SDO HMI 2014-04-24 12:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.22 | 373.85 | 34.79 | 239.42 | 17.90 | 166.25 | 32.53 | 306.13 | 0.6357 | -784.9 | -276.4 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.22 | 348.80 | 34.79 | 223.84 | 17.90 | 166.43 | 32.71 | 305.98 | 0.6377 | -1247.2 | -324.3 | |
| 0.00 | 6.58 | 0.00 | 4.12 | 17.33 | 164.75 | 31.03 | 306.60 | 0.6152 | -482.0 | -184.7 | |
| 0.00 | 1.24 | 0.00 | 0.78 | 17.42 | 164.47 | 30.75 | 306.95 | 0.6127 | -363.0 | -317.8 | |
| 0.00 | 2.22 | 0.00 | 1.38 | 17.12 | 164.34 | 30.62 | 306.65 | 0.6090 | 588.0 | 484.2 | |
| 0.00 | 1.24 | 0.00 | 0.77 | 17.54 | 163.43 | 29.71 | 308.03 | 0.6022 | 528.0 | 485.6 | |
| 0.00 | 2.31 | 0.00 | 1.43 | 17.76 | 163.36 | 29.64 | 308.40 | 0.6032 | 575.0 | 515.1 | |
| 0.00 | 1.24 | 0.00 | 0.77 | 18.09 | 163.38 | 29.67 | 308.82 | 0.6061 | 514.0 | 451.9 | |
| 0.00 | 2.22 | 0.00 | 1.38 | 17.88 | 163.20 | 29.48 | 308.71 | 0.6025 | 774.0 | 669.7 | |
| 0.00 | 1.24 | 0.00 | 0.77 | 18.36 | 162.96 | 29.24 | 309.58 | 0.6038 | 527.0 | 466.9 | |
| 0.00 | 1.87 | 0.00 | 1.15 | 18.13 | 162.77 | 29.05 | 309.44 | 0.5998 | 703.0 | 656.9 | |
| 0.00 | 0.98 | 0.00 | 0.60 | 18.32 | 162.73 | 29.02 | 309.74 | 0.6010 | 646.0 | 572.9 | |
| 0.00 | 2.58 | 0.00 | 1.60 | 18.55 | 162.67 | 28.95 | 310.10 | 0.6022 | 634.0 | 464.3 | |
| 0.00 | 0.53 | 0.00 | 0.33 | 18.12 | 162.48 | 28.76 | 309.70 | 0.5966 | 589.0 | 631.8 | |
| 0.00 | 0.80 | 0.00 | 0.50 | 20.36 | 162.47 | 28.76 | 312.65 | 0.6155 | 643.0 | 565.9 | |
| 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. | |