SDO HMI 2014-04-23 22:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.98 | 373.46 | 35.09 | 222.12 | 17.83 | 166.46 | 25.05 | 313.22 | 0.5552 | -734.2 | -319.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 57.65 | 354.09 | 34.32 | 210.85 | 17.80 | 166.66 | 25.25 | 312.94 | 0.5569 | -1215.7 | -371.7 | |
| 0.00 | 1.24 | 0.00 | 0.73 | 17.46 | 164.42 | 23.01 | 315.06 | 0.5300 | 550.0 | 376.6 | |
| 0.00 | 1.07 | 0.00 | 0.63 | 18.64 | 164.48 | 23.08 | 316.59 | 0.5426 | 442.0 | 335.1 | |
| 1.33 | 4.09 | 0.77 | 2.37 | 17.90 | 163.01 | 21.60 | 317.45 | 0.5201 | 793.7 | 622.5 | |
| 0.00 | 1.07 | 0.00 | 0.62 | 17.86 | 162.76 | 21.36 | 317.71 | 0.5172 | 833.0 | 715.2 | |
| 0.00 | 1.51 | 0.00 | 0.88 | 18.49 | 162.81 | 21.40 | 318.49 | 0.5243 | 594.0 | 543.9 | |
| 0.00 | 2.58 | 0.00 | 1.50 | 18.74 | 162.67 | 21.27 | 319.01 | 0.5258 | 547.0 | 551.4 | |
| 0.00 | 2.31 | 0.00 | 1.34 | 18.57 | 162.41 | 21.01 | 319.13 | 0.5213 | 743.0 | 613.7 | |
| 0.00 | 1.42 | 0.00 | 0.82 | 17.68 | 162.16 | 20.76 | 318.26 | 0.5092 | 744.0 | 503.4 | |
| 0.00 | 1.07 | 0.00 | 0.62 | 18.27 | 162.20 | 20.80 | 319.00 | 0.5160 | 688.0 | 499.0 | |
| 0.00 | 1.24 | 0.00 | 0.73 | 20.02 | 162.30 | 20.90 | 321.14 | 0.5362 | 733.0 | 652.9 | |
| 0.00 | 0.53 | 0.00 | 0.31 | 18.99 | 162.06 | 20.65 | 320.15 | 0.5225 | 808.0 | 680.8 | |
| 0.00 | 1.24 | 0.00 | 0.72 | 19.42 | 160.89 | 19.48 | 322.29 | 0.5164 | 591.0 | 473.6 | |
| 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. | |