SDO HMI 2014-07-19 23:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.02 | 118.37 | 18.84 | 65.61 | -21.69 | 67.93 | -1.90 | 176.13 | 0.4495 | 168.0 | -45.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.14 | 65.04 | 11.12 | 35.96 | -21.47 | 69.41 | -0.42 | 179.12 | 0.4441 | 1116.6 | 350.4 | |
| 0.54 | -1.00 | 0.30 | -1.00 | -21.03 | 69.22 | -0.61 | 178.69 | 0.4372 | 1099.5 | 999999 | |
| 2.72 | 7.26 | 1.50 | 4.00 | -21.20 | 68.86 | -0.97 | 177.93 | 0.4400 | 952.1 | 641.5 | |
| 0.00 | 1.36 | 0.00 | 0.75 | -21.47 | 68.53 | -1.30 | 177.26 | 0.4445 | 706.0 | 505.0 | |
| 0.00 | 2.00 | 0.00 | 1.10 | -21.30 | 68.01 | -1.82 | 176.14 | 0.4423 | 763.0 | 526.5 | |
| 0.00 | 0.63 | 0.00 | 0.35 | -21.88 | 67.61 | -2.23 | 175.41 | 0.4519 | -560.0 | -490.6 | |
| 0.00 | 0.63 | 0.00 | 0.35 | -22.16 | 67.60 | -2.23 | 175.45 | 0.4561 | -631.0 | -626.1 | |
| 0.00 | 1.18 | 0.00 | 0.66 | -22.43 | 67.40 | -2.43 | 175.09 | 0.4606 | -762.0 | -580.8 | |
| 0.00 | 1.81 | 0.00 | 1.01 | -22.02 | 66.16 | -3.68 | 172.49 | 0.4564 | -661.0 | -383.2 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -21.55 | 66.10 | -3.73 | 172.23 | 0.4492 | -1092.0 | -949.7 | |
| 0.00 | 1.63 | 0.00 | 0.91 | -22.30 | 66.02 | -3.82 | 172.29 | 0.4609 | -900.0 | -750.2 | |
| 0.00 | 7.35 | 0.00 | 4.08 | -21.75 | 65.77 | -4.06 | 171.61 | 0.4531 | -879.0 | -794.9 | |
| 0.73 | 3.36 | 0.40 | 1.87 | -22.16 | 65.72 | -4.11 | 171.66 | 0.4595 | -1019.9 | -803.0 | |
| 9.89 | 24.85 | 5.52 | 13.87 | -22.37 | 65.15 | -4.68 | 170.61 | 0.4641 | -872.7 | -763.2 | |
| 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. | |