SDO HMI 2014-11-14 10:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.35 | 38.29 | 8.06 | 26.97 | 8.69 | 4.14 | 45.21 | 279.36 | 0.7131 | -82.7 | -45.5 | |
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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 | 0.43 | 0.00 | 0.32 | 8.67 | 7.31 | 48.38 | 279.00 | 0.7505 | -416.0 | -372.8 | |
| 0.00 | 0.95 | 0.00 | 0.69 | 8.48 | 6.11 | 47.18 | 278.84 | 0.7365 | -444.0 | -331.9 | |
| 7.40 | 10.58 | 5.38 | 7.69 | 8.13 | 5.92 | 46.99 | 278.38 | 0.7341 | -817.5 | -547.8 | |
| 0.00 | 1.29 | 0.00 | 0.94 | 8.49 | 5.84 | 46.91 | 278.88 | 0.7335 | -487.0 | -434.1 | |
| 0.00 | 1.98 | 0.00 | 1.42 | 8.18 | 5.27 | 46.34 | 278.51 | 0.7264 | -837.0 | -651.0 | |
| 0.00 | 0.60 | 0.00 | 0.43 | 8.13 | 5.09 | 46.16 | 278.45 | 0.7242 | -566.0 | -531.3 | |
| 0.00 | 5.68 | 0.00 | 4.04 | 8.14 | 4.83 | 45.90 | 278.49 | 0.7211 | -529.0 | -613.7 | |
| 0.00 | 0.95 | 0.00 | 0.66 | 9.74 | 3.50 | 44.57 | 280.89 | 0.7067 | 636.0 | 544.8 | |
| 0.00 | 1.20 | 0.00 | 0.83 | 9.89 | 2.69 | 43.76 | 281.22 | 0.6969 | 690.0 | 547.6 | |
| 0.00 | 1.38 | 0.00 | 0.94 | 9.90 | 2.48 | 43.55 | 281.26 | 0.6944 | 655.0 | 358.6 | |
| 0.00 | 1.29 | 0.00 | 0.89 | 10.41 | 2.40 | 43.47 | 282.01 | 0.6941 | 607.0 | 452.0 | |
| 0.00 | 0.43 | 0.00 | 0.29 | 10.23 | 2.33 | 43.40 | 281.77 | 0.6930 | 749.0 | 672.2 | |
| 0.00 | 1.81 | 0.00 | 1.23 | 9.52 | 2.12 | 43.20 | 280.77 | 0.6895 | 539.0 | 470.4 | |
| 1.98 | 6.97 | 1.34 | 4.73 | 8.69 | 1.96 | 43.03 | 279.59 | 0.6864 | 817.5 | 644.0 | |
| 1.20 | 2.75 | 0.82 | 1.87 | 9.74 | 1.91 | 42.98 | 281.12 | 0.6872 | 740.9 | 595.6 | |
| 0.77 | -14.00 | 0.52 | -14.00 | 8.67 | 1.75 | 42.82 | 279.58 | 0.6838 | 843.4 | 999999 | |
| 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. | |