SDO HMI 2011-11-14 06:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.05 | 167.60 | 60.83 | 466.24 | 19.07 | 106.49 | 80.04 | 288.86 | 0.9839 | -30.9 | -70.3 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.95 | 86.64 | 28.98 | 286.78 | 19.10 | 108.24 | 81.79 | 288.87 | 0.9891 | 460.9 | 183.2 | |
| 8.17 | -1.00 | 25.06 | -1.00 | 19.03 | 107.64 | 81.19 | 288.81 | 0.9876 | -303.8 | 999999 | |
| 0.00 | 0.52 | 0.00 | 1.36 | 18.92 | 106.06 | 79.61 | 288.70 | 0.9832 | -165.0 | -184.0 | |
| 0.00 | 2.67 | 0.00 | 7.12 | 19.38 | 106.24 | 79.79 | 289.17 | 0.9837 | -453.0 | -387.9 | |
| 2.93 | 50.33 | 6.79 | 112.29 | 18.47 | 104.44 | 77.99 | 288.26 | 0.9779 | -564.1 | -443.0 | |
| 0.00 | 1.38 | 0.00 | 3.11 | 19.68 | 103.99 | 77.54 | 289.51 | 0.9764 | -283.0 | -225.7 | |
| 0.00 | 8.95 | 0.00 | 19.04 | 19.40 | 103.26 | 76.81 | 289.25 | 0.9737 | -608.0 | -494.3 | |
| 0.00 | 1.20 | 0.00 | 2.69 | 19.85 | 103.82 | 77.37 | 289.69 | 0.9758 | -510.0 | -421.4 | |
| 0.00 | 1.46 | 0.00 | 3.19 | 20.15 | 103.57 | 77.12 | 290.00 | 0.9750 | -564.0 | -511.4 | |
| 0.00 | 1.29 | 0.00 | 3.11 | 21.19 | 104.82 | 78.37 | 291.04 | 0.9794 | -431.0 | -384.4 | |
| 0.00 | 2.41 | 0.00 | 5.85 | 21.38 | 105.01 | 78.56 | 291.22 | 0.9800 | -366.0 | -316.2 | |
| 0.00 | 1.46 | 0.00 | 3.02 | 20.22 | 102.71 | 76.26 | 290.10 | 0.9717 | -435.0 | -429.1 | |
| 0.00 | 6.11 | 0.00 | 12.54 | 20.66 | 102.72 | 76.27 | 290.56 | 0.9718 | -372.0 | -334.9 | |
| 0.00 | 3.18 | 0.00 | 6.14 | 20.14 | 101.68 | 75.23 | 290.06 | 0.9676 | 50.0 | 0.2 | |
| 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. | |