SDO HMI 2011-10-16 21:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 99.12 | 636.99 | 54.83 | 351.70 | 27.23 | 56.17 | 15.55 | 327.34 | 0.4427 | -1004.3 | -398.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.96 | 0.00 | 0.53 | 20.45 | 61.82 | 21.20 | 307.48 | 0.4287 | -718.0 | -586.0 | |
| 0.00 | 1.22 | 0.00 | 0.66 | 21.62 | 59.32 | 18.70 | 313.00 | 0.4093 | -648.0 | -532.6 | |
| 0.00 | 0.96 | 0.00 | 0.52 | 21.25 | 59.14 | 18.52 | 312.55 | 0.4035 | -859.0 | -749.0 | |
| 0.00 | 2.18 | 0.00 | 1.17 | 20.74 | 57.53 | 16.91 | 313.96 | 0.3795 | -773.0 | -633.2 | |
| 0.00 | 1.92 | 0.00 | 1.09 | 29.74 | 57.65 | 17.03 | 328.18 | 0.4844 | 711.0 | 620.4 | |
| 1.22 | 582.97 | 0.68 | 322.50 | 28.09 | 57.13 | 16.51 | 326.82 | 0.4599 | -283.1 | -424.9 | |
| 96.59 | -6.00 | 53.42 | -6.00 | 27.29 | 56.72 | 16.10 | 326.35 | 0.4467 | -1476.0 | 999999 | |
| 0.44 | 1.31 | 0.25 | 0.74 | 29.87 | 56.31 | 15.69 | 330.32 | 0.4756 | -668.0 | -519.4 | |
| 0.00 | 1.22 | 0.00 | 0.64 | 20.01 | 54.64 | 14.02 | 317.53 | 0.3387 | -780.0 | -673.2 | |
| 0.00 | 1.57 | 0.00 | 0.82 | 19.07 | 54.30 | 13.68 | 316.14 | 0.3240 | -942.0 | -762.1 | |
| 0.00 | 1.13 | 0.00 | 0.61 | 24.95 | 54.82 | 14.20 | 326.10 | 0.4007 | -845.0 | -628.7 | |
| 0.00 | 1.40 | 0.00 | 0.79 | 30.59 | 55.17 | 14.55 | 332.89 | 0.4765 | -666.0 | -523.2 | |
| 0.00 | 1.22 | 0.00 | 0.64 | 20.09 | 53.83 | 13.21 | 319.33 | 0.3308 | -835.0 | -688.5 | |
| 0.87 | 2.88 | 0.48 | 1.57 | 27.59 | 53.50 | 12.87 | 332.16 | 0.4246 | -733.3 | -777.7 | |
| 0.00 | 1.83 | 0.00 | 1.01 | 29.00 | 52.97 | 12.35 | 334.74 | 0.4401 | -811.0 | -681.3 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 27.61 | 52.74 | 12.12 | 333.55 | 0.4194 | -701.0 | -591.0 | |
| 0.00 | 0.79 | 0.00 | 0.43 | 27.52 | 52.49 | 11.87 | 333.91 | 0.4164 | -894.0 | -817.3 | |
| 0.00 | 2.53 | 0.00 | 1.40 | 29.36 | 52.66 | 12.04 | 335.67 | 0.4431 | -710.0 | -703.7 | |
| 0.00 | 1.57 | 0.00 | 0.86 | 27.78 | 52.34 | 11.72 | 334.48 | 0.4190 | -905.0 | -801.6 | |
| 0.00 | 0.87 | 0.00 | 0.48 | 28.01 | 52.16 | 11.54 | 335.08 | 0.4210 | -829.0 | -718.5 | |
| 0.00 | 1.13 | 0.00 | 0.63 | 29.57 | 52.20 | 11.58 | 336.70 | 0.4431 | -711.0 | -605.9 | |
| 0.00 | 0.96 | 0.00 | 0.52 | 28.01 | 51.95 | 11.33 | 335.47 | 0.4197 | -776.0 | -554.0 | |
| 0.00 | 1.48 | 0.00 | 0.82 | 29.12 | 51.94 | 11.31 | 336.70 | 0.4351 | -788.0 | -597.6 | |
| 0.00 | 1.48 | 0.00 | 0.80 | 27.00 | 51.03 | 10.41 | 336.11 | 0.3992 | -922.0 | -617.8 | |
| 0.00 | 1.83 | 0.00 | 0.99 | 27.91 | 50.53 | 9.91 | 338.08 | 0.4093 | -682.0 | -600.0 | |
| 0.00 | 1.40 | 0.00 | 0.75 | 26.88 | 50.27 | 9.65 | 337.53 | 0.3928 | -866.0 | -713.3 | |
| 0.00 | 1.31 | 0.00 | 0.71 | 28.28 | 47.28 | 6.65 | 345.09 | 0.3983 | 720.0 | 580.0 | |
| 0.00 | 0.79 | 0.00 | 0.42 | 28.06 | 46.07 | 5.45 | 347.55 | 0.3904 | 544.0 | 481.9 | |
| 0.00 | 3.32 | 0.00 | 1.77 | 27.01 | 45.01 | 4.39 | 349.35 | 0.3704 | 725.0 | 628.5 | |
| 0.00 | 1.75 | 0.00 | 0.92 | 25.20 | 43.52 | 2.90 | 352.17 | 0.3373 | 847.0 | 703.0 | |
| 0.00 | 1.75 | 0.00 | 0.94 | 28.47 | 43.13 | 2.51 | 354.31 | 0.3895 | 800.0 | 583.7 | |
| 0.00 | 1.66 | 0.00 | 0.86 | 22.53 | 42.55 | 1.93 | 353.83 | 0.2913 | 964.0 | 787.3 | |
| 0.00 | 3.23 | 0.00 | 1.71 | 26.61 | 41.72 | 1.09 | 357.25 | 0.3576 | 809.0 | 669.5 | |
| 0.00 | 0.87 | 0.00 | 0.46 | 25.40 | 39.52 | -1.10 | 2.95 | 0.3377 | 773.0 | 570.4 | |
| 0.00 | 3.40 | 0.00 | 1.81 | 27.25 | 38.73 | -1.89 | 4.58 | 0.3688 | 660.0 | 662.0 | |
| 0.00 | 1.05 | 0.00 | 0.56 | 27.05 | 38.57 | -2.05 | 5.03 | 0.3659 | 858.0 | 670.9 | |
| 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. | |