SDO HMI 2014-07-13 15:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 10.25 | 32.41 | 8.48 | 26.03 | 6.04 | 205.71 | 52.04 | 274.41 | 0.7878 | -213.2 | -234.3 | |
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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 |
| 0.54 | 2.18 | 0.46 | 1.86 | 5.08 | 208.33 | 54.66 | 273.28 | 0.8161 | -398.5 | -322.6 | |
| 2.45 | 4.18 | 2.07 | 3.53 | 5.32 | 207.93 | 54.27 | 273.56 | 0.8120 | -490.0 | -434.2 | |
| 1.27 | 2.91 | 1.05 | 2.39 | 6.06 | 206.89 | 53.23 | 274.45 | 0.8012 | -459.1 | -401.1 | |
| 5.99 | 8.62 | 4.90 | 7.05 | 6.20 | 206.60 | 52.94 | 274.62 | 0.7981 | -691.6 | -546.2 | |
| 0.00 | 1.45 | 0.00 | 1.20 | 9.73 | 207.07 | 53.40 | 279.04 | 0.8035 | -136.0 | -270.1 | |
| 0.00 | 5.08 | 0.00 | 4.08 | 5.85 | 205.69 | 52.03 | 274.18 | 0.7885 | -656.0 | -538.6 | |
| 0.00 | 1.00 | 0.00 | 0.80 | 4.09 | 205.49 | 51.83 | 271.93 | 0.7868 | 214.0 | 252.0 | |
| 0.00 | 1.63 | 0.00 | 1.29 | 6.33 | 204.81 | 51.15 | 274.78 | 0.7790 | -544.0 | -406.5 | |
| 0.00 | 0.82 | 0.00 | 0.64 | 8.39 | 204.66 | 51.00 | 277.44 | 0.7776 | 215.0 | 258.7 | |
| 0.00 | 0.27 | 0.00 | 0.21 | 9.46 | 204.77 | 51.11 | 278.81 | 0.7792 | 176.0 | 160.0 | |
| 0.00 | 1.18 | 0.00 | 0.88 | 5.60 | 202.00 | 48.34 | 273.79 | 0.7475 | 311.0 | 302.3 | |
| 0.00 | 1.00 | 0.00 | 0.68 | 5.05 | 197.30 | 43.64 | 272.96 | 0.6907 | 445.0 | 372.3 | |
| 0.00 | 1.36 | 0.00 | 0.93 | 5.98 | 197.09 | 43.43 | 274.31 | 0.6880 | 795.0 | 620.7 | |
| 0.00 | 0.73 | 0.00 | 0.49 | 4.98 | 197.00 | 43.34 | 272.84 | 0.6869 | 494.0 | 477.6 | |
| 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. | |