SDO HMI 2014-11-28 23:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.27 | 35.64 | 5.89 | 20.27 | 16.96 | 152.45 | 25.22 | 303.91 | 0.4930 | 275.6 | 134.4 | |
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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 | 1.54 | 0.00 | 0.89 | 17.94 | 154.20 | 26.96 | 303.95 | 0.5222 | 653.0 | 515.0 | |
| 7.87 | 11.63 | 4.55 | 6.73 | 17.60 | 154.07 | 26.84 | 303.49 | 0.5181 | 945.9 | 418.8 | |
| 0.77 | 1.62 | 0.43 | 0.92 | 15.59 | 152.37 | 25.13 | 301.50 | 0.4818 | 756.7 | 607.3 | |
| 0.43 | 7.52 | 0.24 | 4.23 | 15.41 | 152.14 | 24.91 | 301.38 | 0.4775 | 818.2 | 602.7 | |
| 0.00 | 1.71 | 0.00 | 0.97 | 16.81 | 152.23 | 25.00 | 303.86 | 0.4891 | 821.0 | 601.5 | |
| 0.00 | 1.45 | 0.00 | 0.82 | 16.88 | 151.93 | 24.70 | 304.26 | 0.4858 | 745.0 | 581.8 | |
| 0.00 | 1.37 | 0.00 | 0.77 | 17.50 | 151.41 | 24.17 | 305.90 | 0.4842 | -488.0 | -397.4 | |
| 0.00 | 1.03 | 0.00 | 0.58 | 17.57 | 150.71 | 23.47 | 306.77 | 0.4760 | -751.0 | -638.9 | |
| 0.00 | 1.11 | 0.00 | 0.62 | 16.25 | 150.43 | 23.20 | 304.67 | 0.4617 | -879.0 | -796.2 | |
| 0.00 | 1.45 | 0.00 | 0.81 | 16.80 | 150.50 | 23.27 | 305.61 | 0.4671 | -664.0 | -582.0 | |
| 0.00 | 2.05 | 0.00 | 1.15 | 17.42 | 150.52 | 23.28 | 306.71 | 0.4724 | -834.0 | -669.0 | |
| 1.20 | 3.16 | 0.67 | 1.78 | 18.10 | 150.44 | 23.21 | 307.99 | 0.4773 | -931.1 | -711.0 | |
| 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. | |