SDO HMI 2011-11-29 02:58:56 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 34.05 | 166.59 | 23.59 | 115.45 | 15.74 | 233.41 | 42.49 | 291.54 | 0.7013 | -845.1 | -331.2 | |
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See sunspots with tool (Click here to study sunspot positions and configurations with tool using white-light and magnetogram images and polarity drawing) (It is recommended to set high resolution on your display!) |
| spot | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.14 | 5.90 | 1.54 | 4.25 | 17.59 | 235.30 | 44.38 | 293.37 | 0.7286 | -501.8 | -548.2 | |
| 0.00 | 1.11 | 0.00 | 0.80 | 17.97 | 234.94 | 44.02 | 294.00 | 0.7259 | -656.0 | -604.5 | |
| 0.00 | 1.03 | 0.00 | 0.73 | 17.84 | 234.77 | 43.85 | 293.90 | 0.7236 | -624.0 | -504.8 | |
| 0.86 | 154.10 | 0.59 | 106.58 | 15.18 | 233.72 | 42.80 | 290.66 | 0.7032 | -548.1 | -318.4 | |
| 25.23 | -4.00 | 17.44 | -4.00 | 15.40 | 233.36 | 42.44 | 291.09 | 0.6996 | -1044.8 | 999999 | |
| 0.00 | 0.77 | 0.00 | 0.55 | 19.00 | 234.32 | 43.40 | 295.61 | 0.7227 | 323.0 | 273.9 | |
| 4.28 | -4.00 | 2.96 | -4.00 | 16.54 | 233.24 | 42.32 | 292.70 | 0.7020 | -642.1 | 999999 | |
| 1.54 | -4.00 | 1.06 | -4.00 | 15.80 | 232.92 | 42.00 | 291.81 | 0.6958 | -907.8 | 999999 | |
| 0.00 | 0.86 | 0.00 | 0.58 | 13.56 | 232.23 | 41.31 | 288.87 | 0.6805 | -549.0 | -540.2 | |
| 0.00 | 1.54 | 0.00 | 1.07 | 18.96 | 232.77 | 41.85 | 296.19 | 0.7055 | -669.0 | -486.5 | |
| 0.00 | 1.28 | 0.00 | 0.89 | 19.34 | 232.25 | 41.33 | 296.92 | 0.7013 | -651.0 | -551.3 | |
| 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. | |