SDO HMI 2014-04-18 07:00:34 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.87 | 163.49 | 20.23 | 125.09 | 12.02 | 262.23 | 46.52 | 291.11 | 0.7606 | -449.3 | -201.5 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.91 | 144.10 | 10.92 | 112.71 | 11.93 | 263.77 | 48.07 | 290.13 | 0.7775 | -849.0 | -274.3 | |
| 11.96 | -1.00 | 9.31 | -1.00 | 11.63 | 263.52 | 47.81 | 289.85 | 0.7739 | -1156.2 | 999999 | |
| 0.00 | 1.15 | 0.00 | 0.91 | 18.49 | 261.57 | 45.87 | 299.00 | 0.7805 | -601.0 | -468.5 | |
| 0.00 | 0.80 | 0.00 | 0.58 | 12.12 | 259.63 | 43.93 | 292.05 | 0.7341 | -512.0 | -429.9 | |
| 0.00 | 1.77 | 0.00 | 1.31 | 17.33 | 258.32 | 42.61 | 299.26 | 0.7431 | -533.0 | -534.9 | |
| 0.00 | 0.97 | 0.00 | 0.69 | 16.41 | 256.13 | 40.42 | 299.32 | 0.7158 | 459.0 | 394.3 | |
| 0.00 | 0.80 | 0.00 | 0.54 | 12.81 | 255.09 | 39.38 | 295.19 | 0.6861 | 582.0 | 481.1 | |
| 0.00 | 0.89 | 0.00 | 0.54 | 12.81 | 245.78 | 30.07 | 301.50 | 0.5753 | 698.0 | 651.5 | |
| 0.00 | 1.68 | 0.00 | 1.02 | 13.03 | 245.77 | 30.07 | 301.84 | 0.5768 | 647.0 | 505.9 | |
| 0.00 | 2.92 | 0.00 | 1.76 | 12.88 | 245.33 | 29.62 | 302.00 | 0.5703 | 829.0 | 639.2 | |
| 0.00 | 1.68 | 0.00 | 1.01 | 12.62 | 245.11 | 29.41 | 301.78 | 0.5658 | 710.0 | 629.7 | |
| 0.00 | 3.37 | 0.00 | 2.02 | 12.76 | 244.85 | 29.14 | 302.23 | 0.5636 | 835.0 | 676.0 | |
| 0.00 | 0.97 | 0.00 | 0.58 | 13.11 | 244.89 | 29.19 | 302.73 | 0.5668 | 725.0 | 566.8 | |
| 0.00 | 1.24 | 0.00 | 0.74 | 13.27 | 244.77 | 29.07 | 303.07 | 0.5664 | 607.0 | 562.8 | |
| 0.00 | 1.15 | 0.00 | 0.68 | 15.77 | 240.53 | 24.82 | 311.07 | 0.5380 | 658.0 | 512.8 | |
| 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. | |