| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 16.79 | 61.76 | 9.60 | 35.36 | 8.22 | 195.20 | -28.07 | 68.41 | 0.5026 | -83.0 | -14.4 | |
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back to the solar disc SDO HMI 2014-05-14 23:00:37 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.42 | 0.00 | 1.36 | 7.69 | 196.95 | -26.31 | 68.22 | 0.4750 | -791.0 | -734.9 | |
| 0.36 | 1.62 | 0.20 | 0.91 | 7.69 | 196.71 | -26.55 | 68.38 | 0.4785 | -874.2 | -716.3 | |
| 0.00 | 3.14 | 0.00 | 1.77 | 8.31 | 196.64 | -26.63 | 67.23 | 0.4830 | -747.0 | -598.3 | |
| 9.33 | 24.05 | 5.28 | 13.61 | 7.97 | 196.45 | -26.81 | 68.02 | 0.4837 | -976.3 | -625.0 | |
| 0.81 | -4.00 | 0.46 | -4.00 | 7.83 | 196.15 | -27.11 | 68.52 | 0.4872 | -716.8 | 999999 | |
| 0.00 | 1.26 | 0.00 | 0.72 | 8.52 | 195.76 | -27.51 | 67.49 | 0.4965 | -689.0 | -554.9 | |
| 0.00 | 2.24 | 0.00 | 1.28 | 8.55 | 195.44 | -27.82 | 67.64 | 0.5011 | -749.0 | -493.2 | |
| 0.00 | 0.99 | 0.00 | 0.57 | 8.95 | 194.51 | -28.76 | 67.56 | 0.5163 | 894.0 | 619.6 | |
| 0.00 | 0.90 | 0.00 | 0.52 | 8.80 | 194.38 | -28.89 | 67.93 | 0.5172 | 671.0 | 525.5 | |
| 0.00 | 0.63 | 0.00 | 0.36 | 9.32 | 194.26 | -29.00 | 67.05 | 0.5217 | 682.0 | 585.7 | |
| 0.00 | 0.90 | 0.00 | 0.52 | 8.12 | 194.15 | -29.11 | 69.30 | 0.5169 | 649.0 | 496.7 | |
| 0.00 | 0.63 | 0.00 | 0.37 | 9.21 | 193.99 | -29.28 | 67.44 | 0.5248 | 767.0 | 703.7 | |
| 0.00 | 1.62 | 0.00 | 0.94 | 8.53 | 194.01 | -29.25 | 68.65 | 0.5209 | 819.0 | 663.5 | |
| 0.00 | 0.99 | 0.00 | 0.57 | 8.50 | 193.70 | -29.57 | 68.90 | 0.5252 | 809.0 | 782.5 | |
| 1.35 | 6.01 | 0.78 | 3.50 | 8.84 | 193.63 | -29.63 | 68.33 | 0.5278 | 716.8 | 654.6 | |
| 1.62 | 9.51 | 0.94 | 5.53 | 8.10 | 193.63 | -29.64 | 69.66 | 0.5242 | 1075.9 | 750.8 | |
| 3.32 | 4.85 | 1.94 | 2.83 | 8.48 | 193.38 | -29.88 | 69.14 | 0.5294 | 767.1 | 564.7 | |
| 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. | |