SDO HMI 2011-11-26 00:58:57 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 45.54 | 69.61 | 24.68 | 37.66 | 18.05 | 214.26 | -17.30 | 44.71 | 0.4036 | 506.1 | 201.2 | |
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back to the solar disc SDO HMI 2011-11-26 00:58:57 UT
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 | 1.03 | 0.00 | 0.54 | 18.05 | 218.48 | -13.07 | 37.10 | 0.3581 | 755.0 | 640.0 | |
| 0.00 | 2.57 | 0.00 | 1.36 | 17.56 | 217.82 | -13.74 | 39.35 | 0.3586 | 855.0 | 694.5 | |
| 0.00 | 0.86 | 0.00 | 0.46 | 18.51 | 217.48 | -14.07 | 38.28 | 0.3738 | 844.0 | 660.4 | |
| 0.00 | 0.77 | 0.00 | 0.41 | 16.33 | 217.56 | -14.00 | 42.26 | 0.3467 | 802.0 | 707.9 | |
| 9.33 | 10.53 | 4.97 | 5.61 | 17.11 | 216.19 | -15.37 | 43.29 | 0.3710 | -978.8 | -738.8 | |
| 0.00 | 2.40 | 0.00 | 1.31 | 21.71 | 215.63 | -15.92 | 36.43 | 0.4310 | 836.0 | 605.5 | |
| 0.00 | 1.20 | 0.00 | 0.65 | 19.15 | 215.58 | -15.98 | 40.64 | 0.4010 | 818.0 | 590.8 | |
| 0.00 | 2.91 | 0.00 | 1.60 | 21.68 | 215.27 | -16.28 | 37.07 | 0.4340 | 854.0 | 668.5 | |
| 0.00 | 1.88 | 0.00 | 1.01 | 17.26 | 215.63 | -15.93 | 43.99 | 0.3790 | -779.0 | -667.6 | |
| 0.00 | 0.77 | 0.00 | 0.41 | 17.54 | 215.47 | -16.08 | 43.73 | 0.3838 | -607.0 | -537.0 | |
| 1.46 | 4.54 | 0.78 | 2.44 | 18.06 | 215.20 | -16.36 | 43.22 | 0.3927 | -990.0 | -728.8 | |
| 0.00 | 1.63 | 0.00 | 0.88 | 18.03 | 214.84 | -16.71 | 43.87 | 0.3962 | -839.0 | -651.9 | |
| 34.75 | 38.52 | 18.93 | 20.98 | 17.86 | 212.84 | -18.72 | 47.31 | 0.4174 | 1038.1 | 793.4 | |
| 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. | |