SDO HMI 2011-10-20 21:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 104.38 | 473.56 | 120.19 | 566.18 | 9.47 | 53.63 | 65.77 | 278.00 | 0.9084 | -77.6 | -99.9 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.48 | 305.86 | 2.01 | 399.22 | 7.76 | 56.96 | 69.10 | 276.21 | 0.9327 | 576.2 | -172.8 | |
| 4.70 | -1.00 | 6.32 | -1.00 | 7.42 | 56.67 | 68.81 | 275.83 | 0.9310 | -407.4 | 999999 | |
| 1.48 | -1.00 | 2.00 | -1.00 | 7.98 | 56.78 | 68.92 | 276.44 | 0.9315 | 204.9 | 999999 | |
| 3.66 | -1.00 | 4.87 | -1.00 | 7.92 | 56.51 | 68.65 | 276.36 | 0.9298 | -329.6 | 999999 | |
| 3.05 | -1.00 | 4.06 | -1.00 | 8.52 | 56.56 | 68.70 | 277.01 | 0.9300 | 121.0 | 999999 | |
| 30.21 | -1.00 | 39.15 | -1.00 | 8.51 | 55.90 | 68.04 | 276.97 | 0.9257 | -644.7 | 999999 | |
| 5.05 | -1.00 | 6.25 | -1.00 | 8.91 | 54.77 | 66.91 | 277.36 | 0.9180 | -689.0 | 999999 | |
| 0.00 | 2.26 | 0.00 | 2.74 | 8.21 | 54.21 | 66.35 | 276.57 | 0.9144 | -545.0 | -507.3 | |
| 3.48 | -1.00 | 4.24 | -1.00 | 9.37 | 54.40 | 66.54 | 277.85 | 0.9154 | -628.2 | 999999 | |
| 0.00 | 1.31 | 0.00 | 1.57 | 9.18 | 54.10 | 66.24 | 277.63 | 0.9133 | -629.0 | -508.2 | |
| 1.31 | -1.00 | 1.57 | -1.00 | 9.73 | 54.08 | 66.22 | 278.23 | 0.9131 | -801.1 | 999999 | |
| 1.04 | -1.00 | 1.26 | -1.00 | 9.91 | 54.08 | 66.22 | 278.43 | 0.9130 | -846.5 | 999999 | |
| 0.00 | 1.22 | 0.00 | 1.45 | 9.24 | 53.75 | 65.89 | 277.69 | 0.9108 | -629.0 | -622.1 | |
| 2.52 | 2.79 | 2.91 | 3.21 | 9.25 | 52.94 | 65.08 | 277.67 | 0.9050 | -596.6 | -526.7 | |
| 0.00 | 0.96 | 0.00 | 1.12 | 10.81 | 53.47 | 65.61 | 279.41 | 0.9086 | -521.0 | -447.9 | |
| 0.00 | 5.40 | 0.00 | 5.85 | 9.59 | 51.16 | 63.30 | 277.99 | 0.8914 | -132.0 | -172.9 | |
| 0.00 | 1.22 | 0.00 | 1.29 | 8.51 | 50.35 | 62.49 | 276.75 | 0.8852 | 399.0 | 324.1 | |
| 1.65 | 4.88 | 1.77 | 5.21 | 9.90 | 50.72 | 62.86 | 278.33 | 0.8879 | 143.6 | -22.3 | |
| 2.09 | 6.79 | 2.20 | 7.18 | 10.60 | 50.30 | 62.44 | 279.11 | 0.8845 | 287.0 | -54.2 | |
| 0.00 | 0.96 | 0.00 | 0.98 | 9.85 | 49.46 | 61.60 | 278.25 | 0.8777 | 328.0 | 193.5 | |
| 9.75 | 14.54 | 9.76 | 14.59 | 10.55 | 48.68 | 60.81 | 279.05 | 0.8711 | 398.9 | 9.6 | |
| 4.61 | 7.14 | 4.55 | 7.04 | 10.41 | 48.13 | 60.27 | 278.89 | 0.8665 | 539.1 | 340.4 | |
| 0.00 | 0.70 | 0.00 | 0.72 | 15.16 | 49.71 | 61.85 | 284.31 | 0.8802 | -339.0 | -386.8 | |
| 0.00 | 1.83 | 0.00 | 1.76 | 10.60 | 47.34 | 59.48 | 279.10 | 0.8596 | 439.0 | 303.6 | |
| 0.00 | 1.65 | 0.00 | 1.58 | 10.63 | 46.99 | 59.13 | 279.13 | 0.8565 | 630.0 | 552.7 | |
| 0.00 | 0.78 | 0.00 | 0.75 | 10.84 | 46.99 | 59.13 | 279.38 | 0.8566 | 611.0 | 569.7 | |
| 0.00 | 0.96 | 0.00 | 0.96 | 14.71 | 48.46 | 60.60 | 283.84 | 0.8698 | 182.0 | 125.2 | |
| 4.53 | 88.63 | 4.39 | 85.80 | 12.77 | 47.56 | 59.70 | 281.62 | 0.8617 | 550.7 | 153.3 | |
| 0.00 | 2.79 | 0.00 | 2.72 | 13.27 | 47.76 | 59.90 | 282.20 | 0.8636 | 507.0 | 366.5 | |
| 21.85 | -28.00 | 21.02 | -28.00 | 12.18 | 47.28 | 59.42 | 280.95 | 0.8592 | 707.3 | 999999 | |
| 1.31 | 1.65 | 1.27 | 1.61 | 13.04 | 47.61 | 59.75 | 281.93 | 0.8622 | 458.8 | 383.0 | |
| 0.00 | 0.78 | 0.00 | 0.74 | 10.76 | 46.79 | 58.93 | 279.29 | 0.8548 | 666.0 | 583.9 | |
| 0.00 | 0.70 | 0.00 | 0.68 | 13.57 | 47.76 | 59.90 | 282.55 | 0.8637 | 27.0 | 57.5 | |
| 0.26 | 10.97 | 0.26 | 10.80 | 13.99 | 47.88 | 60.02 | 283.03 | 0.8648 | -64.3 | 58.2 | |
| 0.35 | 4.09 | 0.33 | 3.93 | 13.31 | 47.23 | 59.37 | 282.27 | 0.8590 | 635.2 | 474.3 | |
| 0.00 | 0.87 | 0.00 | 0.87 | 19.41 | 48.21 | 60.35 | 289.26 | 0.8703 | 338.0 | 338.1 | |
| 0.00 | 1.83 | 0.00 | 1.81 | 19.82 | 47.82 | 59.96 | 289.77 | 0.8674 | 396.0 | 286.1 | |
| 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. | |