SDO HMI 2011-11-22 15:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.30 | 243.72 | 29.79 | 207.35 | 17.44 | 223.07 | -52.99 | 69.84 | 0.8137 | -594.4 | -150.8 | |
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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 |
| 0.00 | 0.86 | 0.00 | 0.72 | 18.60 | 223.97 | -52.10 | 68.24 | 0.8075 | -657.0 | -604.5 | |
| 30.67 | 221.02 | 25.80 | 187.15 | 17.44 | 223.43 | -52.63 | 69.77 | 0.8103 | -912.2 | -217.2 | |
| 1.46 | -2.00 | 1.25 | -2.00 | 17.98 | 222.79 | -53.28 | 69.26 | 0.8175 | -581.9 | 999999 | |
| 3.17 | -2.00 | 2.74 | -2.00 | 18.00 | 222.36 | -53.71 | 69.33 | 0.8215 | -421.9 | 999999 | |
| 0.00 | 1.46 | 0.00 | 1.26 | 15.83 | 222.05 | -54.01 | 71.99 | 0.8208 | 697.0 | 585.2 | |
| 0.00 | 11.22 | 0.00 | 9.82 | 16.46 | 221.53 | -54.53 | 71.33 | 0.8267 | 355.0 | 299.7 | |
| 0.00 | 1.03 | 0.00 | 0.90 | 16.18 | 221.43 | -54.63 | 71.68 | 0.8271 | 430.0 | 310.3 | |
| 0.00 | 3.85 | 0.00 | 3.52 | 17.31 | 220.01 | -56.06 | 70.60 | 0.8419 | 639.0 | 586.1 | |
| 0.00 | 1.03 | 0.00 | 0.93 | 16.43 | 220.35 | -55.72 | 71.58 | 0.8375 | 616.0 | 591.2 | |
| 0.00 | 2.74 | 0.00 | 2.56 | 17.23 | 219.09 | -56.98 | 70.86 | 0.8498 | 648.0 | 462.6 | |
| 0.00 | 0.51 | 0.00 | 0.49 | 17.58 | 218.33 | -57.73 | 70.58 | 0.8568 | 226.0 | 172.8 | |
| 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. | |