SDO HMI 2014-05-23 20:00:38 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.00 | 284.03 | 35.68 | 158.65 | -10.84 | 80.00 | -25.88 | 110.81 | 0.4595 | 18.2 | -105.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.71 | 0.00 | 0.90 | -6.47 | 86.01 | -19.87 | 104.15 | 0.3498 | 0.0 | 6.9 | |
| 2.52 | 81.68 | 1.35 | 43.71 | -9.91 | 85.30 | -20.58 | 112.72 | 0.3770 | 1420.9 | 497.6 | |
| 4.41 | -2.00 | 2.36 | -2.00 | -9.97 | 85.16 | -20.72 | 112.74 | 0.3794 | 1371.8 | 999999 | |
| 0.00 | 3.06 | 0.00 | 1.62 | -1.66 | 85.46 | -20.42 | 90.24 | 0.3503 | 22.0 | 11.7 | |
| 4.41 | -2.00 | 2.36 | -2.00 | -10.25 | 85.08 | -20.80 | 113.34 | 0.3823 | 994.6 | 999999 | |
| 3.15 | -2.00 | 1.69 | -2.00 | -9.79 | 85.11 | -20.77 | 112.24 | 0.3792 | 1237.9 | 999999 | |
| 6.39 | -2.00 | 3.43 | -2.00 | -10.03 | 84.89 | -20.99 | 112.64 | 0.3837 | 980.4 | 999999 | |
| 0.00 | 1.62 | 0.00 | 0.88 | -11.46 | 83.95 | -21.92 | 115.17 | 0.4060 | 890.0 | 691.6 | |
| 0.00 | 1.17 | 0.00 | 0.64 | -10.19 | 83.02 | -22.86 | 111.45 | 0.4125 | 868.0 | 698.2 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -10.55 | 82.45 | -23.43 | 111.84 | 0.4228 | 833.0 | 673.0 | |
| 0.00 | 1.08 | 0.00 | 0.59 | -10.92 | 82.39 | -23.49 | 112.61 | 0.4257 | 780.0 | 573.2 | |
| 0.45 | 4.23 | 0.25 | 2.33 | -11.50 | 82.03 | -23.85 | 113.59 | 0.4341 | 972.6 | 752.9 | |
| 0.27 | -12.00 | 0.15 | -12.00 | -11.56 | 81.93 | -23.95 | 113.64 | 0.4360 | 840.7 | 999999 | |
| 5.04 | 9.01 | 2.77 | 4.95 | -11.19 | 81.89 | -23.99 | 112.81 | 0.4344 | 1045.2 | 832.4 | |
| 0.00 | 1.26 | 0.00 | 0.69 | -10.48 | 81.72 | -24.16 | 111.13 | 0.4333 | 880.0 | 749.9 | |
| 1.71 | 3.06 | 0.94 | 1.69 | -11.22 | 81.58 | -24.29 | 112.63 | 0.4390 | 789.8 | 590.4 | |
| 0.00 | 1.80 | 0.00 | 0.99 | -10.51 | 81.27 | -24.61 | 110.87 | 0.4399 | 896.0 | 787.5 | |
| 1.53 | 3.87 | 0.85 | 2.16 | -9.47 | 79.76 | -26.12 | 107.69 | 0.4577 | 845.3 | 621.5 | |
| 0.00 | 1.17 | 0.00 | 0.66 | -13.88 | 79.26 | -26.62 | 116.23 | 0.4868 | 642.0 | 495.7 | |
| 5.31 | 11.71 | 2.97 | 6.55 | -10.64 | 79.45 | -26.43 | 109.94 | 0.4673 | -1003.7 | -369.0 | |
| 0.00 | 1.08 | 0.00 | 0.61 | -10.76 | 79.19 | -26.69 | 110.02 | 0.4715 | -738.0 | -565.4 | |
| 0.00 | 9.91 | 0.00 | 5.56 | -10.39 | 79.09 | -26.79 | 109.21 | 0.4714 | -171.0 | -325.4 | |
| 0.00 | 3.51 | 0.00 | 1.96 | -8.18 | 78.93 | -26.95 | 104.53 | 0.4653 | -838.0 | -607.1 | |
| 0.00 | 0.99 | 0.00 | 0.56 | -8.57 | 78.76 | -27.12 | 105.28 | 0.4691 | -566.0 | -457.2 | |
| 4.14 | 10.36 | 2.34 | 5.85 | -10.77 | 78.36 | -27.52 | 109.56 | 0.4837 | -965.8 | -726.3 | |
| 0.00 | 1.26 | 0.00 | 0.71 | -10.90 | 78.20 | -27.67 | 109.72 | 0.4864 | -173.0 | -438.0 | |
| 0.00 | 3.06 | 0.00 | 1.75 | -12.68 | 77.90 | -27.98 | 112.99 | 0.4992 | -655.0 | -657.1 | |
| 0.72 | 63.13 | 0.41 | 36.07 | -10.97 | 77.25 | -28.63 | 109.33 | 0.5005 | -879.6 | -603.3 | |
| 6.75 | -28.00 | 3.87 | -28.00 | -11.19 | 77.15 | -28.72 | 109.69 | 0.5027 | -965.6 | 999999 | |
| 0.99 | 60.79 | 0.57 | 35.21 | -12.23 | 76.86 | -29.02 | 111.50 | 0.5116 | -982.0 | -332.6 | |
| 2.43 | -30.00 | 1.40 | -30.00 | -12.42 | 76.66 | -29.22 | 111.72 | 0.5152 | -940.1 | 999999 | |
| 1.35 | -30.00 | 0.78 | -30.00 | -12.17 | 76.61 | -29.26 | 111.23 | 0.5147 | -1110.9 | 999999 | |
| 0.00 | 1.08 | 0.00 | 0.62 | -11.24 | 76.55 | -29.33 | 109.46 | 0.5116 | -516.0 | -471.2 | |
| 12.43 | -30.00 | 7.19 | -30.00 | -12.10 | 76.27 | -29.61 | 110.91 | 0.5193 | -998.1 | 999999 | |
| 0.00 | 1.35 | 0.00 | 0.80 | -13.10 | 74.80 | -31.08 | 111.90 | 0.5440 | -502.0 | -443.5 | |
| 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. | |