SDO HMI 2014-07-20 20:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.13 | 231.36 | 30.33 | 129.82 | -21.20 | 68.29 | 10.03 | 200.31 | 0.4699 | 304.8 | 70.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 28.02 | 160.61 | 15.73 | 90.29 | -20.97 | 69.50 | 11.23 | 202.74 | 0.4725 | 1226.8 | 310.9 | |
| 4.44 | -1.00 | 2.50 | -1.00 | -21.35 | 69.52 | 11.26 | 202.47 | 0.4779 | 1029.8 | 999999 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -20.19 | 69.21 | 10.94 | 202.91 | 0.4597 | 812.0 | 608.8 | |
| 2.99 | -1.00 | 1.68 | -1.00 | -21.31 | 69.25 | 10.99 | 202.02 | 0.4758 | 804.3 | 999999 | |
| 1.09 | 5.53 | 0.60 | 3.07 | -19.94 | 68.30 | 10.04 | 201.40 | 0.4508 | 1012.2 | 775.1 | |
| 0.00 | 0.91 | 0.00 | 0.51 | -20.51 | 68.24 | 9.98 | 200.80 | 0.4587 | 463.0 | 284.3 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -19.80 | 67.96 | 9.70 | 200.87 | 0.4469 | 756.0 | 598.7 | |
| 0.00 | 1.72 | 0.00 | 0.97 | -21.58 | 67.51 | 9.25 | 198.60 | 0.4704 | 528.0 | 446.9 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -20.54 | 66.00 | 7.74 | 196.41 | 0.4481 | -933.0 | -780.6 | |
| 0.00 | 2.36 | 0.00 | 1.33 | -22.35 | 65.96 | 7.70 | 195.20 | 0.4747 | -848.0 | -683.8 | |
| 0.63 | 2.09 | 0.35 | 1.16 | -21.49 | 65.82 | 7.56 | 195.44 | 0.4614 | -851.1 | -694.1 | |
| 0.00 | 0.73 | 0.00 | 0.41 | -21.80 | 65.73 | 7.47 | 195.09 | 0.4656 | -714.0 | -625.1 | |
| 1.00 | 54.23 | 0.56 | 30.32 | -21.32 | 65.51 | 7.25 | 194.95 | 0.4576 | -1006.1 | -761.1 | |
| 4.90 | -13.00 | 2.73 | -13.00 | -21.52 | 65.26 | 7.00 | 194.33 | 0.4596 | -1173.1 | 999999 | |
| 4.44 | -13.00 | 2.48 | -13.00 | -21.69 | 65.10 | 6.84 | 193.93 | 0.4615 | -1100.2 | 999999 | |
| 0.82 | -13.00 | 0.46 | -13.00 | -22.37 | 65.00 | 6.74 | 193.36 | 0.4714 | -622.7 | 999999 | |
| 5.80 | -13.00 | 3.24 | -13.00 | -21.99 | 64.78 | 6.52 | 193.15 | 0.4649 | -1034.5 | 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. | |