SDO HMI 2011-10-10 04:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 35.59 | 69.88 | 19.04 | 37.47 | 20.76 | 111.35 | -17.76 | 48.20 | 0.3852 | 92.7 | 322.4 | |
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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 | 2.28 | 0.00 | 1.25 | 26.33 | 112.99 | -16.13 | 35.63 | 0.4292 | 641.0 | 445.7 | |
| 0.00 | 2.54 | 0.00 | 1.37 | 22.16 | 111.97 | -17.14 | 44.39 | 0.3919 | 847.0 | 589.8 | |
| 0.00 | 1.58 | 0.00 | 0.85 | 22.50 | 111.76 | -17.36 | 44.08 | 0.3979 | 859.0 | 741.2 | |
| 16.66 | 20.78 | 8.87 | 11.07 | 20.02 | 112.03 | -17.09 | 48.67 | 0.3693 | -980.0 | -434.0 | |
| 0.00 | 1.23 | 0.00 | 0.67 | 24.53 | 111.24 | -17.88 | 41.24 | 0.4255 | 777.0 | 663.7 | |
| 0.00 | 1.67 | 0.00 | 0.90 | 23.08 | 111.17 | -17.94 | 43.90 | 0.4105 | 874.0 | 731.2 | |
| 0.00 | 0.79 | 0.00 | 0.42 | 20.77 | 111.27 | -17.85 | 48.24 | 0.3858 | 725.0 | 536.3 | |
| 3.51 | 4.56 | 1.87 | 2.44 | 19.91 | 111.34 | -17.78 | 49.96 | 0.3766 | -825.5 | -695.4 | |
| 2.63 | 31.47 | 1.41 | 16.90 | 20.49 | 111.17 | -17.95 | 48.97 | 0.3843 | 1036.9 | 492.7 | |
| 0.00 | 1.93 | 0.00 | 1.03 | 19.62 | 111.00 | -18.11 | 51.07 | 0.3781 | -792.0 | -542.8 | |
| 9.20 | -9.00 | 4.95 | -9.00 | 20.60 | 110.85 | -18.26 | 49.20 | 0.3892 | 999.0 | 999999 | |
| 3.59 | -9.00 | 1.94 | -9.00 | 20.62 | 110.48 | -18.64 | 49.69 | 0.3940 | 863.0 | 999999 | |
| 0.00 | 1.05 | 0.00 | 0.57 | 20.04 | 109.64 | -19.48 | 52.04 | 0.3990 | 731.0 | 488.8 | |
| 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. | |