SDO HMI 2011-06-22 15:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 78.21 | 477.83 | 47.78 | 289.57 | 17.14 | 169.10 | 32.15 | 298.00 | 0.5772 | -596.7 | -264.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 1.27 | 0.00 | 0.80 | 14.26 | 173.13 | 36.17 | 291.10 | 0.6154 | -687.0 | -556.6 | |
| 75.31 | 418.92 | 46.03 | 255.87 | 17.08 | 169.98 | 33.02 | 297.19 | 0.5878 | -1402.3 | -381.0 | |
| 1.36 | -2.00 | 0.83 | -2.00 | 16.46 | 169.55 | 32.60 | 296.44 | 0.5792 | -1238.0 | 999999 | |
| 0.00 | 2.00 | 0.00 | 1.19 | 16.42 | 168.05 | 31.09 | 297.32 | 0.5596 | -908.0 | -766.1 | |
| 0.00 | 0.82 | 0.00 | 0.49 | 16.26 | 168.02 | 31.06 | 297.07 | 0.5584 | -261.0 | -236.4 | |
| 0.00 | 1.00 | 0.00 | 0.60 | 16.58 | 168.00 | 31.05 | 297.61 | 0.5599 | -843.0 | -701.9 | |
| 0.00 | 1.63 | 0.00 | 0.98 | 18.19 | 168.23 | 31.28 | 300.07 | 0.5721 | -639.0 | -418.3 | |
| 1.54 | 1.81 | 0.92 | 1.08 | 18.95 | 166.89 | 29.93 | 302.26 | 0.5602 | 682.7 | 548.3 | |
| 0.00 | 1.18 | 0.00 | 0.69 | 18.36 | 165.30 | 28.35 | 302.56 | 0.5367 | 546.0 | 444.9 | |
| 0.00 | 1.45 | 0.00 | 0.84 | 16.16 | 164.61 | 27.66 | 299.33 | 0.5134 | 789.0 | 687.6 | |
| 0.00 | 0.82 | 0.00 | 0.47 | 17.17 | 164.56 | 27.60 | 301.15 | 0.5192 | 626.0 | 504.8 | |
| 0.00 | 0.91 | 0.00 | 0.53 | 19.11 | 164.38 | 27.42 | 304.58 | 0.5306 | 481.0 | 438.1 | |
| 0.00 | 0.91 | 0.00 | 0.53 | 18.51 | 164.24 | 27.28 | 303.70 | 0.5245 | 546.0 | 434.3 | |
| 0.00 | 0.91 | 0.00 | 0.53 | 18.35 | 164.18 | 27.22 | 303.49 | 0.5226 | 640.0 | 499.1 | |
| 0.00 | 2.72 | 0.00 | 1.58 | 18.64 | 163.79 | 26.83 | 304.32 | 0.5199 | 564.0 | 494.9 | |
| 0.00 | 2.36 | 0.00 | 1.36 | 17.79 | 163.51 | 26.55 | 303.11 | 0.5101 | 730.0 | 575.2 | |
| 0.00 | 3.27 | 0.00 | 1.85 | 15.62 | 162.97 | 26.01 | 299.70 | 0.4882 | 934.0 | 737.6 | |
| 0.00 | 1.81 | 0.00 | 1.04 | 17.54 | 162.76 | 25.80 | 303.37 | 0.4989 | 772.0 | 617.1 | |
| 0.00 | 8.35 | 0.00 | 4.77 | 17.77 | 162.65 | 25.69 | 303.87 | 0.4992 | 759.0 | 671.7 | |
| 0.00 | 1.45 | 0.00 | 0.83 | 18.78 | 162.74 | 25.78 | 305.53 | 0.5080 | 763.0 | 657.6 | |
| 0.00 | 0.73 | 0.00 | 0.42 | 18.56 | 162.70 | 25.74 | 305.19 | 0.5058 | 784.0 | 622.9 | |
| 0.00 | 0.82 | 0.00 | 0.45 | 13.38 | 161.79 | 24.83 | 296.38 | 0.4579 | 782.0 | 594.8 | |
| 0.00 | 1.27 | 0.00 | 0.73 | 18.85 | 162.43 | 25.47 | 305.95 | 0.5047 | 747.0 | 560.4 | |
| 0.00 | 1.18 | 0.00 | 0.68 | 19.05 | 162.14 | 25.18 | 306.57 | 0.5028 | 745.0 | 542.7 | |
| 0.00 | 1.45 | 0.00 | 0.83 | 19.50 | 161.75 | 24.79 | 307.72 | 0.5017 | 531.0 | 446.6 | |
| 0.00 | 2.09 | 0.00 | 1.17 | 16.81 | 161.03 | 24.07 | 303.71 | 0.4713 | 896.0 | 756.8 | |
| 0.00 | 2.27 | 0.00 | 1.27 | 17.64 | 160.13 | 23.18 | 306.19 | 0.4666 | 974.0 | 822.2 | |
| 0.00 | 0.91 | 0.00 | 0.51 | 17.83 | 160.12 | 23.17 | 306.54 | 0.4681 | 896.0 | 743.3 | |
| 0.00 | 2.18 | 0.00 | 1.22 | 18.15 | 159.68 | 22.72 | 307.62 | 0.4653 | 853.0 | 612.3 | |
| 0.00 | 1.09 | 0.00 | 0.62 | 21.52 | 159.66 | 22.71 | 313.33 | 0.4956 | 694.0 | 604.2 | |
| 0.00 | 1.18 | 0.00 | 0.65 | 15.45 | 158.49 | 21.53 | 303.84 | 0.4276 | 598.0 | 562.0 | |
| 0.00 | 1.36 | 0.00 | 0.77 | 21.62 | 159.22 | 22.26 | 314.02 | 0.4917 | 440.0 | 475.8 | |
| 0.00 | 1.00 | 0.00 | 0.57 | 22.02 | 158.58 | 21.62 | 315.43 | 0.4886 | 727.0 | 625.0 | |
| 0.00 | 3.63 | 0.00 | 1.96 | 15.31 | 156.78 | 19.83 | 305.63 | 0.4042 | 630.0 | 714.5 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 17.66 | 154.87 | 17.92 | 313.05 | 0.4028 | 822.0 | 652.3 | |
| 0.00 | 1.63 | 0.00 | 0.90 | 20.41 | 154.74 | 17.78 | 318.15 | 0.4308 | 815.0 | 638.7 | |
| 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. | |