SDO HMI 2014-06-03 15:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.02 | 292.70 | 31.17 | 157.65 | -4.75 | 300.39 | -22.71 | 101.26 | 0.3940 | 528.3 | 377.2 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.51 | 11.93 | 3.48 | 6.38 | -5.81 | 301.52 | -21.57 | 104.58 | 0.3796 | 1031.1 | 721.6 | |
| 9.94 | 17.27 | 5.34 | 9.27 | -5.93 | 301.09 | -22.01 | 104.63 | 0.3868 | 1020.2 | 510.2 | |
| 0.54 | 2.53 | 0.29 | 1.36 | -6.39 | 301.07 | -22.03 | 105.77 | 0.3889 | 754.8 | 652.8 | |
| 36.79 | 206.46 | 19.73 | 110.72 | -4.28 | 300.89 | -22.21 | 100.32 | 0.3847 | 1288.6 | 449.1 | |
| 0.72 | -4.00 | 0.39 | -4.00 | -4.68 | 300.71 | -22.39 | 101.25 | 0.3887 | 611.6 | 999999 | |
| 0.00 | 1.99 | 0.00 | 1.07 | -6.60 | 300.63 | -22.47 | 106.01 | 0.3966 | 557.0 | 398.4 | |
| 0.00 | 1.08 | 0.00 | 0.58 | -5.87 | 300.63 | -22.47 | 104.20 | 0.3938 | 571.0 | 479.2 | |
| 0.00 | 1.72 | 0.00 | 0.93 | -6.42 | 300.54 | -22.56 | 105.50 | 0.3973 | 775.0 | 581.4 | |
| 0.00 | 1.90 | 0.00 | 1.02 | -6.02 | 300.43 | -22.67 | 104.46 | 0.3976 | 779.0 | 641.0 | |
| 0.27 | -4.00 | 0.15 | -4.00 | -4.01 | 300.34 | -22.76 | 99.39 | 0.3928 | 753.0 | 999999 | |
| 0.00 | 3.80 | 0.00 | 2.05 | -5.78 | 300.10 | -22.99 | 103.68 | 0.4017 | 728.0 | 550.9 | |
| 0.00 | 1.27 | 0.00 | 0.68 | -4.01 | 300.07 | -23.03 | 99.29 | 0.3970 | 693.0 | 540.6 | |
| 0.00 | 10.40 | 0.00 | 5.65 | -5.87 | 299.43 | -23.66 | 103.54 | 0.4124 | 720.0 | 609.2 | |
| 0.63 | 1.54 | 0.35 | 0.84 | -6.60 | 299.03 | -24.07 | 105.05 | 0.4213 | -946.1 | -839.1 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -3.49 | 299.09 | -24.01 | 97.68 | 0.4115 | 747.0 | 615.6 | |
| 1.18 | 2.26 | 0.64 | 1.24 | -6.60 | 298.76 | -24.34 | 104.90 | 0.4254 | -980.5 | -786.3 | |
| 0.00 | 0.81 | 0.00 | 0.45 | -6.44 | 298.37 | -24.73 | 104.34 | 0.4309 | -696.0 | -520.2 | |
| 0.00 | 1.18 | 0.00 | 0.64 | -4.00 | 298.40 | -24.69 | 98.70 | 0.4234 | 750.0 | 637.2 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -3.91 | 298.07 | -25.03 | 98.38 | 0.4284 | 624.0 | 403.1 | |
| 0.90 | 1.81 | 0.50 | 0.99 | -3.85 | 297.77 | -25.33 | 98.15 | 0.4330 | 842.3 | 698.8 | |
| 0.00 | 1.72 | 0.00 | 0.96 | -9.45 | 297.18 | -25.92 | 110.15 | 0.4612 | -791.0 | -631.9 | |
| 0.00 | 0.99 | 0.00 | 0.55 | -3.21 | 297.35 | -25.75 | 96.57 | 0.4384 | 808.0 | 635.7 | |
| 0.54 | 1.63 | 0.30 | 0.90 | -7.11 | 297.11 | -25.99 | 105.17 | 0.4524 | -916.5 | -777.2 | |
| 0.00 | 3.53 | 0.00 | 1.94 | -2.87 | 297.29 | -25.81 | 95.80 | 0.4388 | 756.0 | 640.8 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -5.61 | 296.71 | -26.39 | 101.74 | 0.4536 | -813.0 | -701.7 | |
| 0.00 | 1.36 | 0.00 | 0.76 | -9.07 | 296.45 | -26.65 | 108.93 | 0.4701 | -777.0 | -673.3 | |
| 0.00 | 0.72 | 0.00 | 0.40 | -7.45 | 296.57 | -26.53 | 105.61 | 0.4617 | -779.0 | -641.2 | |
| 0.00 | 2.62 | 0.00 | 1.47 | -7.48 | 296.26 | -26.84 | 105.51 | 0.4665 | -742.0 | -606.4 | |
| 0.00 | 1.54 | 0.00 | 0.86 | -6.62 | 296.25 | -26.85 | 103.70 | 0.4637 | -841.0 | -725.6 | |
| 0.00 | 0.90 | 0.00 | 0.50 | -5.03 | 296.23 | -26.87 | 100.30 | 0.4595 | -839.0 | -733.4 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -7.87 | 296.06 | -27.04 | 106.24 | 0.4709 | -737.0 | -601.3 | |
| 0.00 | 0.90 | 0.00 | 0.51 | -7.05 | 296.05 | -27.05 | 104.51 | 0.4681 | -727.0 | -627.0 | |
| 0.00 | 1.72 | 0.00 | 0.96 | -5.00 | 295.99 | -27.11 | 100.15 | 0.4631 | -762.0 | -672.4 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -3.71 | 294.77 | -28.33 | 97.10 | 0.4792 | -771.0 | -626.5 | |
| 0.00 | 0.72 | 0.00 | 0.41 | -5.24 | 294.46 | -28.64 | 100.15 | 0.4869 | -545.0 | -493.5 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -4.63 | 294.42 | -28.68 | 98.89 | 0.4862 | -632.0 | -595.9 | |
| 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. | |