| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 111.46 | 479.03 | 62.62 | 270.51 | 16.56 | 64.72 | -26.02 | 61.13 | 0.4815 | -656.9 | -336.5 | |
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back to the solar disc SDO HMI 2011-11-09 09:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.12 | 0.00 | 0.62 | 14.82 | 65.85 | -24.88 | 63.65 | 0.4558 | -241.0 | -223.0 | |
| 79.40 | 410.03 | 44.46 | 229.79 | 16.21 | 65.57 | -25.17 | 61.11 | 0.4683 | -1169.2 | -404.4 | |
| 0.00 | 1.98 | 0.00 | 1.14 | 20.22 | 64.76 | -25.97 | 54.49 | 0.5069 | -808.0 | -591.7 | |
| 2.24 | 2.85 | 1.27 | 1.61 | 18.01 | 65.10 | -25.64 | 58.12 | 0.4865 | -745.1 | -740.4 | |
| 1.90 | -2.00 | 1.06 | -2.00 | 15.60 | 65.38 | -25.36 | 62.48 | 0.4671 | -591.5 | 999999 | |
| 1.03 | 8.71 | 0.59 | 4.93 | 17.51 | 64.93 | -25.80 | 59.19 | 0.4853 | -685.1 | -644.3 | |
| 6.21 | -2.00 | 3.50 | -2.00 | 16.84 | 65.00 | -25.74 | 60.39 | 0.4800 | -654.5 | 999999 | |
| 3.62 | 4.83 | 2.06 | 2.74 | 17.96 | 64.62 | -26.12 | 58.62 | 0.4925 | -776.4 | -674.2 | |
| 0.00 | 0.78 | 0.00 | 0.46 | 23.11 | 63.58 | -27.16 | 50.88 | 0.5433 | -785.0 | -606.8 | |
| 9.22 | -2.00 | 5.21 | -2.00 | 16.37 | 64.69 | -26.05 | 61.54 | 0.4812 | -758.1 | 999999 | |
| 5.35 | -2.00 | 3.02 | -2.00 | 15.97 | 64.47 | -26.27 | 62.48 | 0.4817 | -783.1 | 999999 | |
| 0.00 | 5.86 | 0.00 | 3.32 | 15.71 | 63.88 | -26.85 | 63.42 | 0.4882 | -484.0 | -385.8 | |
| 0.43 | 5.52 | 0.25 | 3.15 | 17.01 | 63.30 | -27.43 | 61.44 | 0.5036 | -649.2 | -629.4 | |
| 1.72 | 1.90 | 0.99 | 1.08 | 16.58 | 63.34 | -27.40 | 62.20 | 0.5006 | -657.4 | -487.0 | |
| 0.00 | 4.31 | 0.00 | 2.46 | 16.04 | 63.42 | -27.31 | 63.15 | 0.4963 | -652.0 | -436.2 | |
| 0.00 | 1.12 | 0.00 | 0.68 | 24.55 | 61.54 | -29.20 | 50.49 | 0.5773 | -698.0 | -607.7 | |
| 0.00 | 0.95 | 0.00 | 0.55 | 19.13 | 61.98 | -28.76 | 58.72 | 0.5340 | -665.0 | -586.7 | |
| 0.00 | 1.64 | 0.00 | 0.94 | 15.80 | 62.48 | -28.26 | 64.26 | 0.5078 | 780.0 | 732.8 | |
| 0.00 | 1.12 | 0.00 | 0.65 | 17.42 | 61.43 | -29.30 | 62.07 | 0.5307 | 906.0 | 775.7 | |
| 0.00 | 1.64 | 0.00 | 0.96 | 16.24 | 60.88 | -29.85 | 64.50 | 0.5316 | -698.0 | -521.5 | |
| 0.00 | 1.47 | 0.00 | 0.87 | 16.43 | 59.08 | -31.65 | 65.24 | 0.5564 | -604.0 | -312.4 | |
| 0.34 | 1.21 | 0.21 | 0.73 | 18.77 | 58.43 | -32.30 | 61.73 | 0.5766 | 835.5 | 723.3 | |
| 0.00 | 2.50 | 0.00 | 1.51 | 18.46 | 58.43 | -32.31 | 62.24 | 0.5751 | 872.0 | 797.5 | |
| 0.00 | 1.38 | 0.00 | 0.85 | 20.61 | 57.78 | -32.95 | 59.23 | 0.5947 | 789.0 | 701.8 | |
| 0.00 | 0.95 | 0.00 | 0.58 | 20.18 | 57.81 | -32.92 | 59.88 | 0.5919 | 731.0 | 554.2 | |
| 0.00 | 1.98 | 0.00 | 1.22 | 19.42 | 57.54 | -33.19 | 61.24 | 0.5912 | 516.0 | 419.2 | |
| 0.00 | 1.64 | 0.00 | 1.01 | 19.67 | 57.37 | -33.36 | 60.96 | 0.5946 | 705.0 | 678.3 | |
| 0.00 | 1.38 | 0.00 | 0.85 | 20.25 | 57.15 | -33.58 | 60.18 | 0.6004 | 695.0 | 615.9 | |
| 0.00 | 1.21 | 0.00 | 0.75 | 19.43 | 56.82 | -33.92 | 61.65 | 0.6002 | 783.0 | 571.0 | |
| 0.00 | 4.22 | 0.00 | 2.68 | 20.42 | 54.87 | -35.87 | 61.22 | 0.6287 | 774.0 | 707.9 | |
| 0.00 | 0.52 | 0.00 | 0.33 | 20.76 | 54.74 | -36.00 | 60.79 | 0.6320 | 630.0 | 556.5 | |
| 0.00 | 0.95 | 0.00 | 0.61 | 20.52 | 53.97 | -36.76 | 61.55 | 0.6398 | 602.0 | 537.5 | |
| 0.00 | 0.52 | 0.00 | 0.34 | 21.78 | 53.44 | -37.29 | 59.99 | 0.6520 | 675.0 | 575.7 | |
| 0.00 | 2.24 | 0.00 | 1.45 | 20.69 | 53.65 | -37.09 | 61.46 | 0.6445 | 775.0 | 591.5 | |
| 0.00 | 1.03 | 0.00 | 0.68 | 21.82 | 52.86 | -37.87 | 60.23 | 0.6589 | 525.0 | 458.9 | |
| 0.00 | 1.47 | 0.00 | 0.97 | 21.29 | 52.01 | -38.72 | 61.40 | 0.6662 | 618.0 | 562.8 | |
| 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. | |