SDO HMI 2014-11-06 12:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.00 | 0.00 | 9.82 | -22.48 | 76.73 | 13.42 | 205.48 | 0.5134 | 207.8 | 252.8 | |
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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 | 1.47 | 0.00 | 0.95 | -28.28 | 88.77 | 25.46 | 215.75 | 0.6502 | -590.0 | -366.2 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -16.22 | 84.99 | 21.68 | 226.37 | 0.4921 | 678.0 | 573.5 | |
| 0.00 | 1.81 | 0.00 | 1.04 | -19.88 | 82.66 | 19.35 | 218.04 | 0.5078 | 847.0 | 718.2 | |
| 0.00 | 1.55 | 0.00 | 0.89 | -20.17 | 82.70 | 19.39 | 217.71 | 0.5115 | 604.0 | 488.5 | |
| 0.00 | 2.24 | 0.00 | 1.29 | -19.71 | 82.47 | 19.16 | 217.99 | 0.5041 | 809.0 | 737.3 | |
| 0.00 | 1.12 | 0.00 | 0.65 | -21.39 | 81.68 | 18.37 | 214.77 | 0.5166 | 731.0 | 585.5 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -20.78 | 76.22 | 12.91 | 206.73 | 0.4663 | 810.0 | 610.3 | |
| 0.00 | 1.21 | 0.00 | 0.68 | -20.98 | 76.17 | 12.86 | 206.44 | 0.4686 | 877.0 | 725.3 | |
| 0.00 | 1.21 | 0.00 | 0.68 | -21.30 | 75.74 | 12.43 | 205.36 | 0.4701 | 752.0 | 557.1 | |
| 0.00 | 0.78 | 0.00 | 0.44 | -25.10 | 65.23 | 1.92 | 183.59 | 0.4865 | -691.0 | -566.9 | |
| 0.00 | 1.47 | 0.00 | 0.83 | -25.58 | 65.01 | 1.70 | 183.12 | 0.4936 | -597.0 | -440.6 | |
| 0.00 | 1.21 | 0.00 | 0.70 | -27.51 | 58.63 | -4.68 | 172.07 | 0.5269 | -781.0 | -495.4 | |
| 0.00 | 0.86 | 0.00 | 0.50 | -27.55 | 58.36 | -4.95 | 171.63 | 0.5280 | -747.0 | -544.8 | |
| 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. | |