SDO HMI 2014-01-14 08:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 22.46 | 62.17 | 12.31 | 33.96 | 16.26 | 27.74 | 13.83 | 327.09 | 0.4233 | -308.0 | -53.9 | |
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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 | 1.96 | 0.00 | 1.08 | 15.38 | 30.38 | 16.48 | 320.90 | 0.4355 | -601.0 | -462.2 | |
| 1.45 | 18.96 | 0.80 | 10.44 | 16.13 | 30.19 | 16.28 | 322.33 | 0.4426 | -717.1 | -675.9 | |
| 9.01 | -2.00 | 4.96 | -2.00 | 15.99 | 29.92 | 16.02 | 322.59 | 0.4385 | -1085.6 | 999999 | |
| 0.00 | 3.06 | 0.00 | 1.68 | 15.98 | 29.32 | 15.41 | 323.63 | 0.4326 | -949.0 | -728.8 | |
| 4.08 | 15.39 | 2.23 | 8.42 | 15.96 | 28.52 | 14.62 | 325.03 | 0.4251 | -1123.1 | -795.4 | |
| 5.19 | -5.00 | 2.84 | -5.00 | 16.34 | 28.39 | 14.49 | 325.79 | 0.4287 | -1039.9 | 999999 | |
| 0.00 | 3.15 | 0.00 | 1.71 | 16.55 | 25.97 | 12.07 | 330.70 | 0.4113 | 839.0 | 592.8 | |
| 1.62 | 9.18 | 0.88 | 5.00 | 16.90 | 25.87 | 11.96 | 331.34 | 0.4153 | 949.8 | 386.0 | |
| 1.11 | 2.64 | 0.60 | 1.43 | 16.82 | 25.05 | 11.14 | 332.92 | 0.4081 | 971.8 | 775.7 | |
| 0.00 | 1.02 | 0.00 | 0.55 | 17.26 | 24.60 | 10.70 | 334.34 | 0.4112 | 699.0 | 557.8 | |
| 0.00 | 2.13 | 0.00 | 1.15 | 16.37 | 24.49 | 10.58 | 333.58 | 0.3977 | 942.0 | 756.4 | |
| 0.00 | 1.19 | 0.00 | 0.64 | 16.22 | 22.86 | 8.95 | 337.03 | 0.3846 | 811.0 | 680.5 | |
| 0.00 | 1.45 | 0.00 | 0.77 | 15.87 | 22.63 | 8.72 | 337.20 | 0.3780 | 1116.0 | 945.9 | |
| 0.00 | 2.04 | 0.00 | 1.09 | 16.15 | 22.27 | 8.36 | 338.34 | 0.3800 | 885.0 | 729.3 | |
| 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. | |