SDO HMI 2014-07-08 10:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 26.89 | 170.26 | 14.02 | 89.13 | 6.50 | 204.04 | -18.55 | 80.45 | 0.3219 | -590.0 | -367.4 | |
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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 | 1.00 | 0.00 | 0.52 | 10.55 | 206.00 | -16.59 | 66.36 | 0.3078 | -847.0 | -584.7 | |
| 0.00 | 1.82 | 0.00 | 0.95 | 10.77 | 205.76 | -16.83 | 66.01 | 0.3127 | -944.0 | -796.8 | |
| 0.00 | 1.64 | 0.00 | 0.85 | 6.42 | 205.92 | -16.67 | 79.85 | 0.2909 | -956.0 | -810.3 | |
| 2.54 | 7.81 | 1.32 | 4.06 | 7.12 | 205.51 | -17.08 | 77.75 | 0.2995 | -1172.0 | -862.7 | |
| 24.35 | 142.73 | 12.70 | 74.47 | 6.34 | 204.48 | -18.11 | 80.81 | 0.3144 | -1389.5 | -442.6 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 8.60 | 203.05 | -19.54 | 74.79 | 0.3443 | -736.0 | -551.2 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 6.88 | 201.33 | -21.27 | 80.43 | 0.3667 | 735.0 | 686.1 | |
| 0.00 | 1.45 | 0.00 | 0.78 | 7.90 | 200.21 | -22.38 | 78.19 | 0.3869 | 823.0 | 668.5 | |
| 0.00 | 1.82 | 0.00 | 0.98 | 6.12 | 200.00 | -22.59 | 82.84 | 0.3866 | 641.0 | 422.8 | |
| 0.00 | 1.36 | 0.00 | 0.74 | 5.79 | 198.75 | -23.84 | 83.94 | 0.4061 | 638.0 | 523.1 | |
| 0.00 | 2.09 | 0.00 | 1.14 | 5.67 | 197.88 | -24.71 | 84.36 | 0.4198 | 747.0 | 565.3 | |
| 0.00 | 1.00 | 0.00 | 0.55 | 7.99 | 197.62 | -24.97 | 78.96 | 0.4277 | 651.0 | 513.0 | |
| 0.00 | 1.73 | 0.00 | 0.95 | 5.93 | 197.39 | -25.20 | 83.81 | 0.4277 | 811.0 | 580.6 | |
| 0.00 | 2.00 | 0.00 | 1.10 | 6.33 | 197.24 | -25.35 | 82.92 | 0.4306 | 877.0 | 652.4 | |
| 0.00 | 1.36 | 0.00 | 0.75 | 8.83 | 197.05 | -25.54 | 77.24 | 0.4386 | 813.0 | 617.7 | |
| 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. | |