SDO HMI 2014-04-23 06:00:35 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.57 | 381.50 | 30.59 | 213.81 | 17.76 | 166.56 | 16.35 | 325.02 | 0.4692 | -675.8 | -333.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 53.32 | 351.29 | 29.92 | 197.18 | 17.73 | 166.93 | 16.72 | 324.33 | 0.4718 | -1410.3 | -433.6 | |
| 0.00 | 1.33 | 0.00 | 0.74 | 18.11 | 163.23 | 13.01 | 331.19 | 0.4460 | 737.0 | 562.7 | |
| 0.00 | 1.33 | 0.00 | 0.74 | 19.09 | 163.01 | 12.80 | 332.67 | 0.4578 | 825.0 | 657.9 | |
| 0.00 | 1.24 | 0.00 | 0.69 | 18.56 | 162.93 | 12.72 | 332.23 | 0.4500 | 676.0 | 572.1 | |
| 0.00 | 1.51 | 0.00 | 0.84 | 18.76 | 162.92 | 12.71 | 332.48 | 0.4526 | 726.0 | 578.1 | |
| 0.00 | 8.18 | 0.00 | 4.51 | 18.10 | 162.83 | 12.62 | 331.91 | 0.4430 | 885.0 | 838.3 | |
| 0.00 | 3.55 | 0.00 | 1.97 | 18.82 | 162.56 | 12.35 | 333.20 | 0.4509 | 701.0 | 634.9 | |
| 0.00 | 1.51 | 0.00 | 0.83 | 18.00 | 162.50 | 12.29 | 332.42 | 0.4391 | 917.0 | 771.1 | |
| 0.00 | 0.98 | 0.00 | 0.54 | 18.81 | 162.27 | 12.06 | 333.74 | 0.4487 | 651.0 | 565.8 | |
| 0.00 | 1.16 | 0.00 | 0.64 | 18.28 | 162.00 | 11.79 | 333.68 | 0.4395 | 755.0 | 548.8 | |
| 0.36 | 2.22 | 0.19 | 1.21 | 17.49 | 161.43 | 11.22 | 333.95 | 0.4244 | 904.5 | 698.7 | |
| 0.00 | 1.07 | 0.00 | 0.58 | 17.55 | 161.21 | 11.00 | 334.46 | 0.4238 | 899.0 | 759.0 | |
| 0.00 | 2.13 | 0.00 | 1.16 | 17.29 | 161.19 | 10.98 | 334.22 | 0.4200 | 831.0 | 683.1 | |
| 0.00 | 1.78 | 0.00 | 0.97 | 17.54 | 160.37 | 10.16 | 336.16 | 0.4180 | 915.0 | 712.5 | |
| 0.89 | 2.22 | 0.48 | 1.21 | 17.18 | 160.32 | 10.11 | 335.91 | 0.4125 | 991.8 | 851.3 | |
| 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. | |