SDO HMI 2014-01-06 23:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 161.27 | 750.85 | 83.48 | 388.93 | 9.01 | 99.89 | -11.11 | 40.51 | 0.2924 | 259.0 | 89.1 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.57 | 73.39 | 6.41 | 37.41 | 8.62 | 105.08 | -5.92 | 25.61 | 0.2371 | -1254.6 | -444.1 | |
| 11.30 | -1.00 | 5.76 | -1.00 | 8.45 | 104.64 | -6.37 | 27.61 | 0.2378 | -1203.3 | 999999 | |
| 0.00 | 1.95 | 0.00 | 1.00 | 8.36 | 104.16 | -6.85 | 29.53 | 0.2404 | -1061.0 | -867.0 | |
| 3.48 | 5.35 | 1.78 | 2.73 | 8.63 | 104.03 | -6.97 | 29.41 | 0.2455 | -1062.9 | -742.1 | |
| 0.00 | 4.93 | 0.00 | 2.51 | 7.64 | 103.84 | -7.16 | 32.25 | 0.2327 | -1224.0 | -942.0 | |
| 0.76 | 2.04 | 0.39 | 1.04 | 8.67 | 103.79 | -7.21 | 30.18 | 0.2480 | -955.0 | -745.9 | |
| 0.00 | 1.10 | 0.00 | 0.57 | 10.21 | 103.70 | -7.30 | 27.57 | 0.2715 | -771.0 | -528.9 | |
| 0.00 | 4.50 | 0.00 | 2.29 | 7.73 | 103.57 | -7.44 | 33.01 | 0.2365 | -846.0 | -785.5 | |
| 0.00 | 0.93 | 0.00 | 0.48 | 8.79 | 103.55 | -7.45 | 30.76 | 0.2519 | -593.0 | -474.4 | |
| 0.93 | 97.85 | 0.48 | 50.34 | 9.04 | 102.94 | -8.06 | 32.24 | 0.2608 | -947.5 | -664.6 | |
| 0.00 | 8.49 | 0.00 | 4.34 | 7.75 | 102.34 | -8.67 | 37.10 | 0.2487 | -599.0 | -798.4 | |
| 2.63 | -10.00 | 1.35 | -10.00 | 9.35 | 102.24 | -8.76 | 33.78 | 0.2716 | -1011.4 | 999999 | |
| 1.95 | -10.00 | 1.00 | -10.00 | 8.96 | 102.04 | -8.97 | 35.22 | 0.2681 | -1029.7 | 999999 | |
| 1.61 | 6.37 | 0.83 | 3.26 | 8.08 | 101.94 | -9.07 | 37.52 | 0.2573 | -1142.1 | -719.1 | |
| 0.00 | 1.87 | 0.00 | 0.96 | 8.78 | 101.83 | -9.17 | 36.24 | 0.2677 | -912.0 | -674.0 | |
| 16.05 | -10.00 | 8.27 | -10.00 | 9.38 | 101.70 | -9.31 | 35.32 | 0.2773 | -1006.3 | 999999 | |
| 0.00 | 1.19 | 0.00 | 0.61 | 8.60 | 101.68 | -9.32 | 37.08 | 0.2668 | -868.0 | -805.1 | |
| 0.00 | 1.10 | 0.00 | 0.57 | 11.30 | 101.55 | -9.46 | 32.01 | 0.3052 | -796.0 | -545.9 | |
| 2.80 | 56.74 | 1.44 | 29.18 | 8.18 | 101.24 | -9.76 | 39.35 | 0.2659 | -1080.5 | -379.1 | |
| 6.46 | -19.00 | 3.32 | -19.00 | 8.55 | 101.08 | -9.92 | 38.94 | 0.2723 | -1027.9 | 999999 | |
| 0.00 | 1.36 | 0.00 | 0.70 | 9.18 | 101.03 | -9.97 | 37.63 | 0.2812 | -194.0 | -269.4 | |
| 0.00 | 0.68 | 0.00 | 0.35 | 7.55 | 100.92 | -10.08 | 41.82 | 0.2614 | 683.0 | 566.0 | |
| 1.36 | -19.00 | 0.70 | -19.00 | 8.40 | 100.78 | -10.22 | 40.12 | 0.2736 | -593.2 | 999999 | |
| 1.95 | -19.00 | 1.00 | -19.00 | 7.86 | 100.77 | -10.24 | 41.50 | 0.2670 | 830.0 | 999999 | |
| 0.00 | 1.27 | 0.00 | 0.66 | 9.46 | 100.24 | -10.77 | 39.15 | 0.2932 | 811.0 | 484.9 | |
| 0.00 | 1.10 | 0.00 | 0.57 | 9.22 | 100.03 | -10.97 | 40.21 | 0.2923 | 803.0 | 632.4 | |
| 0.00 | 0.68 | 0.00 | 0.35 | 8.44 | 99.90 | -11.10 | 42.36 | 0.2839 | 773.0 | 605.0 | |
| 3.57 | 476.18 | 1.85 | 248.08 | 9.29 | 99.39 | -11.61 | 41.67 | 0.3002 | 997.9 | 433.1 | |
| 0.76 | -28.00 | 0.40 | -28.00 | 9.66 | 99.04 | -11.96 | 41.69 | 0.3086 | 1202.7 | 999999 | |
| 2.04 | -28.00 | 1.06 | -28.00 | 9.84 | 99.00 | -12.00 | 41.38 | 0.3113 | 974.3 | 999999 | |
| 4.25 | -28.00 | 2.21 | -28.00 | 9.09 | 99.00 | -12.00 | 43.07 | 0.3021 | 1123.8 | 999999 | |
| 6.71 | -28.00 | 3.48 | -28.00 | 8.63 | 98.98 | -12.02 | 44.17 | 0.2968 | 1100.1 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.45 | 11.22 | 98.61 | -12.39 | 39.46 | 0.3326 | 816.0 | 665.5 | |
| 0.00 | 0.93 | 0.00 | 0.48 | 7.89 | 98.67 | -12.33 | 46.74 | 0.2918 | -444.0 | -307.0 | |
| 3.48 | -28.00 | 1.82 | -28.00 | 9.73 | 98.37 | -12.64 | 43.10 | 0.3170 | 912.1 | 999999 | |
| 75.34 | -28.00 | 39.26 | -28.00 | 9.13 | 98.17 | -12.83 | 44.88 | 0.3121 | 1371.5 | 999999 | |
| 1.27 | -28.00 | 0.67 | -28.00 | 9.89 | 98.15 | -12.86 | 43.25 | 0.3214 | 594.1 | 999999 | |
| 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. | |