SDO HMI 2014-04-23 21:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 55.51 | 360.00 | 32.89 | 213.15 | 17.83 | 166.49 | 24.53 | 313.80 | 0.5498 | -703.8 | -357.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.95 | 341.61 | 1.16 | 202.51 | 18.34 | 166.84 | 24.88 | 314.09 | 0.5582 | -756.1 | -413.4 | |
| 52.23 | -1.00 | 30.96 | -1.00 | 17.78 | 166.68 | 24.72 | 313.50 | 0.5512 | -1235.9 | 999999 | |
| 0.00 | 0.89 | 0.00 | 0.52 | 17.35 | 164.55 | 22.59 | 315.43 | 0.5245 | 520.0 | 451.6 | |
| 0.00 | 0.98 | 0.00 | 0.57 | 18.56 | 164.51 | 22.55 | 317.13 | 0.5364 | 536.0 | 341.4 | |
| 1.33 | 4.35 | 0.77 | 2.51 | 17.92 | 163.02 | 21.06 | 318.18 | 0.5148 | 839.1 | 628.4 | |
| 0.00 | 1.07 | 0.00 | 0.61 | 17.91 | 162.75 | 20.79 | 318.54 | 0.5120 | 899.0 | 780.2 | |
| 0.00 | 2.40 | 0.00 | 1.39 | 18.43 | 162.75 | 20.79 | 319.24 | 0.5177 | 660.0 | 636.0 | |
| 0.00 | 1.51 | 0.00 | 0.88 | 18.73 | 162.75 | 20.79 | 319.63 | 0.5210 | 683.0 | 625.1 | |
| 0.00 | 1.24 | 0.00 | 0.72 | 18.07 | 162.63 | 20.67 | 318.91 | 0.5126 | 714.0 | 667.2 | |
| 0.00 | 0.98 | 0.00 | 0.56 | 18.52 | 162.35 | 20.39 | 319.89 | 0.5148 | 805.0 | 703.9 | |
| 0.00 | 1.15 | 0.00 | 0.66 | 17.76 | 162.26 | 20.30 | 319.01 | 0.5056 | 703.0 | 533.1 | |
| 0.00 | 1.15 | 0.00 | 0.66 | 17.63 | 162.14 | 20.18 | 318.98 | 0.5029 | 777.0 | 637.5 | |
| 0.00 | 1.69 | 0.00 | 0.99 | 20.00 | 162.31 | 20.35 | 321.85 | 0.5310 | 731.0 | 593.2 | |
| 0.00 | 0.98 | 0.00 | 0.57 | 19.37 | 162.02 | 20.06 | 321.44 | 0.5211 | 579.0 | 493.5 | |
| 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. | |