| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.63 | 317.12 | 23.82 | 173.22 | 28.02 | 43.32 | 0.40 | 359.20 | 0.4231 | -900.5 | -412.2 | |
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back to the solar disc SDO HMI 2011-11-13 00:58:58 UT
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| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 0.69 | 0.00 | 0.38 | 29.70 | 50.29 | 7.37 | 346.02 | 0.4632 | -751.0 | -666.8 | |
| 0.00 | 1.12 | 0.00 | 0.62 | 29.21 | 49.26 | 6.34 | 347.63 | 0.4522 | -713.0 | -585.9 | |
| 0.00 | 1.03 | 0.00 | 0.57 | 28.59 | 48.75 | 5.83 | 348.28 | 0.4410 | -700.0 | -567.6 | |
| 0.00 | 1.98 | 0.00 | 1.12 | 32.31 | 44.97 | 2.05 | 356.46 | 0.4905 | -748.0 | -553.2 | |
| 1.38 | 302.84 | 0.75 | 165.39 | 27.69 | 44.10 | 1.18 | 357.48 | 0.4177 | -852.8 | -436.0 | |
| 35.28 | -5.00 | 19.26 | -5.00 | 27.98 | 43.50 | 0.58 | 358.78 | 0.4221 | -1321.9 | 999999 | |
| 5.08 | -5.00 | 2.78 | -5.00 | 28.37 | 43.16 | 0.24 | 359.49 | 0.4282 | -848.2 | 999999 | |
| 1.89 | -5.00 | 1.03 | -5.00 | 28.18 | 42.79 | -0.13 | 0.26 | 0.4251 | -815.8 | 999999 | |
| 0.00 | 1.12 | 0.00 | 0.62 | 29.00 | 40.49 | -2.43 | 4.87 | 0.4397 | -734.0 | -623.5 | |
| 0.00 | 1.20 | 0.00 | 0.66 | 28.77 | 40.46 | -2.46 | 4.98 | 0.4361 | -850.0 | -659.4 | |
| 0.00 | 2.15 | 0.00 | 1.18 | 27.67 | 37.56 | -5.36 | 11.26 | 0.4255 | 873.0 | 694.1 | |
| 0.00 | 1.12 | 0.00 | 0.60 | 26.02 | 37.01 | -5.91 | 13.38 | 0.4017 | 762.0 | 622.6 | |
| 0.00 | 1.89 | 0.00 | 1.02 | 25.60 | 36.44 | -6.48 | 14.92 | 0.3974 | 946.0 | 772.9 | |
| 0.00 | 1.98 | 0.00 | 1.06 | 23.28 | 33.06 | -9.86 | 24.50 | 0.3809 | 757.0 | 510.8 | |
| 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. | |