SDO HMI 2011-11-01 10:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 19.65 | 119.46 | 45.72 | 275.51 | -13.57 | 119.73 | -75.94 | 104.98 | 0.9764 | 145.6 | 74.7 | |
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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 |
| 1.13 | 66.74 | 2.24 | 130.78 | -15.56 | 121.88 | -73.79 | 107.29 | 0.9699 | 315.3 | 138.1 | |
| 2.25 | -1.00 | 4.44 | -1.00 | -15.34 | 121.99 | -73.68 | 107.08 | 0.9694 | 414.5 | 999999 | |
| 5.11 | -1.00 | 9.76 | -1.00 | -14.68 | 122.48 | -73.19 | 106.48 | 0.9669 | 565.0 | 999999 | |
| 2.16 | -1.00 | 4.26 | -1.00 | -14.96 | 122.01 | -73.66 | 106.70 | 0.9690 | 247.0 | 999999 | |
| 0.00 | 1.38 | 0.00 | 2.87 | -15.23 | 121.29 | -74.38 | 106.87 | 0.9721 | -469.0 | -432.7 | |
| 0.00 | 1.13 | 0.00 | 2.98 | -17.33 | 118.43 | -77.24 | 108.59 | 0.9831 | -111.0 | -84.1 | |
| 0.00 | 0.87 | 0.00 | 1.83 | -14.51 | 120.93 | -74.74 | 106.08 | 0.9730 | -254.0 | -301.7 | |
| 0.00 | 1.47 | 0.00 | 3.88 | -15.59 | 118.16 | -77.51 | 106.80 | 0.9832 | -375.0 | -321.5 | |
| 3.12 | 5.80 | 9.26 | 17.40 | -15.81 | 116.93 | -78.74 | 106.86 | 0.9868 | -260.5 | -223.0 | |
| 0.00 | 5.11 | 0.00 | 14.68 | -15.33 | 117.14 | -78.53 | 106.40 | 0.9860 | -28.0 | -15.1 | |
| 4.24 | 35.40 | 11.24 | 96.53 | -10.91 | 117.60 | -78.07 | 102.00 | 0.9830 | 240.0 | 89.6 | |
| 1.64 | -11.00 | 4.52 | -11.00 | -10.98 | 117.07 | -78.60 | 102.01 | 0.9847 | -152.4 | 999999 | |
| 0.00 | 1.56 | 0.00 | 4.56 | -9.36 | 116.33 | -79.34 | 100.29 | 0.9863 | 55.0 | 13.3 | |
| 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. | |