SDO HMI 2014-04-08 10:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.36 | 143.74 | 32.46 | 97.73 | 2.99 | 28.07 | 41.98 | 281.56 | 0.6823 | 44.4 | -60.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.11 | 4.76 | 1.56 | 3.52 | 1.80 | 33.45 | 47.36 | 277.98 | 0.7448 | -499.3 | -375.5 | |
| 1.59 | 2.91 | 1.17 | 2.15 | 2.27 | 33.29 | 47.20 | 278.64 | 0.7439 | -462.6 | -311.3 | |
| 6.52 | 13.92 | 4.79 | 10.22 | 1.89 | 33.05 | 46.96 | 278.19 | 0.7404 | -776.5 | -572.5 | |
| 3.88 | -3.00 | 2.84 | -3.00 | 2.09 | 32.93 | 46.84 | 278.49 | 0.7394 | -795.4 | 999999 | |
| 0.00 | 1.41 | 0.00 | 1.03 | 2.27 | 32.85 | 46.76 | 278.75 | 0.7388 | -563.0 | -529.6 | |
| 0.00 | 1.15 | 0.00 | 0.83 | 0.59 | 32.71 | 46.62 | 276.52 | 0.7339 | -450.0 | -417.5 | |
| 1.06 | 16.83 | 0.76 | 11.99 | 1.93 | 31.62 | 45.53 | 278.59 | 0.7236 | -710.4 | -640.0 | |
| 5.90 | -7.00 | 4.20 | -7.00 | 1.67 | 31.44 | 45.35 | 278.29 | 0.7209 | -839.0 | 999999 | |
| 3.00 | -7.00 | 2.13 | -7.00 | 1.88 | 31.40 | 45.31 | 278.58 | 0.7209 | -914.1 | 999999 | |
| 0.62 | 1.67 | 0.44 | 1.19 | 2.10 | 31.11 | 45.02 | 278.96 | 0.7179 | -724.0 | -626.4 | |
| 0.00 | 1.06 | 0.00 | 0.75 | 1.97 | 30.93 | 44.84 | 278.82 | 0.7155 | -825.0 | -672.7 | |
| 0.00 | 3.35 | 0.00 | 2.37 | 2.36 | 30.86 | 44.77 | 279.38 | 0.7156 | -649.0 | -566.4 | |
| 0.00 | 0.79 | 0.00 | 0.56 | 2.60 | 30.83 | 44.74 | 279.71 | 0.7158 | -654.0 | -493.8 | |
| 0.00 | 1.06 | 0.00 | 0.74 | 1.28 | 30.66 | 44.57 | 277.94 | 0.7107 | -741.0 | -543.2 | |
| 0.00 | 0.88 | 0.00 | 0.61 | 1.35 | 29.90 | 43.81 | 278.22 | 0.7016 | 462.0 | 390.0 | |
| 0.00 | 0.97 | 0.00 | 0.67 | 1.36 | 29.65 | 43.56 | 278.30 | 0.6986 | 536.0 | 491.9 | |
| 0.00 | 0.62 | 0.00 | 0.43 | 2.88 | 29.71 | 43.62 | 280.42 | 0.7029 | 483.0 | 363.0 | |
| 0.00 | 2.20 | 0.00 | 1.51 | 2.93 | 28.80 | 42.71 | 280.76 | 0.6919 | 628.0 | 486.2 | |
| 0.00 | 0.62 | 0.00 | 0.42 | 2.89 | 28.59 | 42.51 | 280.76 | 0.6892 | 334.0 | 347.6 | |
| 0.00 | 0.88 | 0.00 | 0.60 | 1.97 | 28.52 | 42.43 | 279.48 | 0.6859 | 602.0 | 466.6 | |
| 0.00 | 1.06 | 0.00 | 0.72 | 3.52 | 28.47 | 42.38 | 281.70 | 0.6893 | -426.0 | -446.8 | |
| 0.00 | 1.32 | 0.00 | 0.90 | 2.72 | 28.42 | 42.33 | 280.58 | 0.6867 | 294.0 | 288.5 | |
| 0.00 | 1.15 | 0.00 | 0.78 | 4.18 | 28.43 | 42.34 | 282.66 | 0.6907 | -643.0 | -531.5 | |
| 1.15 | 67.41 | 0.78 | 45.33 | 2.98 | 28.11 | 42.02 | 281.04 | 0.6834 | 611.6 | -30.6 | |
| 0.00 | 1.85 | 0.00 | 1.25 | 2.61 | 28.09 | 42.00 | 280.52 | 0.6822 | 683.0 | 572.7 | |
| 8.72 | -24.00 | 5.88 | -24.00 | 3.08 | 27.87 | 41.78 | 281.26 | 0.6807 | 770.1 | 999999 | |
| 11.81 | -24.00 | 7.91 | -24.00 | 2.90 | 27.46 | 41.37 | 281.13 | 0.6751 | 1009.9 | 999999 | |
| 0.00 | 0.88 | 0.00 | 0.58 | 2.41 | 26.60 | 40.51 | 280.69 | 0.6628 | -578.0 | -400.9 | |
| 0.00 | 0.70 | 0.00 | 0.46 | 7.60 | 23.67 | 37.58 | 289.56 | 0.6439 | 496.0 | 408.8 | |
| 0.00 | 3.44 | 0.00 | 1.97 | 8.17 | 12.63 | 26.54 | 298.02 | 0.5031 | 700.0 | 563.9 | |
| 0.00 | 2.47 | 0.00 | 1.41 | 7.98 | 12.48 | 26.39 | 297.81 | 0.4998 | 852.0 | 655.7 | |
| 0.00 | 0.88 | 0.00 | 0.50 | 7.66 | 12.26 | 26.17 | 297.44 | 0.4945 | 799.0 | 700.1 | |
| 0.00 | 1.06 | 0.00 | 0.60 | 7.47 | 12.21 | 26.12 | 297.15 | 0.4926 | 830.0 | 661.2 | |
| 0.00 | 1.41 | 0.00 | 0.80 | 7.43 | 11.94 | 25.85 | 297.32 | 0.4886 | 796.0 | 700.8 | |
| 0.00 | 1.59 | 0.00 | 0.89 | 6.25 | 11.60 | 25.51 | 295.41 | 0.4759 | 848.0 | 701.9 | |
| 0.00 | 3.44 | 0.00 | 1.95 | 8.73 | 11.36 | 25.27 | 300.23 | 0.4903 | 142.0 | 269.5 | |
| 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. | |