SDO HMI 2014-03-27 19:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.98 | 294.82 | 25.49 | 153.41 | 9.94 | 144.85 | 5.39 | 342.26 | 0.3066 | -274.2 | -267.7 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.87 | 0.00 | 0.45 | 5.72 | 149.42 | 9.96 | 321.24 | 0.2762 | -787.0 | -609.7 | |
| 0.00 | 0.70 | 0.00 | 0.37 | 10.29 | 149.20 | 9.74 | 330.28 | 0.3374 | -706.0 | -585.0 | |
| 32.19 | 179.30 | 16.75 | 93.32 | 9.62 | 146.51 | 7.05 | 336.71 | 0.3076 | -1336.2 | -434.6 | |
| 0.00 | 1.40 | 0.00 | 0.73 | 10.97 | 146.36 | 6.90 | 338.77 | 0.3273 | 123.0 | 73.9 | |
| 0.00 | 1.84 | 0.00 | 0.96 | 11.06 | 145.90 | 6.44 | 340.16 | 0.3260 | 833.0 | 638.3 | |
| 0.00 | 1.05 | 0.00 | 0.55 | 11.21 | 145.91 | 6.45 | 340.32 | 0.3285 | 747.0 | 543.2 | |
| 0.00 | 2.71 | 0.00 | 1.42 | 10.93 | 145.53 | 6.07 | 341.09 | 0.3220 | -695.0 | -505.5 | |
| 0.70 | 32.80 | 0.37 | 17.10 | 10.83 | 145.16 | 5.70 | 342.07 | 0.3185 | -867.9 | -780.4 | |
| 4.90 | -8.00 | 2.55 | -8.00 | 10.42 | 144.94 | 5.48 | 342.33 | 0.3109 | -1126.0 | 999999 | |
| 0.00 | 0.87 | 0.00 | 0.45 | 8.14 | 144.66 | 5.20 | 340.74 | 0.2733 | -861.0 | -689.3 | |
| 0.00 | 0.52 | 0.00 | 0.27 | 10.66 | 144.46 | 5.00 | 344.02 | 0.3125 | -769.0 | -570.3 | |
| 0.00 | 0.35 | 0.00 | 0.18 | 8.26 | 144.39 | 4.93 | 341.81 | 0.2737 | -671.0 | -521.2 | |
| 0.00 | 1.75 | 0.00 | 0.91 | 11.01 | 144.40 | 4.94 | 344.49 | 0.3178 | -815.0 | -610.0 | |
| 0.44 | 5.60 | 0.23 | 2.92 | 10.63 | 144.24 | 4.78 | 344.65 | 0.3110 | -1116.2 | -877.5 | |
| 0.00 | 1.75 | 0.00 | 0.90 | 7.73 | 143.99 | 4.53 | 342.62 | 0.2632 | -769.0 | -655.7 | |
| 0.00 | 1.31 | 0.00 | 0.69 | 11.76 | 143.92 | 4.47 | 346.49 | 0.3279 | -809.0 | -661.9 | |
| 0.00 | 1.66 | 0.00 | 0.86 | 9.72 | 143.74 | 4.28 | 345.44 | 0.2942 | -968.0 | -862.3 | |
| 0.61 | 3.67 | 0.32 | 1.91 | 10.34 | 143.66 | 4.20 | 346.23 | 0.3039 | -1071.1 | -865.7 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 10.34 | 142.74 | 3.29 | 349.14 | 0.3006 | -926.0 | -652.5 | |
| 0.87 | 4.29 | 0.45 | 2.21 | 9.58 | 141.98 | 2.52 | 351.25 | 0.2860 | 1053.1 | 772.6 | |
| 0.00 | 1.49 | 0.00 | 0.77 | 9.74 | 141.40 | 1.94 | 353.29 | 0.2873 | 975.0 | 747.5 | |
| 0.00 | 2.36 | 0.00 | 1.23 | 10.99 | 140.65 | 1.19 | 356.17 | 0.3070 | 911.0 | 735.8 | |
| 0.00 | 2.97 | 0.00 | 1.55 | 10.96 | 139.98 | 0.52 | 358.32 | 0.3059 | 382.0 | 306.4 | |
| 0.00 | 2.80 | 0.00 | 1.44 | 9.33 | 139.94 | 0.49 | 358.27 | 0.2786 | 909.0 | 767.3 | |
| 0.00 | 1.66 | 0.00 | 0.86 | 8.99 | 139.91 | 0.45 | 358.35 | 0.2729 | 1009.0 | 863.6 | |
| 0.00 | 2.36 | 0.00 | 1.22 | 9.46 | 139.73 | 0.27 | 359.03 | 0.2806 | 736.0 | 649.1 | |
| 0.00 | 1.92 | 0.00 | 1.00 | 10.33 | 139.52 | 0.06 | 359.79 | 0.2953 | 928.0 | 811.5 | |
| 8.75 | 12.07 | 4.55 | 6.28 | 10.96 | 139.09 | -0.36 | 1.17 | 0.3058 | 1003.9 | 698.9 | |
| 0.00 | 2.45 | 0.00 | 1.28 | 12.28 | 139.06 | -0.39 | 1.18 | 0.3279 | 706.0 | 718.1 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 9.83 | 139.03 | -0.42 | 1.46 | 0.2870 | 912.0 | 781.7 | |
| 0.52 | 4.11 | 0.27 | 2.13 | 10.46 | 138.97 | -0.48 | 1.61 | 0.2975 | 1062.2 | 900.8 | |
| 0.00 | 0.96 | 0.00 | 0.50 | 9.18 | 138.97 | -0.48 | 1.74 | 0.2760 | 754.0 | 673.1 | |
| 0.00 | 2.36 | 0.00 | 1.22 | 10.08 | 138.85 | -0.61 | 2.06 | 0.2913 | 806.0 | 750.3 | |
| 0.00 | 1.40 | 0.00 | 0.73 | 10.83 | 138.76 | -0.70 | 2.27 | 0.3039 | 1024.0 | 928.8 | |
| 0.00 | 1.05 | 0.00 | 0.54 | 9.61 | 138.70 | -0.76 | 2.65 | 0.2835 | 854.0 | 660.3 | |
| 0.00 | 4.29 | 0.00 | 2.23 | 10.71 | 138.55 | -0.91 | 2.98 | 0.3020 | 829.0 | 793.0 | |
| 0.00 | 6.21 | 0.00 | 3.23 | 11.05 | 138.36 | -1.09 | 3.50 | 0.3079 | 813.0 | 714.2 | |
| 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. | |