SDO HMI 2014-07-20 06:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.10 | 150.31 | 23.84 | 83.16 | -21.43 | 68.04 | 2.06 | 184.37 | 0.4460 | 254.8 | 104.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.61 | 82.60 | 8.64 | 45.69 | -21.39 | 69.45 | 3.47 | 187.28 | 0.4467 | 1126.1 | 360.9 | |
| 1.36 | -1.00 | 0.75 | -1.00 | -20.94 | 69.35 | 3.36 | 187.19 | 0.4396 | 1130.4 | 999999 | |
| 0.00 | 1.72 | 0.00 | 0.95 | -20.71 | 69.31 | 3.32 | 187.18 | 0.4359 | 1150.0 | 890.4 | |
| 4.90 | -1.00 | 2.70 | -1.00 | -21.15 | 69.02 | 3.04 | 186.45 | 0.4422 | 914.2 | 999999 | |
| 5.81 | 19.61 | 3.19 | 10.78 | -20.74 | 68.59 | 2.61 | 185.64 | 0.4351 | 1086.0 | 704.2 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -20.90 | 68.07 | 2.09 | 184.49 | 0.4370 | 671.0 | 550.3 | |
| 1.63 | 15.61 | 0.90 | 8.63 | -21.44 | 65.89 | -0.10 | 179.79 | 0.4441 | -1066.4 | -773.3 | |
| 5.99 | -7.00 | 3.32 | -7.00 | -21.64 | 65.75 | -0.23 | 179.52 | 0.4473 | -1092.4 | 999999 | |
| 0.00 | 0.73 | 0.00 | 0.40 | -22.47 | 65.52 | -0.46 | 179.07 | 0.4602 | -399.0 | -424.4 | |
| 0.00 | 2.36 | 0.00 | 1.31 | -21.75 | 65.49 | -0.49 | 178.98 | 0.4490 | -1079.0 | -903.4 | |
| 0.00 | 1.36 | 0.00 | 0.76 | -22.60 | 65.45 | -0.53 | 178.94 | 0.4623 | -528.0 | -435.1 | |
| 1.36 | 25.32 | 0.76 | 14.09 | -22.29 | 65.32 | -0.66 | 178.66 | 0.4576 | -972.6 | -752.4 | |
| 2.45 | -12.00 | 1.36 | -12.00 | -22.02 | 65.19 | -0.79 | 178.38 | 0.4534 | -1107.1 | 999999 | |
| 3.99 | -12.00 | 2.22 | -12.00 | -22.23 | 65.06 | -0.92 | 178.12 | 0.4566 | -966.0 | 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. | |