SDO HMI 2014-10-30 14:00:29 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.50 | 53.88 | 16.10 | 50.39 | -15.89 | 99.67 | -54.85 | 111.95 | 0.8496 | 353.8 | 173.6 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.14 | 23.30 | 9.19 | 21.15 | -15.79 | 100.82 | -53.69 | 112.19 | 0.8396 | 697.6 | 366.1 | |
| 0.00 | 0.69 | 0.00 | 0.64 | -15.58 | 100.22 | -54.30 | 111.75 | 0.8443 | 385.0 | 361.5 | |
| 5.02 | 13.69 | 4.66 | 12.74 | -15.91 | 99.93 | -54.59 | 112.04 | 0.8477 | 624.3 | 412.0 | |
| 0.00 | 1.99 | 0.00 | 1.83 | -15.24 | 100.08 | -54.43 | 111.33 | 0.8446 | 421.0 | 224.2 | |
| 0.78 | -3.00 | 0.73 | -3.00 | -15.77 | 99.66 | -54.86 | 111.80 | 0.8497 | 444.8 | 999999 | |
| 0.00 | 0.43 | 0.00 | 0.41 | -16.34 | 99.09 | -55.42 | 112.27 | 0.8559 | 181.0 | 234.2 | |
| 0.52 | 1.39 | 0.49 | 1.31 | -15.96 | 99.20 | -55.32 | 111.87 | 0.8540 | 176.8 | 180.5 | |
| 0.00 | 1.04 | 0.00 | 0.99 | -16.14 | 98.85 | -55.67 | 111.97 | 0.8574 | 72.0 | 89.2 | |
| 0.61 | 2.17 | 0.57 | 2.05 | -15.62 | 99.01 | -55.51 | 111.44 | 0.8548 | -483.7 | -388.7 | |
| 0.00 | 2.51 | 0.00 | 2.46 | -16.17 | 97.94 | -56.58 | 111.73 | 0.8650 | 104.0 | 165.5 | |
| 0.00 | 2.17 | 0.00 | 2.11 | -15.41 | 97.99 | -56.53 | 110.89 | 0.8628 | -397.0 | -331.1 | |
| 0.00 | 1.99 | 0.00 | 1.99 | -15.50 | 97.15 | -57.37 | 110.75 | 0.8698 | -237.0 | -336.5 | |
| 0.00 | 1.04 | 0.00 | 1.16 | -19.02 | 94.41 | -60.11 | 113.84 | 0.8979 | -240.0 | -329.2 | |
| 0.43 | 1.47 | 0.46 | 1.55 | -16.52 | 95.54 | -58.97 | 111.44 | 0.8845 | -470.8 | -469.4 | |
| 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. | |