| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 48.56 | 151.78 | 102.93 | 348.30 | 19.58 | 88.11 | 77.57 | 289.47 | 0.9755 | -132.4 | -145.5 | |
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back to the solar disc SDO HMI 2011-11-15 11:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 6.19 | 63.52 | 17.51 | 184.95 | 19.10 | 90.91 | 80.37 | 288.90 | 0.9855 | -441.9 | -81.5 | |
| 2.92 | -1.00 | 8.62 | -1.00 | 19.30 | 91.34 | 80.80 | 289.10 | 0.9867 | 461.5 | 999999 | |
| 3.52 | -1.00 | 9.67 | -1.00 | 19.72 | 90.49 | 79.96 | 289.53 | 0.9844 | -404.3 | 999999 | |
| 1.80 | 4.64 | 3.98 | 10.33 | 18.27 | 87.81 | 77.27 | 288.10 | 0.9755 | 173.2 | 23.7 | |
| 0.00 | 3.09 | 0.00 | 6.12 | 18.19 | 86.20 | 75.66 | 288.06 | 0.9693 | 271.0 | 123.1 | |
| 2.49 | 30.08 | 4.90 | 57.64 | 19.01 | 86.01 | 75.47 | 288.92 | 0.9686 | 371.4 | -193.4 | |
| 0.00 | 1.46 | 0.00 | 2.72 | 18.52 | 85.24 | 74.70 | 288.43 | 0.9653 | 305.0 | 214.2 | |
| 16.42 | -6.00 | 31.70 | -6.00 | 19.15 | 85.81 | 75.27 | 289.06 | 0.9678 | -381.2 | 999999 | |
| 0.00 | 1.03 | 0.00 | 1.99 | 20.57 | 85.77 | 75.24 | 290.53 | 0.9679 | -351.0 | -213.2 | |
| 1.12 | -6.00 | 2.05 | -6.00 | 20.04 | 84.92 | 74.38 | 290.02 | 0.9642 | -260.4 | 999999 | |
| 0.00 | 0.26 | 0.00 | 0.43 | 19.56 | 83.08 | 72.55 | 289.61 | 0.9556 | 486.0 | 516.3 | |
| 3.01 | 47.70 | 5.48 | 84.12 | 21.22 | 84.73 | 74.20 | 291.26 | 0.9637 | -579.3 | -354.7 | |
| 8.94 | -12.00 | 15.35 | -12.00 | 20.51 | 83.68 | 73.14 | 290.57 | 0.9587 | 460.7 | 999999 | |
| 2.15 | -12.00 | 3.67 | -12.00 | 20.79 | 83.60 | 73.06 | 290.88 | 0.9584 | -268.4 | 999999 | |
| 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. | |