SDO HMI 2011-11-15 19:58:58 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 42.54 | 115.62 | 126.85 | 377.62 | 19.68 | 87.88 | 81.75 | 289.52 | 0.9877 | -162.9 | -65.0 | |
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.30 | 35.39 | 20.59 | 181.34 | 19.01 | 90.90 | 84.77 | 288.83 | 0.9952 | -280.7 | -92.5 | |
| 3.87 | -1.00 | 20.28 | -1.00 | 19.23 | 91.47 | 85.34 | 289.07 | 0.9961 | 512.4 | 999999 | |
| 0.00 | 1.55 | 0.00 | 4.86 | 18.57 | 87.48 | 81.35 | 288.37 | 0.9882 | 120.0 | 43.4 | |
| 0.00 | 1.63 | 0.00 | 4.45 | 18.36 | 86.04 | 79.92 | 288.16 | 0.9842 | 247.0 | 64.7 | |
| 2.41 | 17.78 | 6.70 | 47.74 | 18.92 | 86.21 | 80.08 | 288.72 | 0.9847 | 265.0 | -332.4 | |
| 0.00 | 1.29 | 0.00 | 3.91 | 19.50 | 87.08 | 80.95 | 289.31 | 0.9871 | -249.0 | -259.6 | |
| 12.11 | -5.00 | 32.23 | -5.00 | 19.00 | 85.65 | 79.53 | 288.82 | 0.9831 | -456.9 | 999999 | |
| 0.00 | 1.03 | 0.00 | 2.99 | 20.12 | 86.66 | 80.54 | 289.94 | 0.9860 | -445.0 | -371.2 | |
| 0.86 | 7.56 | 2.07 | 18.28 | 19.97 | 84.57 | 78.45 | 289.82 | 0.9797 | -224.1 | -184.4 | |
| 0.00 | 0.69 | 0.00 | 1.54 | 19.33 | 83.48 | 77.35 | 289.19 | 0.9759 | 260.0 | 270.2 | |
| 0.00 | 0.94 | 0.00 | 2.21 | 20.37 | 84.18 | 78.05 | 290.23 | 0.9785 | 194.0 | 99.5 | |
| 13.75 | 47.33 | 33.71 | 109.34 | 21.04 | 84.64 | 78.51 | 290.91 | 0.9800 | -519.7 | 52.8 | |
| 0.00 | 0.43 | 0.00 | 0.96 | 20.40 | 83.48 | 77.35 | 290.29 | 0.9760 | 261.0 | 198.4 | |
| 5.24 | -12.00 | 11.27 | -12.00 | 20.61 | 82.96 | 76.83 | 290.52 | 0.9742 | 366.0 | 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. | |