SDO HMI 2014-11-10 14:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.05 | 0.00 | 10.63 | -23.84 | 8.31 | -1.17 | 178.20 | 0.4619 | 685.6 | 582.2 | |
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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 | 1.98 | 0.00 | 1.08 | -21.12 | 10.42 | 0.95 | 182.14 | 0.4167 | 633.0 | 513.4 | |
| 0.00 | 1.55 | 0.00 | 0.85 | -21.51 | 10.04 | 0.57 | 181.26 | 0.4228 | 856.0 | 706.6 | |
| 0.00 | 0.95 | 0.00 | 0.52 | -22.56 | 10.02 | 0.54 | 181.14 | 0.4394 | 794.0 | 673.6 | |
| 0.00 | 1.12 | 0.00 | 0.62 | -22.53 | 9.79 | 0.32 | 180.67 | 0.4388 | 837.0 | 655.8 | |
| 0.00 | 1.21 | 0.00 | 0.66 | -21.90 | 9.41 | -0.07 | 179.85 | 0.4289 | 858.0 | 704.4 | |
| 0.00 | 1.90 | 0.00 | 1.07 | -25.00 | 9.14 | -0.34 | 179.36 | 0.4773 | 584.0 | 520.9 | |
| 0.00 | 1.38 | 0.00 | 0.77 | -24.09 | 9.11 | -0.36 | 179.28 | 0.4633 | 774.0 | 634.6 | |
| 0.00 | 1.21 | 0.00 | 0.67 | -24.36 | 9.08 | -0.40 | 179.22 | 0.4674 | 855.0 | 770.5 | |
| 0.00 | 2.41 | 0.00 | 1.35 | -24.53 | 8.94 | -0.53 | 178.97 | 0.4701 | 939.0 | 742.1 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -24.83 | 8.94 | -0.53 | 178.98 | 0.4747 | 641.0 | 596.7 | |
| 0.00 | 1.29 | 0.00 | 0.72 | -23.99 | 8.82 | -0.66 | 178.70 | 0.4618 | 835.0 | 721.7 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -24.09 | 8.65 | -0.82 | 178.38 | 0.4634 | 813.0 | 691.0 | |
| 0.00 | 1.12 | 0.00 | 0.62 | -23.89 | 7.84 | -1.63 | 176.75 | 0.4608 | 779.0 | 648.5 | |
| 0.00 | 1.21 | 0.00 | 0.74 | -29.55 | 355.14 | -14.33 | 158.34 | 0.5855 | -600.0 | -402.3 | |
| 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. | |