SDO HMI 2011-12-01 04:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 39.23 | 269.78 | 23.77 | 163.11 | 20.12 | 193.12 | 29.65 | 305.70 | 0.5742 | -206.3 | -271.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 2.22 | 0.00 | 1.39 | 19.10 | 197.16 | 33.69 | 300.98 | 0.6137 | -771.0 | -552.0 | |
| 33.59 | 206.47 | 20.52 | 126.17 | 19.68 | 194.65 | 31.18 | 303.61 | 0.5876 | -1117.6 | -391.6 | |
| 0.00 | 4.44 | 0.00 | 2.65 | 19.14 | 192.36 | 28.89 | 304.58 | 0.5566 | -838.0 | -717.6 | |
| 0.00 | 3.33 | 0.00 | 1.96 | 17.40 | 191.94 | 28.47 | 302.14 | 0.5394 | -318.0 | -468.3 | |
| 0.00 | 1.54 | 0.00 | 0.93 | 22.13 | 192.34 | 28.87 | 309.12 | 0.5787 | -818.0 | -601.8 | |
| 0.00 | 1.20 | 0.00 | 0.71 | 21.22 | 190.98 | 27.52 | 309.00 | 0.5564 | -1034.0 | -845.9 | |
| 0.00 | 1.03 | 0.00 | 0.61 | 20.46 | 190.73 | 27.26 | 308.09 | 0.5474 | -779.0 | -683.1 | |
| 0.00 | 1.97 | 0.00 | 1.16 | 20.75 | 190.75 | 27.28 | 308.51 | 0.5499 | -914.0 | -762.3 | |
| 0.00 | 0.94 | 0.00 | 0.56 | 21.91 | 190.99 | 27.52 | 310.04 | 0.5620 | -685.0 | -551.4 | |
| 0.00 | 1.71 | 0.00 | 1.02 | 21.35 | 190.76 | 27.29 | 309.40 | 0.5549 | -685.0 | -591.3 | |
| 0.00 | 1.45 | 0.00 | 0.86 | 21.35 | 190.33 | 26.86 | 309.81 | 0.5501 | -771.0 | -635.9 | |
| 0.00 | 1.11 | 0.00 | 0.63 | 15.46 | 189.05 | 25.58 | 301.27 | 0.4889 | -807.0 | -642.3 | |
| 0.00 | 3.33 | 0.00 | 1.89 | 15.34 | 188.79 | 25.33 | 301.28 | 0.4847 | -627.0 | -509.7 | |
| 0.00 | 1.71 | 0.00 | 1.00 | 21.80 | 188.54 | 25.08 | 312.30 | 0.5341 | 542.0 | 463.5 | |
| 0.00 | 0.68 | 0.00 | 0.40 | 21.78 | 187.70 | 24.23 | 313.17 | 0.5247 | 769.0 | 659.9 | |
| 0.00 | 1.28 | 0.00 | 0.75 | 22.31 | 187.76 | 24.29 | 313.90 | 0.5303 | 861.0 | 652.5 | |
| 3.16 | 3.93 | 1.83 | 2.27 | 22.38 | 186.62 | 23.15 | 315.29 | 0.5189 | 803.9 | 765.2 | |
| 0.00 | 3.59 | 0.00 | 2.07 | 22.13 | 186.33 | 22.87 | 315.26 | 0.5134 | 913.0 | 684.8 | |
| 0.00 | 1.62 | 0.00 | 0.94 | 22.55 | 186.16 | 22.69 | 316.07 | 0.5157 | 818.0 | 513.1 | |
| 0.00 | 1.79 | 0.00 | 1.03 | 22.20 | 185.89 | 22.43 | 315.88 | 0.5094 | 974.0 | 756.2 | |
| 0.00 | 2.22 | 0.00 | 1.28 | 22.64 | 185.87 | 22.40 | 316.56 | 0.5136 | 728.0 | 579.2 | |
| 2.48 | 2.82 | 1.42 | 1.62 | 22.93 | 185.15 | 21.69 | 317.86 | 0.5093 | 836.6 | 710.2 | |
| 0.00 | 0.85 | 0.00 | 0.50 | 24.22 | 185.20 | 21.74 | 319.59 | 0.5231 | 654.0 | 508.6 | |
| 0.00 | 0.77 | 0.00 | 0.44 | 23.13 | 184.98 | 21.51 | 318.35 | 0.5095 | 881.0 | 777.2 | |
| 0.00 | 0.51 | 0.00 | 0.29 | 22.90 | 184.84 | 21.37 | 318.21 | 0.5058 | 894.0 | 748.5 | |
| 0.00 | 3.85 | 0.00 | 2.22 | 23.61 | 184.89 | 21.42 | 319.14 | 0.5136 | 833.0 | 677.8 | |
| 0.00 | 0.68 | 0.00 | 0.40 | 25.90 | 185.20 | 21.74 | 321.82 | 0.5410 | 805.0 | 717.6 | |
| 0.00 | 0.94 | 0.00 | 0.54 | 23.96 | 184.85 | 21.38 | 319.69 | 0.5170 | 733.0 | 585.5 | |
| 0.00 | 1.20 | 0.00 | 0.69 | 22.97 | 184.64 | 21.17 | 318.55 | 0.5045 | 785.0 | 671.6 | |
| 0.00 | 1.71 | 0.00 | 1.01 | 26.20 | 185.23 | 21.76 | 322.16 | 0.5444 | 670.0 | 572.8 | |
| 0.00 | 1.03 | 0.00 | 0.60 | 26.04 | 185.05 | 21.59 | 322.17 | 0.5411 | 895.0 | 792.8 | |
| 0.00 | 0.94 | 0.00 | 0.54 | 22.94 | 184.43 | 20.96 | 318.78 | 0.5020 | 939.0 | 826.2 | |
| 0.00 | 0.60 | 0.00 | 0.35 | 26.46 | 184.99 | 21.53 | 322.77 | 0.5452 | 704.0 | 568.3 | |
| 0.00 | 3.16 | 0.00 | 1.82 | 23.87 | 184.31 | 20.84 | 320.24 | 0.5108 | 774.0 | 681.6 | |
| 0.00 | 1.03 | 0.00 | 0.59 | 23.61 | 184.06 | 20.59 | 320.21 | 0.5056 | 736.0 | 578.9 | |
| 0.00 | 0.85 | 0.00 | 0.50 | 25.52 | 184.29 | 20.82 | 322.46 | 0.5285 | 683.0 | 579.6 | |
| 0.00 | 1.28 | 0.00 | 0.72 | 20.92 | 182.91 | 19.44 | 317.81 | 0.4649 | 815.0 | 598.5 | |
| 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. | |