SDO HMI 2014-07-06 12:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.97 | 135.45 | 24.88 | 94.47 | 6.50 | 203.22 | -44.74 | 84.24 | 0.7049 | -561.7 | -214.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.27 | 12.17 | 4.27 | 8.28 | 6.87 | 204.62 | -43.34 | 83.63 | 0.6879 | -901.7 | -577.6 | |
| 23.16 | 100.83 | 15.99 | 69.70 | 6.32 | 203.74 | -44.22 | 84.47 | 0.6987 | -1006.5 | -261.8 | |
| 0.73 | 1.91 | 0.51 | 1.34 | 8.49 | 202.99 | -44.97 | 81.42 | 0.7092 | -498.4 | -411.0 | |
| 3.72 | 9.45 | 2.60 | 6.61 | 7.27 | 203.03 | -44.93 | 83.15 | 0.7079 | -639.5 | -409.0 | |
| 1.64 | -4.00 | 1.15 | -4.00 | 7.11 | 202.83 | -45.13 | 83.39 | 0.7103 | -477.7 | 999999 | |
| 0.00 | 0.82 | 0.00 | 0.59 | 3.54 | 200.86 | -47.10 | 88.37 | 0.7337 | -378.0 | -421.2 | |
| 0.00 | 1.82 | 0.00 | 1.36 | 6.01 | 199.31 | -48.65 | 85.02 | 0.7517 | 638.0 | 522.0 | |
| 0.00 | 1.18 | 0.00 | 0.89 | 6.60 | 198.91 | -49.05 | 84.24 | 0.7564 | 551.0 | 454.8 | |
| 0.00 | 0.55 | 0.00 | 0.42 | 6.16 | 197.92 | -50.04 | 84.84 | 0.7674 | -385.0 | -294.3 | |
| 0.00 | 1.09 | 0.00 | 0.85 | 6.57 | 197.43 | -50.53 | 84.32 | 0.7729 | 529.0 | 472.3 | |
| 0.00 | 1.18 | 0.00 | 0.92 | 7.75 | 197.15 | -50.81 | 82.80 | 0.7763 | 478.0 | 483.5 | |
| 0.00 | 0.91 | 0.00 | 0.71 | 7.51 | 197.19 | -50.77 | 83.11 | 0.7758 | 686.0 | 579.0 | |
| 0.00 | 0.91 | 0.00 | 0.72 | 8.22 | 196.78 | -51.19 | 82.21 | 0.7806 | 537.0 | 454.6 | |
| 0.45 | 2.63 | 0.36 | 2.08 | 6.99 | 196.73 | -51.23 | 83.79 | 0.7807 | 533.8 | 386.6 | |
| 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. | |