| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 70.91 | 438.68 | 37.20 | 230.25 | 12.55 | 13.65 | -3.77 | 11.27 | 0.3302 | -948.8 | -390.9 | |
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back to the solar disc SDO HMI 2014-04-06 01:00:32 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.14 | 0.00 | 0.60 | 12.23 | 15.89 | -1.53 | 4.69 | 0.3197 | -649.0 | -490.0 | |
| 70.38 | 414.73 | 36.92 | 217.69 | 12.59 | 13.77 | -3.65 | 10.89 | 0.3304 | -1372.8 | -425.5 | |
| 0.00 | 1.32 | 0.00 | 0.68 | 9.49 | 12.58 | -4.83 | 17.04 | 0.2850 | 798.0 | 659.4 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 11.37 | 12.37 | -5.05 | 15.90 | 0.3161 | -597.0 | -456.2 | |
| 0.00 | 1.41 | 0.00 | 0.74 | 11.72 | 12.33 | -5.08 | 15.71 | 0.3218 | -463.0 | -384.6 | |
| 0.00 | 1.41 | 0.00 | 0.74 | 12.60 | 12.22 | -5.19 | 15.29 | 0.3364 | -521.0 | -422.6 | |
| 0.00 | 1.06 | 0.00 | 0.55 | 10.09 | 12.08 | -5.33 | 18.02 | 0.2970 | 893.0 | 727.8 | |
| 0.53 | 3.26 | 0.28 | 1.70 | 11.85 | 11.99 | -5.42 | 16.59 | 0.3254 | -615.5 | -351.9 | |
| 0.00 | 0.70 | 0.00 | 0.38 | 15.42 | 11.73 | -5.69 | 14.52 | 0.3830 | 571.0 | 488.9 | |
| 0.00 | 3.96 | 0.00 | 2.08 | 12.04 | 11.46 | -5.95 | 17.91 | 0.3311 | -637.0 | -354.2 | |
| 0.00 | 1.23 | 0.00 | 0.64 | 11.41 | 11.26 | -6.15 | 19.11 | 0.3223 | 835.0 | 719.2 | |
| 0.00 | 0.97 | 0.00 | 0.51 | 12.55 | 11.18 | -6.24 | 18.23 | 0.3406 | 679.0 | 552.5 | |
| 0.00 | 1.85 | 0.00 | 0.97 | 11.51 | 10.98 | -6.43 | 19.81 | 0.3254 | 878.0 | 699.4 | |
| 0.00 | 2.82 | 0.00 | 1.48 | 11.87 | 10.61 | -6.81 | 20.49 | 0.3330 | 959.0 | 753.7 | |
| 0.00 | 1.85 | 0.00 | 0.98 | 11.78 | 8.35 | -9.07 | 26.57 | 0.3464 | 149.0 | 251.8 | |
| 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. | |