| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.44 | 42.03 | 4.73 | 23.77 | -8.30 | 8.84 | -28.94 | 95.76 | 0.4830 | 452.1 | 371.5 | |
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back to the solar disc SDO HMI 2014-04-04 12:00:32 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.23 | 0.00 | 0.67 | -8.12 | 12.56 | -25.22 | 95.61 | 0.4257 | 772.0 | 717.6 | |
| 0.00 | 1.32 | 0.00 | 0.72 | -7.85 | 12.58 | -25.20 | 94.97 | 0.4252 | 814.0 | 556.5 | |
| 0.00 | 1.23 | 0.00 | 0.68 | -6.57 | 11.65 | -26.13 | 91.99 | 0.4397 | 791.0 | 620.2 | |
| 4.22 | 9.14 | 2.34 | 5.08 | -8.36 | 10.78 | -27.00 | 95.99 | 0.4535 | 973.7 | 721.2 | |
| 1.05 | 5.01 | 0.59 | 2.81 | -8.67 | 9.77 | -28.01 | 96.56 | 0.4693 | 977.6 | 852.1 | |
| 0.70 | -5.00 | 0.39 | -5.00 | -8.72 | 9.59 | -28.19 | 96.65 | 0.4720 | 952.5 | 999999 | |
| 0.00 | 2.29 | 0.00 | 1.29 | -9.04 | 9.39 | -28.39 | 97.30 | 0.4754 | 791.0 | 637.0 | |
| 0.00 | 1.41 | 0.00 | 0.79 | -10.75 | 9.19 | -28.59 | 100.84 | 0.4806 | 651.0 | 483.0 | |
| 0.00 | 2.20 | 0.00 | 1.23 | -7.09 | 9.47 | -28.31 | 93.18 | 0.4732 | 879.0 | 682.8 | |
| 1.41 | 3.52 | 0.79 | 1.98 | -9.21 | 9.27 | -28.51 | 97.66 | 0.4773 | 884.6 | 729.5 | |
| 0.00 | 2.11 | 0.00 | 1.19 | -8.83 | 9.30 | -28.48 | 96.84 | 0.4765 | 641.0 | 484.4 | |
| 0.00 | 2.11 | 0.00 | 1.19 | -8.67 | 8.73 | -29.05 | 96.47 | 0.4851 | 489.0 | 363.6 | |
| 0.00 | 1.14 | 0.00 | 0.65 | -9.46 | 8.31 | -29.47 | 98.04 | 0.4921 | 698.0 | 524.0 | |
| 0.62 | 2.46 | 0.36 | 1.43 | -7.91 | 5.91 | -31.87 | 94.80 | 0.5269 | 672.6 | 541.0 | |
| 0.00 | 1.32 | 0.00 | 0.77 | -6.48 | 5.09 | -32.69 | 92.11 | 0.5391 | -837.0 | -735.0 | |
| 0.00 | 0.88 | 0.00 | 0.52 | -8.62 | 4.72 | -33.05 | 96.09 | 0.5445 | -641.0 | -515.6 | |
| 0.00 | 1.23 | 0.00 | 0.73 | -5.89 | 4.81 | -32.97 | 91.04 | 0.5435 | -723.0 | -551.4 | |
| 0.44 | 3.43 | 0.26 | 2.04 | -7.65 | 4.02 | -33.76 | 94.28 | 0.5545 | -950.6 | -768.5 | |
| 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. | |