SDO HMI 2011-11-24 01:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 94.74 | 487.89 | 53.55 | 276.50 | 15.24 | 231.44 | -25.93 | 60.57 | 0.4844 | -394.7 | -179.8 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.94 | 0.00 | 0.51 | 13.13 | 236.14 | -21.23 | 60.65 | 0.4063 | 709.0 | 419.5 | |
| 0.00 | 0.51 | 0.00 | 0.28 | 13.28 | 236.03 | -21.34 | 60.44 | 0.4089 | 522.0 | 355.0 | |
| 9.77 | 29.13 | 5.32 | 15.86 | 13.24 | 235.31 | -22.05 | 61.27 | 0.4186 | -1130.1 | -491.9 | |
| 2.83 | -3.00 | 1.54 | -3.00 | 13.09 | 235.13 | -22.24 | 61.78 | 0.4201 | -840.4 | 999999 | |
| 45.06 | 263.77 | 24.88 | 145.64 | 14.83 | 234.32 | -23.05 | 58.96 | 0.4436 | -1324.7 | -463.6 | |
| 4.45 | 5.23 | 2.44 | 2.86 | 13.26 | 234.49 | -22.88 | 62.04 | 0.4303 | -923.3 | -711.1 | |
| 0.00 | 1.03 | 0.00 | 0.58 | 17.67 | 233.79 | -23.57 | 54.10 | 0.4724 | -915.0 | -749.6 | |
| 0.00 | 0.94 | 0.00 | 0.53 | 17.09 | 233.84 | -23.53 | 55.12 | 0.4671 | -771.0 | -551.8 | |
| 0.00 | 1.29 | 0.00 | 0.71 | 12.92 | 233.56 | -23.81 | 63.61 | 0.4411 | -812.0 | -627.7 | |
| 0.00 | 1.37 | 0.00 | 0.78 | 17.53 | 232.35 | -25.02 | 55.83 | 0.4894 | -750.0 | -616.1 | |
| 0.00 | 1.03 | 0.00 | 0.57 | 12.97 | 232.72 | -24.64 | 64.22 | 0.4532 | 920.0 | 627.0 | |
| 0.00 | 1.97 | 0.00 | 1.13 | 17.83 | 231.41 | -25.96 | 56.20 | 0.5035 | -640.0 | -572.5 | |
| 0.00 | 1.63 | 0.00 | 0.93 | 17.67 | 231.33 | -26.04 | 56.55 | 0.5034 | -674.0 | -620.8 | |
| 0.00 | 3.43 | 0.00 | 1.95 | 16.04 | 231.16 | -26.21 | 59.61 | 0.4941 | -870.0 | -614.9 | |
| 0.00 | 1.71 | 0.00 | 0.98 | 17.20 | 230.81 | -26.56 | 57.83 | 0.5066 | -631.0 | -482.2 | |
| 0.00 | 2.31 | 0.00 | 1.31 | 14.49 | 231.13 | -26.24 | 62.52 | 0.4845 | -813.0 | -687.6 | |
| 4.88 | 13.28 | 2.79 | 7.58 | 15.76 | 230.61 | -26.76 | 60.58 | 0.4994 | -819.4 | -646.8 | |
| 0.00 | 1.71 | 0.00 | 0.99 | 17.16 | 229.49 | -27.87 | 59.03 | 0.5231 | -589.0 | -504.9 | |
| 2.48 | 19.28 | 1.46 | 11.31 | 16.49 | 227.98 | -29.39 | 61.33 | 0.5384 | -472.8 | -292.3 | |
| 0.00 | 1.03 | 0.00 | 0.61 | 16.85 | 227.70 | -29.66 | 60.91 | 0.5441 | -466.0 | -407.5 | |
| 0.34 | 3.00 | 0.20 | 1.76 | 16.24 | 227.56 | -29.81 | 62.06 | 0.5424 | 1039.2 | 655.8 | |
| 0.00 | 1.20 | 0.00 | 0.71 | 16.66 | 227.20 | -30.16 | 61.59 | 0.5495 | -440.0 | -215.6 | |
| 0.00 | 6.00 | 0.00 | 3.57 | 17.24 | 226.95 | -30.41 | 60.80 | 0.5560 | -597.0 | -265.9 | |
| 0.00 | 1.37 | 0.00 | 0.81 | 16.05 | 227.13 | -30.24 | 62.68 | 0.5469 | 798.0 | 663.6 | |
| 0.00 | 3.94 | 0.00 | 2.35 | 17.36 | 226.75 | -30.61 | 60.74 | 0.5593 | -42.0 | -38.5 | |
| 0.00 | 0.69 | 0.00 | 0.41 | 16.14 | 226.93 | -30.43 | 62.66 | 0.5499 | 780.0 | 557.8 | |
| 0.00 | 1.11 | 0.00 | 0.66 | 15.95 | 226.47 | -30.90 | 63.29 | 0.5550 | 741.0 | 610.6 | |
| 1.80 | 10.79 | 1.08 | 6.45 | 16.65 | 226.16 | -31.21 | 62.32 | 0.5627 | 1007.6 | 737.6 | |
| 8.14 | 99.89 | 4.84 | 59.68 | 15.61 | 226.20 | -31.17 | 64.03 | 0.5566 | 948.3 | 545.6 | |
| 0.00 | 1.29 | 0.00 | 0.77 | 16.89 | 225.83 | -31.54 | 62.14 | 0.5683 | 734.0 | 609.6 | |
| 0.00 | 1.97 | 0.00 | 1.17 | 14.17 | 226.07 | -31.29 | 66.54 | 0.5511 | 617.0 | 493.2 | |
| 7.88 | -29.00 | 4.72 | -29.00 | 15.87 | 225.65 | -31.72 | 63.92 | 0.5652 | 1061.1 | 999999 | |
| 0.00 | 2.14 | 0.00 | 1.29 | 16.88 | 225.43 | -31.94 | 62.41 | 0.5734 | 82.0 | 176.7 | |
| 7.11 | -29.00 | 4.28 | -29.00 | 16.48 | 225.43 | -31.94 | 63.06 | 0.5712 | 923.0 | 999999 | |
| 0.00 | 1.03 | 0.00 | 0.62 | 14.74 | 225.19 | -32.18 | 66.09 | 0.5656 | 701.0 | 625.1 | |
| 0.00 | 1.88 | 0.00 | 1.14 | 14.72 | 224.36 | -33.01 | 66.57 | 0.5765 | 622.0 | 434.3 | |
| 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. | |