| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.29 | 31.10 | 5.25 | 21.31 | 13.04 | 92.18 | -43.63 | 77.93 | 0.6868 | 186.2 | 141.9 | |
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back to the solar disc SDO HMI 2014-10-04 17:00:32 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.32 | 0.00 | 0.75 | 12.00 | 105.83 | -29.98 | 77.31 | 0.5030 | 728.0 | 629.9 | |
| 0.00 | 1.14 | 0.00 | 0.66 | 13.06 | 104.69 | -31.12 | 75.58 | 0.5219 | 555.0 | 414.8 | |
| 0.00 | 1.32 | 0.00 | 0.77 | 10.02 | 103.24 | -32.57 | 81.61 | 0.5380 | -486.0 | -397.5 | |
| 0.00 | 1.49 | 0.00 | 0.92 | 12.45 | 99.22 | -36.59 | 77.89 | 0.5975 | -843.0 | -678.7 | |
| 0.00 | 1.23 | 0.00 | 0.78 | 14.44 | 97.22 | -38.59 | 75.02 | 0.6276 | -591.0 | -547.7 | |
| 0.00 | 0.79 | 0.00 | 0.50 | 14.49 | 97.01 | -38.80 | 74.99 | 0.6304 | -555.0 | -410.7 | |
| 0.00 | 1.14 | 0.00 | 0.72 | 10.74 | 97.13 | -38.68 | 80.96 | 0.6241 | -533.0 | -486.2 | |
| 0.00 | 2.37 | 0.00 | 1.50 | 7.96 | 97.06 | -38.75 | 85.43 | 0.6241 | -683.0 | -633.6 | |
| 0.00 | 1.32 | 0.00 | 0.93 | 14.23 | 90.23 | -45.58 | 76.44 | 0.7144 | -527.0 | -391.3 | |
| 0.00 | 0.88 | 0.00 | 0.63 | 16.85 | 89.16 | -46.65 | 72.98 | 0.7301 | 521.0 | 443.6 | |
| 7.29 | 13.97 | 5.25 | 10.06 | 13.23 | 89.06 | -46.75 | 77.95 | 0.7274 | 869.9 | 641.9 | |
| 0.00 | 1.23 | 0.00 | 0.92 | 14.79 | 87.25 | -48.56 | 76.00 | 0.7493 | 618.0 | 424.7 | |
| 0.00 | 2.90 | 0.00 | 2.17 | 14.90 | 87.12 | -48.69 | 75.87 | 0.7508 | 441.0 | 464.6 | |
| 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. | |