SDO HMI 2014-07-06 00:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 27.61 | 135.77 | 21.59 | 107.16 | 6.38 | 203.41 | -51.14 | 84.54 | 0.7794 | -643.6 | -218.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.91 | 12.44 | 1.47 | 9.56 | 6.64 | 204.55 | -50.00 | 84.17 | 0.7671 | -977.0 | -646.1 | |
| 1.45 | -1.00 | 1.12 | -1.00 | 6.79 | 204.48 | -50.07 | 83.97 | 0.7679 | -800.2 | 999999 | |
| 0.00 | 1.00 | 0.00 | 0.77 | 6.75 | 204.25 | -50.30 | 84.03 | 0.7705 | -520.0 | -473.3 | |
| 22.16 | 100.98 | 17.34 | 79.18 | 6.21 | 203.74 | -50.81 | 84.75 | 0.7760 | -978.9 | -231.3 | |
| 0.00 | 1.09 | 0.00 | 0.86 | 8.17 | 203.09 | -51.46 | 82.25 | 0.7836 | -505.0 | -438.8 | |
| 0.00 | 0.64 | 0.00 | 0.51 | 8.29 | 203.07 | -51.48 | 82.09 | 0.7839 | -355.0 | -288.0 | |
| 0.00 | 0.82 | 0.00 | 0.65 | 7.29 | 203.19 | -51.36 | 83.37 | 0.7822 | -493.0 | -429.4 | |
| 2.09 | 10.35 | 1.66 | 8.23 | 6.97 | 203.04 | -51.51 | 83.78 | 0.7838 | -570.3 | -174.8 | |
| 0.00 | 1.00 | 0.00 | 0.80 | 6.01 | 202.68 | -51.87 | 85.02 | 0.7875 | 260.0 | 214.0 | |
| 0.00 | 0.64 | 0.00 | 0.53 | 3.77 | 200.68 | -53.86 | 87.80 | 0.8087 | -544.0 | -455.1 | |
| 0.00 | 1.54 | 0.00 | 1.36 | 6.83 | 198.68 | -55.87 | 84.04 | 0.8285 | 634.0 | 545.3 | |
| 0.00 | 1.82 | 0.00 | 1.60 | 7.10 | 198.52 | -56.03 | 83.72 | 0.8301 | 526.0 | 446.4 | |
| 0.00 | 0.91 | 0.00 | 0.80 | 6.25 | 198.61 | -55.94 | 84.75 | 0.8291 | 594.0 | 501.5 | |
| 0.00 | 2.54 | 0.00 | 2.31 | 7.23 | 197.43 | -57.12 | 83.57 | 0.8405 | 325.0 | 281.9 | |
| 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. | |