| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 98.02 | 465.52 | 54.83 | 259.58 | 15.16 | 231.78 | -23.94 | 58.85 | 0.4575 | -450.2 | -212.8 | |
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back to the solar disc SDO HMI 2011-11-24 04:58:57 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.05 | 33.24 | 5.96 | 17.90 | 13.27 | 235.30 | -20.42 | 59.39 | 0.3963 | -1094.9 | -513.4 | |
| 3.26 | 4.97 | 1.76 | 2.69 | 13.26 | 234.55 | -21.17 | 60.25 | 0.4066 | -896.8 | -531.5 | |
| 46.44 | 271.35 | 25.35 | 148.13 | 14.83 | 234.30 | -21.42 | 57.17 | 0.4220 | -1353.4 | -431.6 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 17.74 | 233.93 | -21.79 | 51.94 | 0.4510 | -802.0 | -605.8 | |
| 0.00 | 1.03 | 0.00 | 0.56 | 12.71 | 234.02 | -21.71 | 62.03 | 0.4103 | -846.0 | -655.2 | |
| 1.29 | -3.00 | 0.70 | -3.00 | 14.79 | 233.65 | -22.08 | 57.98 | 0.4305 | -830.7 | 999999 | |
| 0.00 | 1.46 | 0.00 | 0.79 | 12.92 | 233.64 | -22.09 | 61.95 | 0.4171 | -753.0 | -555.5 | |
| 0.00 | 0.26 | 0.00 | 0.14 | 14.87 | 232.54 | -23.18 | 58.97 | 0.4459 | -642.0 | -518.0 | |
| 0.00 | 1.03 | 0.00 | 0.58 | 17.10 | 232.06 | -23.66 | 55.20 | 0.4691 | -827.0 | -617.4 | |
| 0.00 | 1.20 | 0.00 | 0.67 | 17.37 | 231.72 | -24.00 | 55.06 | 0.4756 | -716.0 | -552.9 | |
| 0.00 | 0.86 | 0.00 | 0.47 | 13.77 | 231.96 | -23.76 | 61.75 | 0.4461 | -685.0 | -566.9 | |
| 0.00 | 0.86 | 0.00 | 0.48 | 17.83 | 231.42 | -24.31 | 54.55 | 0.4830 | -796.0 | -657.6 | |
| 0.00 | 0.86 | 0.00 | 0.48 | 17.71 | 231.33 | -24.39 | 54.86 | 0.4831 | -692.0 | -557.3 | |
| 0.00 | 0.77 | 0.00 | 0.44 | 17.52 | 231.32 | -24.40 | 55.20 | 0.4817 | -475.0 | -461.1 | |
| 0.00 | 1.54 | 0.00 | 0.87 | 16.14 | 231.18 | -24.55 | 57.88 | 0.4732 | -952.0 | -774.8 | |
| 0.00 | 1.71 | 0.00 | 0.96 | 14.61 | 231.13 | -24.59 | 60.84 | 0.4631 | -959.0 | -720.6 | |
| 0.00 | 1.80 | 0.00 | 1.02 | 16.71 | 230.72 | -25.00 | 57.25 | 0.4833 | -674.0 | -584.3 | |
| 0.00 | 0.69 | 0.00 | 0.38 | 14.88 | 230.93 | -24.79 | 60.49 | 0.4676 | -626.0 | -478.5 | |
| 4.28 | 8.40 | 2.41 | 4.73 | 15.76 | 230.68 | -25.04 | 59.04 | 0.4770 | -839.9 | -759.1 | |
| 1.03 | 10.62 | 0.59 | 6.13 | 16.71 | 228.27 | -27.45 | 59.42 | 0.5149 | -887.7 | -688.1 | |
| 0.00 | 1.88 | 0.00 | 1.09 | 16.34 | 227.63 | -28.09 | 60.59 | 0.5208 | 742.0 | 600.2 | |
| 0.00 | 3.34 | 0.00 | 1.95 | 17.25 | 227.10 | -28.63 | 59.43 | 0.5335 | -699.0 | -598.6 | |
| 0.00 | 1.20 | 0.00 | 0.70 | 16.05 | 227.15 | -28.57 | 61.45 | 0.5253 | 781.0 | 731.1 | |
| 1.20 | 4.46 | 0.70 | 2.61 | 17.40 | 226.89 | -28.83 | 59.34 | 0.5371 | -368.6 | 63.5 | |
| 0.00 | 1.46 | 0.00 | 0.85 | 15.62 | 226.94 | -28.79 | 62.36 | 0.5256 | 357.0 | 294.5 | |
| 0.00 | 1.29 | 0.00 | 0.76 | 17.61 | 226.54 | -29.19 | 59.26 | 0.5429 | -481.0 | -260.7 | |
| 0.00 | 0.77 | 0.00 | 0.46 | 18.13 | 226.41 | -29.32 | 58.49 | 0.5480 | -431.0 | -350.4 | |
| 0.00 | 0.86 | 0.00 | 0.50 | 17.33 | 226.52 | -29.21 | 59.74 | 0.5415 | 656.0 | 530.3 | |
| 3.17 | 16.02 | 1.86 | 9.43 | 16.68 | 226.20 | -29.52 | 61.07 | 0.5415 | 1009.2 | 679.1 | |
| 8.74 | 35.13 | 5.12 | 20.50 | 15.61 | 226.20 | -29.52 | 62.90 | 0.5353 | 942.8 | 406.9 | |
| 8.48 | 49.44 | 5.00 | 29.20 | 15.85 | 225.66 | -30.06 | 62.86 | 0.5436 | 1103.8 | 690.9 | |
| 0.00 | 1.11 | 0.00 | 0.66 | 16.83 | 225.46 | -30.26 | 61.35 | 0.5518 | 313.0 | 341.6 | |
| 9.08 | -31.00 | 5.38 | -31.00 | 16.43 | 225.42 | -30.30 | 62.05 | 0.5500 | 905.0 | 999999 | |
| 0.00 | 2.83 | 0.00 | 1.66 | 14.68 | 225.32 | -30.41 | 65.09 | 0.5420 | 674.0 | 588.7 | |
| 0.00 | 1.03 | 0.00 | 0.61 | 15.05 | 225.26 | -30.46 | 64.50 | 0.5446 | 651.0 | 503.0 | |
| 0.00 | 0.94 | 0.00 | 0.56 | 14.77 | 224.98 | -30.74 | 65.15 | 0.5469 | 647.0 | 510.0 | |
| 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. | |