| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.10 | 0.00 | 11.27 | -8.73 | 8.75 | 12.75 | 256.62 | 0.2288 | 336.9 | 311.2 | |
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back to the solar disc SDO HMI 2014-04-07 16:00:32 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.06 | 0.00 | 0.55 | -8.24 | 12.95 | 16.96 | 261.90 | 0.2929 | 767.0 | 630.4 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -6.15 | 12.59 | 16.60 | 269.10 | 0.2853 | 778.0 | 691.5 | |
| 0.00 | 0.88 | 0.00 | 0.45 | -8.16 | 12.60 | 16.61 | 262.05 | 0.2869 | 864.0 | 680.1 | |
| 0.00 | 1.50 | 0.00 | 0.77 | -5.90 | 11.95 | 15.96 | 270.06 | 0.2748 | 745.0 | 690.5 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -8.04 | 11.55 | 15.56 | 262.09 | 0.2694 | 607.0 | 579.8 | |
| 0.00 | 3.52 | 0.00 | 1.81 | -8.54 | 10.88 | 14.89 | 259.90 | 0.2593 | 863.0 | 676.3 | |
| 0.00 | 1.23 | 0.00 | 0.63 | -9.12 | 10.59 | 14.60 | 257.50 | 0.2560 | 1050.0 | 899.9 | |
| 0.00 | 0.97 | 0.00 | 0.50 | -9.19 | 10.31 | 14.32 | 257.03 | 0.2517 | 1019.0 | 840.1 | |
| 0.00 | 1.06 | 0.00 | 0.54 | -8.20 | 8.65 | 12.66 | 259.96 | 0.2213 | 844.0 | 689.1 | |
| 0.00 | 1.32 | 0.00 | 0.67 | -10.40 | 8.51 | 12.52 | 250.24 | 0.2276 | 889.0 | 570.5 | |
| 0.00 | 1.14 | 0.00 | 0.58 | -7.49 | 6.72 | 10.72 | 262.20 | 0.1871 | -890.0 | -725.2 | |
| 0.00 | 1.23 | 0.00 | 0.62 | -7.09 | 5.97 | 9.98 | 264.05 | 0.1737 | -819.0 | -667.6 | |
| 0.00 | 1.32 | 0.00 | 0.66 | -7.69 | 5.58 | 9.59 | 260.25 | 0.1683 | -849.0 | -688.3 | |
| 0.00 | 1.41 | 0.00 | 0.71 | -8.15 | 4.92 | 8.93 | 256.73 | 0.1585 | -978.0 | -736.8 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -8.33 | 4.89 | 8.90 | 255.58 | 0.1588 | -785.0 | -647.3 | |
| 0.00 | 1.32 | 0.00 | 0.67 | -12.34 | 4.75 | 8.76 | 233.78 | 0.1853 | 819.0 | 636.0 | |
| 0.00 | 1.14 | 0.00 | 0.58 | -15.57 | 3.08 | 7.09 | 215.87 | 0.2038 | 803.0 | 686.3 | |
| 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. | |