| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.75 | 114.68 | 98.36 | 342.29 | 19.60 | 88.02 | 80.79 | 289.45 | 0.9853 | -115.6 | -97.0 | |
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back to the solar disc SDO HMI 2011-11-15 17:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.47 | 41.75 | 18.20 | 178.47 | 19.04 | 90.82 | 83.59 | 288.84 | 0.9931 | -339.4 | -99.6 | |
| 4.38 | -1.00 | 19.20 | -1.00 | 19.27 | 91.28 | 84.05 | 289.08 | 0.9940 | 572.5 | 999999 | |
| 0.00 | 2.23 | 0.00 | 6.37 | 18.50 | 87.62 | 80.38 | 288.29 | 0.9856 | 261.0 | 113.6 | |
| 0.00 | 2.15 | 0.00 | 5.38 | 18.25 | 86.25 | 79.02 | 288.05 | 0.9815 | -76.0 | 47.1 | |
| 11.00 | 16.49 | 26.76 | 40.35 | 18.99 | 85.73 | 78.50 | 288.82 | 0.9798 | -492.5 | -83.8 | |
| 0.00 | 2.92 | 0.00 | 6.61 | 19.66 | 84.85 | 77.61 | 289.52 | 0.9769 | -393.0 | -332.3 | |
| 0.00 | 2.75 | 0.00 | 6.03 | 20.12 | 84.43 | 77.19 | 290.01 | 0.9754 | 109.0 | 52.9 | |
| 1.20 | 2.58 | 2.60 | 5.62 | 20.39 | 84.14 | 76.91 | 290.29 | 0.9744 | 166.8 | -27.7 | |
| 4.47 | 43.81 | 10.03 | 93.46 | 20.84 | 84.61 | 77.38 | 290.74 | 0.9762 | -587.1 | -120.8 | |
| 1.89 | -9.00 | 3.90 | -9.00 | 20.27 | 83.39 | 76.16 | 290.19 | 0.9716 | 473.1 | 999999 | |
| 0.52 | -9.00 | 1.20 | -9.00 | 21.36 | 85.09 | 77.85 | 291.26 | 0.9779 | 189.0 | 999999 | |
| 2.66 | -9.00 | 6.08 | -9.00 | 21.24 | 84.87 | 77.64 | 291.14 | 0.9771 | -443.8 | 999999 | |
| 4.47 | -9.00 | 8.98 | -9.00 | 20.57 | 83.05 | 75.81 | 290.51 | 0.9703 | 353.8 | 999999 | |
| 0.69 | -9.00 | 1.41 | -9.00 | 20.84 | 83.33 | 76.10 | 290.78 | 0.9714 | -326.1 | 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. | |