SDO HMI 2014-04-07 17:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.72 | 0.00 | 11.60 | -8.19 | 9.48 | 14.04 | 260.40 | 0.2452 | 306.2 | 330.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.97 | 0.00 | 0.50 | -8.20 | 12.84 | 17.40 | 262.20 | 0.3001 | 708.0 | 528.7 | |
| 0.00 | 2.64 | 0.00 | 1.37 | -8.12 | 12.58 | 17.14 | 262.39 | 0.2957 | 718.0 | 623.0 | |
| 0.00 | 1.94 | 0.00 | 1.00 | -5.94 | 11.97 | 16.53 | 269.84 | 0.2842 | 872.0 | 710.4 | |
| 0.00 | 2.38 | 0.00 | 1.22 | -8.59 | 10.90 | 15.46 | 260.04 | 0.2688 | 991.0 | 752.0 | |
| 0.00 | 4.22 | 0.00 | 2.17 | -9.13 | 10.70 | 15.26 | 257.90 | 0.2669 | 700.0 | 722.5 | |
| 0.00 | 1.14 | 0.00 | 0.59 | -9.17 | 10.32 | 14.88 | 257.50 | 0.2609 | 986.0 | 835.0 | |
| 0.00 | 1.50 | 0.00 | 0.76 | -7.57 | 9.70 | 14.26 | 263.47 | 0.2469 | 887.0 | 730.9 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -7.84 | 9.61 | 14.17 | 262.34 | 0.2459 | 879.0 | 666.7 | |
| 0.00 | 2.38 | 0.00 | 1.20 | -7.45 | 6.69 | 11.25 | 262.71 | 0.1958 | -862.0 | -636.2 | |
| 0.00 | 0.62 | 0.00 | 0.31 | -7.11 | 6.00 | 10.56 | 264.21 | 0.1836 | -899.0 | -812.3 | |
| 0.00 | 1.67 | 0.00 | 0.84 | -7.57 | 5.46 | 10.02 | 261.34 | 0.1752 | -916.0 | -782.6 | |
| 0.00 | 1.32 | 0.00 | 0.66 | -8.11 | 4.92 | 9.48 | 257.65 | 0.1676 | -902.0 | -763.7 | |
| 0.00 | 0.97 | 0.00 | 0.49 | -11.62 | 3.99 | 8.55 | 236.51 | 0.1755 | 818.0 | 671.2 | |
| 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. | |