| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 56.69 | 232.67 | 35.66 | 146.63 | 19.12 | 172.70 | 33.95 | 301.23 | 0.6187 | -221.4 | -96.7 | |
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back to the solar disc SDO HMI 2011-12-03 01:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 25.96 | 142.43 | 16.67 | 91.50 | 18.76 | 174.60 | 35.85 | 299.41 | 0.6388 | -963.4 | -274.4 | |
| 4.87 | -1.00 | 3.11 | -1.00 | 19.05 | 174.09 | 35.34 | 300.12 | 0.6344 | -950.1 | 999999 | |
| 2.56 | -1.00 | 1.63 | -1.00 | 18.55 | 173.93 | 35.18 | 299.49 | 0.6298 | -916.6 | 999999 | |
| 0.00 | 0.94 | 0.00 | 0.60 | 19.99 | 173.67 | 34.92 | 301.73 | 0.6348 | -236.0 | -266.4 | |
| 1.79 | 3.84 | 1.14 | 2.44 | 19.30 | 173.35 | 34.60 | 300.95 | 0.6272 | -729.3 | -637.6 | |
| 0.00 | 6.23 | 0.00 | 3.91 | 18.12 | 172.96 | 34.21 | 299.45 | 0.6159 | -688.0 | -717.0 | |
| 0.00 | 0.51 | 0.00 | 0.32 | 18.81 | 172.93 | 34.18 | 300.49 | 0.6194 | -624.0 | -491.0 | |
| 1.37 | 2.05 | 0.86 | 1.28 | 18.34 | 172.75 | 33.99 | 299.91 | 0.6146 | -836.9 | -790.0 | |
| 0.00 | 2.13 | 0.00 | 1.33 | 18.19 | 172.52 | 33.77 | 299.82 | 0.6110 | -936.0 | -769.3 | |
| 1.54 | 5.64 | 0.96 | 3.53 | 19.00 | 172.44 | 33.69 | 301.08 | 0.6147 | -726.4 | -720.7 | |
| 1.02 | -10.00 | 0.64 | -10.00 | 18.68 | 172.37 | 33.62 | 300.66 | 0.6121 | -809.3 | 999999 | |
| 0.00 | 1.20 | 0.00 | 0.76 | 21.07 | 172.34 | 33.59 | 304.15 | 0.6262 | -679.0 | -523.7 | |
| 0.00 | 1.37 | 0.00 | 0.83 | 18.26 | 170.39 | 31.64 | 301.37 | 0.5857 | 578.0 | 422.4 | |
| 0.00 | 1.02 | 0.00 | 0.63 | 18.98 | 170.32 | 31.57 | 302.52 | 0.5894 | 642.0 | 518.3 | |
| 0.00 | 0.60 | 0.00 | 0.36 | 18.98 | 170.03 | 31.27 | 302.74 | 0.5859 | 452.0 | 523.3 | |
| 1.54 | 13.32 | 0.93 | 8.06 | 18.79 | 169.70 | 30.94 | 302.70 | 0.5807 | 745.5 | 468.3 | |
| 0.00 | 1.20 | 0.00 | 0.72 | 18.98 | 169.37 | 30.62 | 303.24 | 0.5780 | 414.0 | 272.4 | |
| 2.39 | -16.00 | 1.44 | -16.00 | 18.67 | 169.24 | 30.48 | 302.86 | 0.5743 | -543.4 | 999999 | |
| 2.05 | 7.00 | 1.26 | 4.29 | 20.80 | 169.62 | 30.86 | 305.77 | 0.5934 | 702.0 | 569.6 | |
| 0.00 | 4.35 | 0.00 | 2.63 | 19.11 | 169.14 | 30.39 | 303.61 | 0.5762 | 71.0 | 48.3 | |
| 0.00 | 1.45 | 0.00 | 0.89 | 20.77 | 169.24 | 30.49 | 306.03 | 0.5889 | 768.0 | 658.4 | |
| 0.00 | 1.28 | 0.00 | 0.77 | 18.83 | 168.83 | 30.08 | 303.42 | 0.5706 | -592.0 | -451.6 | |
| 1.37 | 1.45 | 0.83 | 0.88 | 20.30 | 169.10 | 30.35 | 305.44 | 0.5839 | 749.4 | 770.0 | |
| 0.00 | 1.37 | 0.00 | 0.82 | 19.39 | 168.62 | 29.87 | 304.45 | 0.5719 | 577.0 | 360.3 | |
| 4.01 | 12.30 | 2.44 | 7.50 | 20.93 | 168.76 | 30.01 | 306.65 | 0.5845 | 767.9 | 701.7 | |
| 0.00 | 0.85 | 0.00 | 0.52 | 21.28 | 168.66 | 29.91 | 307.25 | 0.5859 | 509.0 | 387.5 | |
| 0.00 | 1.88 | 0.00 | 1.14 | 20.77 | 168.51 | 29.76 | 306.63 | 0.5805 | 692.0 | 735.5 | |
| 1.11 | 5.55 | 0.67 | 3.33 | 19.64 | 168.20 | 29.45 | 305.18 | 0.5687 | 712.6 | 549.2 | |
| 2.13 | -28.00 | 1.28 | -28.00 | 19.71 | 168.00 | 29.25 | 305.45 | 0.5668 | 690.9 | 999999 | |
| 2.13 | 4.10 | 1.29 | 2.48 | 20.87 | 168.20 | 29.45 | 307.03 | 0.5777 | 791.6 | 715.7 | |
| 0.85 | 0.94 | 0.51 | 0.56 | 20.15 | 167.22 | 28.47 | 306.79 | 0.5610 | 772.7 | 684.0 | |
| 0.00 | 1.02 | 0.00 | 0.61 | 20.31 | 166.90 | 28.15 | 307.32 | 0.5585 | 716.0 | 592.8 | |
| 0.00 | 3.67 | 0.00 | 2.18 | 20.37 | 166.55 | 27.80 | 307.73 | 0.5550 | 933.0 | 784.7 | |
| 0.00 | 1.02 | 0.00 | 0.61 | 20.59 | 166.35 | 27.59 | 308.25 | 0.5544 | 814.0 | 710.2 | |
| 0.00 | 0.85 | 0.00 | 0.50 | 20.00 | 165.38 | 26.63 | 308.25 | 0.5385 | 704.0 | 554.8 | |
| 0.00 | 1.11 | 0.00 | 0.65 | 20.48 | 164.10 | 25.35 | 310.27 | 0.5278 | 769.0 | 647.0 | |
| 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. | |