0.00 | 2.45 | 0.00 | 1.37 | -22.65 | 65.37 | -2.80 | 174.40 | 0.4649 | -254.0 | -413.3 | |
| 1.54 | -10.00 | 0.86 | -10.00 | -22.48 | 65.24 | -2.93 | 174.11 | 0.4625 | -772.5 | 999999 | |
| 6.08 | -10.00 | 3.39 | -10.00 | -22.24 | 65.05 | -3.13 | 173.66 | 0.4591 | -860.9 | 999999 | |
| 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. | |