| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 99.45 | 436.37 | 91.28 | 401.12 | -13.71 | 120.49 | -54.83 | 109.34 | 0.8431 | 308.4 | 175.9 | |
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back to the solar disc SDO HMI 2011-11-02 23:58:59 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.03 | 237.64 | 8.54 | 205.25 | -14.75 | 123.87 | -51.45 | 111.53 | 0.8152 | 1001.2 | 301.6 | |
| 9.25 | -1.00 | 8.03 | -1.00 | -15.29 | 123.19 | -52.13 | 111.94 | 0.8232 | 593.4 | 999999 | |
| 2.85 | -1.00 | 2.49 | -1.00 | -15.55 | 122.99 | -52.33 | 112.18 | 0.8257 | 355.9 | 999999 | |
| 21.71 | -1.00 | 18.77 | -1.00 | -14.79 | 123.16 | -52.16 | 111.34 | 0.8220 | 720.3 | 999999 | |
| 8.56 | -1.00 | 7.45 | -1.00 | -14.47 | 122.81 | -52.51 | 110.85 | 0.8243 | 595.4 | 999999 | |
| 1.47 | -1.00 | 1.29 | -1.00 | -14.83 | 122.43 | -52.89 | 111.16 | 0.8288 | 210.5 | 999999 | |
| 0.00 | 0.69 | 0.00 | 0.62 | -15.39 | 121.61 | -53.71 | 111.54 | 0.8377 | 137.0 | 66.8 | |
| 0.00 | 0.61 | 0.00 | 0.55 | -14.34 | 121.36 | -53.96 | 110.25 | 0.8372 | 384.0 | 271.3 | |
| 0.69 | 1.90 | 0.62 | 1.72 | -14.13 | 121.22 | -54.10 | 109.97 | 0.8379 | 399.6 | 190.4 | |
| 0.00 | 1.21 | 0.00 | 1.11 | -14.83 | 120.92 | -54.41 | 110.69 | 0.8424 | 204.0 | 154.2 | |
| 3.55 | 5.88 | 3.21 | 5.33 | -13.68 | 120.96 | -54.36 | 109.37 | 0.8392 | 451.0 | 175.1 | |
| 0.00 | 0.78 | 0.00 | 0.73 | -13.51 | 119.73 | -55.59 | 108.83 | 0.8497 | -527.0 | -457.0 | |
| 1.38 | 7.00 | 1.33 | 6.75 | -14.61 | 118.99 | -56.34 | 109.88 | 0.8585 | -663.8 | -578.0 | |
| 0.52 | 4.67 | 0.49 | 4.42 | -13.32 | 119.30 | -56.02 | 108.49 | 0.8529 | -806.0 | -630.4 | |
| 2.33 | -13.00 | 2.26 | -13.00 | -14.60 | 118.71 | -56.61 | 109.79 | 0.8608 | -697.4 | 999999 | |
| 1.04 | -14.00 | 0.98 | -14.00 | -13.51 | 119.12 | -56.20 | 108.67 | 0.8549 | -620.1 | 999999 | |
| 1.12 | 1.56 | 1.07 | 1.48 | -13.31 | 118.92 | -56.40 | 108.38 | 0.8562 | -527.8 | -470.4 | |
| 0.00 | 0.61 | 0.00 | 0.58 | -13.27 | 118.60 | -56.72 | 108.25 | 0.8589 | -315.0 | -312.3 | |
| 3.81 | 5.45 | 3.84 | 5.49 | -15.37 | 117.41 | -57.91 | 110.30 | 0.8730 | -594.9 | -598.0 | |
| 0.00 | 1.82 | 0.00 | 1.81 | -14.85 | 117.63 | -57.69 | 109.78 | 0.8702 | -646.0 | -548.1 | |
| 2.59 | 32.60 | 2.62 | 33.51 | -15.03 | 117.26 | -58.06 | 109.89 | 0.8735 | -643.3 | -146.0 | |
| 4.24 | -21.00 | 4.32 | -21.00 | -15.24 | 117.00 | -58.32 | 110.04 | 0.8760 | -299.8 | 999999 | |
| 0.35 | 1.21 | 0.38 | 1.34 | -18.08 | 115.13 | -60.19 | 112.66 | 0.8957 | -470.5 | -428.8 | |
| 4.24 | 12.11 | 4.28 | 12.22 | -13.96 | 117.01 | -58.31 | 108.62 | 0.8734 | -650.7 | -400.0 | |
| 8.47 | 111.30 | 8.16 | 108.29 | -10.90 | 117.98 | -57.34 | 105.40 | 0.8596 | 950.5 | 210.8 | |
| 0.00 | 0.69 | 0.00 | 0.73 | -15.96 | 116.00 | -59.32 | 110.58 | 0.8852 | 491.0 | 441.6 | |
| 0.00 | 0.43 | 0.00 | 0.46 | -15.64 | 115.73 | -59.59 | 110.15 | 0.8866 | 238.0 | 239.6 | |
| 0.00 | 1.04 | 0.00 | 1.07 | -14.41 | 116.29 | -59.03 | 108.94 | 0.8800 | -114.0 | -58.8 | |
| 9.43 | -25.00 | 9.23 | -25.00 | -10.94 | 117.40 | -57.92 | 105.31 | 0.8646 | 496.3 | 999999 | |
| 0.00 | 0.43 | 0.00 | 0.46 | -14.88 | 115.77 | -59.55 | 109.33 | 0.8849 | -477.0 | -392.8 | |
| 0.00 | 1.64 | 0.00 | 1.83 | -15.64 | 114.21 | -61.11 | 109.78 | 0.8979 | -601.0 | -518.5 | |
| 0.00 | 0.78 | 0.00 | 0.80 | -10.92 | 115.88 | -59.44 | 104.95 | 0.8771 | 391.0 | 280.1 | |
| 0.00 | 0.43 | 0.00 | 0.44 | -10.26 | 116.03 | -59.30 | 104.24 | 0.8749 | 493.0 | 444.4 | |
| 0.00 | 0.26 | 0.00 | 0.29 | -14.34 | 113.63 | -61.69 | 108.23 | 0.8999 | -374.0 | -417.0 | |
| 1.82 | 3.63 | 1.92 | 3.84 | -10.26 | 114.69 | -60.63 | 103.96 | 0.8856 | 452.2 | 434.6 | |
| 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. | |