SDO HMI 2011-01-01 11:58:55 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 54.71 | 198.86 | 35.97 | 130.89 | 34.09 | 267.41 | 18.61 | 336.30 | 0.6603 | -122.0 | 20.5 | |
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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 |
| 20.90 | 99.73 | 13.84 | 66.11 | 33.45 | 269.92 | 21.13 | 333.05 | 0.6660 | -1047.8 | -270.2 | |
| 2.38 | 3.06 | 1.56 | 2.01 | 33.42 | 268.67 | 19.87 | 334.38 | 0.6585 | -822.7 | -756.9 | |
| 4.67 | 8.50 | 3.07 | 5.59 | 33.67 | 268.43 | 19.63 | 334.84 | 0.6600 | -810.3 | -511.7 | |
| 0.00 | 0.93 | 0.00 | 0.61 | 33.11 | 267.74 | 18.94 | 335.16 | 0.6497 | -656.0 | -595.0 | |
| 1.95 | 2.63 | 1.29 | 1.73 | 34.49 | 266.78 | 17.98 | 337.26 | 0.6606 | -627.8 | -548.8 | |
| 0.00 | 1.19 | 0.00 | 0.79 | 34.79 | 266.85 | 18.05 | 337.40 | 0.6644 | -497.0 | -396.6 | |
| 0.00 | 4.84 | 0.00 | 3.16 | 34.72 | 264.73 | 15.93 | 339.73 | 0.6533 | 750.0 | 586.6 | |
| 1.36 | 31.43 | 0.89 | 20.67 | 35.32 | 264.81 | 16.01 | 340.02 | 0.6609 | 657.3 | 482.4 | |
| 0.00 | 2.80 | 0.00 | 1.79 | 33.20 | 264.40 | 15.60 | 339.11 | 0.6333 | 870.0 | 713.3 | |
| 5.69 | -8.00 | 3.75 | -8.00 | 35.54 | 264.52 | 15.72 | 340.49 | 0.6623 | 613.7 | 999999 | |
| 5.10 | -8.00 | 3.34 | -8.00 | 35.20 | 264.41 | 15.61 | 340.39 | 0.6577 | 835.9 | 999999 | |
| 2.38 | 43.75 | 1.54 | 28.43 | 34.37 | 263.99 | 15.19 | 340.36 | 0.6458 | 943.6 | 463.8 | |
| 10.28 | -12.00 | 6.69 | -12.00 | 34.82 | 263.89 | 15.09 | 340.75 | 0.6508 | 987.4 | 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. | |