SDO HMI 2014-01-13 22:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.10 | 19.08 | 0.59 | 10.24 | 16.55 | 26.77 | 7.40 | 341.09 | 0.3817 | 114.5 | -21.2 | |
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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 |
| 1.10 | 5.01 | 0.59 | 2.69 | 15.92 | 29.87 | 10.50 | 333.17 | 0.3899 | -985.2 | -815.3 | |
| 0.00 | 1.53 | 0.00 | 0.82 | 16.15 | 28.61 | 9.23 | 336.26 | 0.3846 | -752.0 | -552.9 | |
| 0.00 | 0.93 | 0.00 | 0.51 | 17.83 | 28.32 | 8.94 | 338.61 | 0.4075 | -633.0 | -564.6 | |
| 0.00 | 0.76 | 0.00 | 0.41 | 16.68 | 27.95 | 8.58 | 338.32 | 0.3883 | -748.0 | -651.9 | |
| 0.00 | 1.02 | 0.00 | 0.54 | 15.38 | 26.38 | 7.01 | 340.83 | 0.3596 | -888.0 | -663.3 | |
| 0.00 | 0.93 | 0.00 | 0.50 | 15.56 | 26.11 | 6.73 | 341.68 | 0.3611 | -722.0 | -565.5 | |
| 0.00 | 0.59 | 0.00 | 0.33 | 20.22 | 26.07 | 6.70 | 345.27 | 0.4324 | 714.0 | 628.9 | |
| 0.00 | 1.95 | 0.00 | 1.05 | 17.45 | 25.62 | 6.24 | 344.42 | 0.3881 | 1011.0 | 793.6 | |
| 0.00 | 0.76 | 0.00 | 0.41 | 18.35 | 25.56 | 6.18 | 345.19 | 0.4016 | 769.0 | 650.0 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 16.03 | 25.42 | 6.04 | 343.84 | 0.3650 | 819.0 | 672.1 | |
| 0.00 | 1.87 | 0.00 | 1.00 | 17.19 | 24.65 | 5.27 | 346.58 | 0.3801 | 792.0 | 535.0 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 15.92 | 22.80 | 3.42 | 350.62 | 0.3538 | 883.0 | 677.4 | |
| 0.00 | 1.19 | 0.00 | 0.63 | 16.01 | 22.12 | 2.75 | 352.48 | 0.3537 | 778.0 | 633.9 | |
| 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. | |