SDO HMI 2014-04-24 00:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.78 | 354.83 | 29.32 | 212.99 | 17.85 | 166.47 | 26.17 | 312.01 | 0.5672 | -622.1 | -355.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.78 | 337.84 | 29.32 | 203.05 | 17.82 | 166.65 | 26.35 | 311.77 | 0.5687 | -1173.0 | -406.4 | |
| 0.00 | 0.89 | 0.00 | 0.52 | 17.23 | 164.87 | 24.57 | 312.89 | 0.5442 | 229.0 | 147.1 | |
| 0.00 | 0.98 | 0.00 | 0.58 | 18.30 | 164.54 | 24.24 | 314.74 | 0.5510 | 481.0 | 419.3 | |
| 0.00 | 1.07 | 0.00 | 0.63 | 17.41 | 164.38 | 24.08 | 313.71 | 0.5407 | 494.0 | 409.8 | |
| 0.00 | 2.04 | 0.00 | 1.19 | 17.88 | 163.03 | 22.73 | 315.99 | 0.5313 | 907.0 | 764.7 | |
| 0.00 | 0.89 | 0.00 | 0.52 | 17.84 | 162.78 | 22.48 | 316.23 | 0.5283 | 749.0 | 656.1 | |
| 0.00 | 1.60 | 0.00 | 0.94 | 18.50 | 162.81 | 22.51 | 317.10 | 0.5353 | 678.0 | 596.2 | |
| 0.00 | 0.80 | 0.00 | 0.47 | 18.30 | 162.64 | 22.34 | 317.03 | 0.5316 | 753.0 | 668.1 | |
| 0.00 | 3.20 | 0.00 | 1.87 | 18.72 | 162.67 | 22.37 | 317.57 | 0.5363 | 606.0 | 523.0 | |
| 0.00 | 0.98 | 0.00 | 0.58 | 19.41 | 162.56 | 22.26 | 318.61 | 0.5424 | 531.0 | 432.4 | |
| 0.00 | 1.16 | 0.00 | 0.68 | 19.97 | 162.29 | 21.99 | 319.65 | 0.5458 | 769.0 | 648.8 | |
| 0.00 | 0.98 | 0.00 | 0.57 | 19.23 | 162.12 | 21.82 | 318.93 | 0.5362 | 638.0 | 527.5 | |
| 0.00 | 1.42 | 0.00 | 0.83 | 18.93 | 162.04 | 21.74 | 318.64 | 0.5323 | 754.0 | 604.9 | |
| 0.00 | 0.98 | 0.00 | 0.56 | 17.37 | 161.33 | 21.03 | 317.46 | 0.5085 | 475.0 | 380.1 | |
| 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. | |