SDO HMI 2011-06-03 22:59:10 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.61 | 30.48 | 3.13 | 16.64 | 17.29 | 41.81 | 17.25 | 317.86 | 0.4191 | -109.3 | 75.2 | |
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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 |
| 0.00 | 2.44 | 0.00 | 1.36 | 14.94 | 47.69 | 23.13 | 304.78 | 0.4639 | 519.0 | 592.7 | |
| 3.89 | 10.12 | 2.17 | 5.66 | 17.98 | 45.45 | 20.89 | 312.85 | 0.4644 | -919.1 | -776.9 | |
| 1.72 | -2.00 | 0.96 | -2.00 | 18.08 | 45.19 | 20.63 | 313.35 | 0.4624 | -784.5 | 999999 | |
| 0.00 | 1.63 | 0.00 | 0.91 | 18.69 | 44.44 | 19.88 | 315.36 | 0.4603 | -697.0 | -658.9 | |
| 0.00 | 1.45 | 0.00 | 0.79 | 16.51 | 44.09 | 19.53 | 312.15 | 0.4341 | -911.0 | -747.1 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 17.95 | 43.41 | 18.84 | 315.62 | 0.4411 | -847.0 | -705.1 | |
| 0.00 | 1.27 | 0.00 | 0.70 | 18.36 | 43.11 | 18.55 | 316.74 | 0.4424 | -826.0 | -667.6 | |
| 0.00 | 2.26 | 0.00 | 1.21 | 16.82 | 38.16 | 13.59 | 322.70 | 0.3729 | 875.0 | 648.2 | |
| 0.00 | 3.34 | 0.00 | 1.78 | 16.82 | 37.34 | 12.78 | 324.37 | 0.3650 | 833.0 | 699.8 | |
| 0.00 | 1.90 | 0.00 | 1.00 | 16.62 | 35.70 | 11.14 | 327.64 | 0.3474 | 855.0 | 668.4 | |
| 0.00 | 1.36 | 0.00 | 0.72 | 18.38 | 35.78 | 11.22 | 330.12 | 0.3722 | 847.0 | 646.6 | |
| 0.00 | 3.44 | 0.00 | 1.81 | 16.49 | 35.47 | 10.91 | 327.97 | 0.3436 | 664.0 | 637.3 | |
| 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. | |