SDO HMI 2014-07-20 19:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 68.57 | 220.92 | 38.34 | 123.75 | -21.25 | 68.30 | 9.48 | 199.26 | 0.4676 | 112.6 | 122.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 14.06 | 155.62 | 7.90 | 87.30 | -21.27 | 69.54 | 10.72 | 201.56 | 0.4737 | 956.3 | 324.1 | |
| 23.76 | -1.00 | 13.31 | -1.00 | -20.93 | 69.42 | 10.60 | 201.62 | 0.4681 | 1241.9 | 999999 | |
| 0.00 | 0.82 | 0.00 | 0.45 | -20.24 | 68.64 | 9.83 | 200.74 | 0.4539 | 608.0 | 424.6 | |
| 2.09 | 3.72 | 1.15 | 2.06 | -19.90 | 68.26 | 9.44 | 200.28 | 0.4468 | 976.9 | 743.9 | |
| 0.00 | 0.54 | 0.00 | 0.30 | -20.44 | 66.32 | 7.50 | 196.01 | 0.4454 | -506.0 | -553.7 | |
| 0.00 | 0.82 | 0.00 | 0.45 | -20.48 | 66.12 | 7.31 | 195.60 | 0.4451 | -827.0 | -677.2 | |
| 0.00 | 1.90 | 0.00 | 1.07 | -22.34 | 66.02 | 7.20 | 194.26 | 0.4726 | -812.0 | -679.4 | |
| 0.63 | 1.63 | 0.35 | 0.91 | -21.49 | 65.88 | 7.06 | 194.48 | 0.4593 | -758.0 | -628.8 | |
| 0.00 | 3.63 | 0.00 | 2.04 | -22.37 | 65.65 | 6.84 | 193.55 | 0.4717 | -636.0 | -578.8 | |
| 5.71 | 50.15 | 3.20 | 28.00 | -22.03 | 65.54 | 6.72 | 193.52 | 0.4661 | -899.0 | -683.1 | |
| 0.00 | 2.09 | 0.00 | 1.17 | -22.30 | 65.39 | 6.57 | 193.08 | 0.4697 | -622.0 | -578.9 | |
| 13.88 | -10.00 | 7.72 | -10.00 | -21.55 | 65.25 | 6.44 | 193.22 | 0.4579 | -1114.7 | 999999 | |
| 2.18 | -10.00 | 1.22 | -10.00 | -22.19 | 64.98 | 6.17 | 192.36 | 0.4667 | -923.6 | 999999 | |
| 6.26 | -10.00 | 3.49 | -10.00 | -21.99 | 64.81 | 5.99 | 192.12 | 0.4630 | -1052.7 | 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. | |