| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 46.28 | 308.08 | 26.47 | 175.64 | 20.08 | 192.94 | 22.87 | 312.27 | 0.4959 | -325.9 | -207.3 | |
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back to the solar disc SDO HMI 2011-11-30 16:58:56 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.02 | 0.00 | 0.60 | 20.62 | 196.79 | 26.71 | 308.76 | 0.5417 | -588.0 | -357.4 | |
| 40.31 | 234.19 | 23.15 | 134.52 | 19.48 | 194.70 | 24.63 | 309.05 | 0.5079 | -1236.7 | -377.2 | |
| 0.00 | 2.48 | 0.00 | 1.40 | 19.12 | 192.93 | 22.86 | 310.41 | 0.4840 | -861.0 | -713.7 | |
| 0.00 | 1.11 | 0.00 | 0.64 | 22.04 | 193.23 | 23.15 | 314.68 | 0.5147 | -814.0 | -646.1 | |
| 0.00 | 1.02 | 0.00 | 0.58 | 20.62 | 192.96 | 22.88 | 312.82 | 0.4982 | -870.0 | -639.8 | |
| 0.00 | 1.37 | 0.00 | 0.77 | 20.32 | 191.04 | 20.97 | 314.70 | 0.4740 | -884.0 | -672.6 | |
| 0.00 | 1.02 | 0.00 | 0.58 | 20.60 | 190.91 | 20.84 | 315.32 | 0.4755 | -977.0 | -814.2 | |
| 0.00 | 1.02 | 0.00 | 0.58 | 22.40 | 191.15 | 21.08 | 317.76 | 0.4966 | -620.0 | -462.2 | |
| 0.00 | 4.53 | 0.00 | 2.55 | 21.10 | 190.72 | 20.64 | 316.37 | 0.4786 | -848.0 | -681.0 | |
| 0.00 | 2.22 | 0.00 | 1.21 | 15.07 | 189.89 | 19.81 | 306.75 | 0.4102 | -799.0 | -558.7 | |
| 0.00 | 1.20 | 0.00 | 0.67 | 21.17 | 190.32 | 20.24 | 317.00 | 0.4751 | -842.0 | -589.7 | |
| 0.00 | 2.48 | 0.00 | 1.36 | 17.46 | 189.75 | 19.67 | 311.55 | 0.4309 | -766.0 | -613.8 | |
| 0.00 | 2.22 | 0.00 | 1.20 | 14.99 | 188.78 | 18.70 | 308.09 | 0.3952 | -913.0 | -769.3 | |
| 0.00 | 2.14 | 0.00 | 1.19 | 22.22 | 187.77 | 17.70 | 322.22 | 0.4612 | 889.0 | 724.4 | |
| 4.95 | 6.06 | 2.75 | 3.36 | 22.23 | 186.77 | 16.69 | 323.78 | 0.4519 | 892.7 | 718.7 | |
| 0.00 | 0.94 | 0.00 | 0.52 | 21.75 | 186.71 | 16.64 | 323.19 | 0.4456 | 775.0 | 668.3 | |
| 0.00 | 4.87 | 0.00 | 2.70 | 22.61 | 186.35 | 16.27 | 324.98 | 0.4527 | 873.0 | 746.1 | |
| 1.02 | 5.47 | 0.57 | 3.03 | 22.71 | 186.03 | 15.95 | 325.64 | 0.4510 | 917.1 | 823.9 | |
| 0.00 | 1.28 | 0.00 | 0.71 | 22.11 | 185.96 | 15.88 | 324.92 | 0.4429 | 896.0 | 733.9 | |
| 0.00 | 0.94 | 0.00 | 0.52 | 22.23 | 185.87 | 15.79 | 325.23 | 0.4437 | 852.0 | 732.3 | |
| 0.00 | 2.05 | 0.00 | 1.13 | 22.42 | 185.66 | 15.58 | 325.85 | 0.4443 | 868.0 | 768.7 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 23.80 | 185.32 | 15.25 | 328.21 | 0.4587 | 720.0 | 588.3 | |
| 0.00 | 6.32 | 0.00 | 3.49 | 22.90 | 185.09 | 15.01 | 327.46 | 0.4453 | 1111.0 | 918.9 | |
| 0.00 | 1.37 | 0.00 | 0.74 | 19.91 | 184.68 | 14.60 | 323.88 | 0.4038 | 914.0 | 665.1 | |
| 0.00 | 3.67 | 0.00 | 2.03 | 23.26 | 184.99 | 14.92 | 328.07 | 0.4490 | 625.0 | 692.7 | |
| 0.00 | 1.37 | 0.00 | 0.78 | 26.52 | 185.40 | 15.33 | 331.28 | 0.4942 | 777.0 | 620.7 | |
| 0.00 | 1.20 | 0.00 | 0.68 | 25.97 | 185.12 | 15.05 | 331.10 | 0.4850 | 779.0 | 645.0 | |
| 0.00 | 1.11 | 0.00 | 0.61 | 23.35 | 184.74 | 14.66 | 328.63 | 0.4482 | 732.0 | 635.2 | |
| 0.00 | 4.78 | 0.00 | 2.70 | 25.68 | 184.78 | 14.70 | 331.32 | 0.4787 | 819.0 | 701.5 | |
| 0.00 | 0.85 | 0.00 | 0.47 | 23.00 | 184.43 | 14.36 | 328.70 | 0.4412 | 843.0 | 769.3 | |
| 0.00 | 0.94 | 0.00 | 0.52 | 23.19 | 184.39 | 14.31 | 329.02 | 0.4433 | 809.0 | 580.7 | |
| 0.00 | 1.71 | 0.00 | 0.95 | 23.87 | 184.36 | 14.29 | 329.90 | 0.4519 | 714.0 | 641.6 | |
| 0.00 | 1.71 | 0.00 | 0.96 | 25.38 | 184.41 | 14.33 | 331.60 | 0.4721 | 865.0 | 735.5 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 24.12 | 184.22 | 14.15 | 330.45 | 0.4542 | 673.0 | 504.0 | |
| 0.00 | 1.20 | 0.00 | 0.65 | 21.04 | 182.90 | 12.82 | 328.91 | 0.4027 | 847.0 | 748.7 | |
| 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. | |