SDO HMI 2014-11-06 20:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.04 | 142.64 | 28.00 | 134.04 | 13.20 | 117.05 | 58.15 | 283.14 | 0.8509 | -499.0 | -226.0 | |
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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 |
| 23.30 | 120.29 | 22.42 | 115.73 | 13.94 | 117.87 | 58.97 | 283.99 | 0.8591 | -788.4 | -242.5 | |
| 1.04 | 16.22 | 0.86 | 13.43 | 7.72 | 112.43 | 53.53 | 276.80 | 0.8048 | -486.4 | -437.0 | |
| 4.06 | -2.00 | 3.37 | -2.00 | 8.11 | 112.41 | 53.51 | 277.29 | 0.8046 | -575.7 | 999999 | |
| 1.64 | -2.00 | 1.35 | -2.00 | 7.95 | 112.12 | 53.22 | 277.09 | 0.8016 | -675.7 | 999999 | |
| 0.00 | 0.69 | 0.00 | 0.57 | 11.91 | 112.36 | 53.45 | 282.01 | 0.8059 | 524.0 | 459.6 | |
| 0.00 | 1.04 | 0.00 | 0.83 | 8.34 | 110.90 | 52.00 | 277.62 | 0.7889 | 79.0 | 89.6 | |
| 0.00 | 0.60 | 0.00 | 0.48 | 8.39 | 110.57 | 51.67 | 277.70 | 0.7854 | 577.0 | 535.3 | |
| 0.00 | 1.12 | 0.00 | 0.89 | 11.07 | 110.43 | 51.53 | 281.13 | 0.7853 | 570.0 | 448.9 | |
| 0.00 | 1.21 | 0.00 | 0.94 | 8.05 | 109.59 | 50.69 | 277.30 | 0.7747 | 604.0 | 543.6 | |
| 0.00 | 0.78 | 0.00 | 0.62 | 11.20 | 110.26 | 51.36 | 281.30 | 0.7837 | 591.0 | 536.2 | |
| 0.00 | 0.69 | 0.00 | 0.55 | 10.79 | 110.11 | 51.21 | 280.79 | 0.7818 | 536.0 | 471.8 | |
| 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. | |