| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.04 | 0.00 | 14.36 | -18.13 | 77.51 | -39.59 | 122.94 | 0.7234 | 455.4 | 469.1 | |
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back to the solar disc SDO HMI 2014-10-06 03:00:32 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.70 | 0.00 | 0.48 | -20.81 | 82.36 | -34.74 | 129.54 | 0.6930 | 671.0 | 591.4 | |
| 0.00 | 0.97 | 0.00 | 0.68 | -22.37 | 81.25 | -35.85 | 130.51 | 0.7147 | 86.0 | 143.3 | |
| 0.00 | 1.41 | 0.00 | 0.99 | -20.49 | 79.83 | -37.27 | 127.28 | 0.7152 | 558.0 | 428.8 | |
| 0.00 | 0.26 | 0.00 | 0.19 | -20.16 | 79.72 | -37.38 | 126.82 | 0.7141 | 558.0 | 576.3 | |
| 0.00 | 3.87 | 0.00 | 2.68 | -18.15 | 79.62 | -37.48 | 124.31 | 0.7023 | 887.0 | 749.4 | |
| 0.00 | 2.02 | 0.00 | 1.37 | -15.17 | 79.69 | -37.41 | 120.57 | 0.6834 | 817.0 | 688.5 | |
| 0.00 | 0.97 | 0.00 | 0.68 | -16.47 | 77.27 | -39.83 | 120.70 | 0.7167 | 568.0 | 528.4 | |
| 0.00 | 1.41 | 0.00 | 1.00 | -16.75 | 77.03 | -40.07 | 120.90 | 0.7207 | 823.0 | 689.5 | |
| 0.00 | 1.05 | 0.00 | 0.75 | -16.39 | 77.08 | -40.02 | 120.48 | 0.7182 | 576.0 | 522.8 | |
| 0.00 | 1.32 | 0.00 | 0.95 | -16.61 | 76.33 | -40.77 | 120.30 | 0.7272 | 536.0 | 475.5 | |
| 0.00 | 1.67 | 0.00 | 1.21 | -16.84 | 76.18 | -40.92 | 120.51 | 0.7300 | 669.0 | 529.0 | |
| 0.00 | 0.97 | 0.00 | 0.73 | -19.41 | 75.09 | -42.01 | 122.96 | 0.7546 | 447.0 | 387.0 | |
| 0.00 | 1.05 | 0.00 | 0.77 | -17.05 | 75.54 | -41.56 | 120.40 | 0.7377 | 590.0 | 418.9 | |
| 0.00 | 0.70 | 0.00 | 0.52 | -17.03 | 74.99 | -42.11 | 120.06 | 0.7430 | 546.0 | 476.8 | |
| 0.00 | 0.97 | 0.00 | 0.81 | -23.02 | 71.11 | -45.99 | 124.84 | 0.8087 | -497.0 | -344.3 | |
| 0.00 | 0.70 | 0.00 | 0.55 | -18.92 | 72.58 | -44.52 | 120.99 | 0.7759 | -548.0 | -431.5 | |
| 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. | |