SDO HMI 2014-11-20 20:00:26 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 78.64 | 669.58 | 119.35 | 1055.24 | -13.36 | 164.58 | -69.75 | 104.97 | 0.9452 | 243.7 | -185.5 | |
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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 | 0.86 | 0.00 | 0.97 | -17.21 | 172.35 | -61.98 | 110.35 | 0.9013 | 449.0 | 435.1 | |
| 0.00 | 1.80 | 0.00 | 1.97 | -11.39 | 172.36 | -61.97 | 103.95 | 0.8935 | 186.0 | 144.3 | |
| 0.00 | 0.60 | 0.00 | 0.89 | -14.86 | 165.20 | -69.14 | 106.61 | 0.9440 | -332.0 | -299.6 | |
| 59.60 | 653.37 | 83.20 | 1025.13 | -12.97 | 166.32 | -68.01 | 104.77 | 0.9360 | 523.3 | -191.4 | |
| 0.00 | 0.43 | 0.00 | 0.63 | -11.50 | 164.96 | -69.37 | 103.04 | 0.9429 | -423.0 | -375.4 | |
| 6.09 | -4.00 | 10.94 | -4.00 | -14.01 | 161.45 | -72.88 | 105.25 | 0.9624 | -598.5 | 999999 | |
| 8.32 | -4.00 | 16.03 | -4.00 | -14.64 | 160.36 | -73.98 | 105.77 | 0.9675 | -241.8 | 999999 | |
| 0.00 | 2.57 | 0.00 | 4.86 | -13.98 | 160.61 | -73.72 | 105.13 | 0.9661 | -515.0 | -394.0 | |
| 1.46 | -4.00 | 2.85 | -4.00 | -14.22 | 160.06 | -74.27 | 105.31 | 0.9686 | 81.9 | 999999 | |
| 0.00 | 2.66 | 0.00 | 5.19 | -13.85 | 160.05 | -74.28 | 104.93 | 0.9684 | -123.0 | -72.1 | |
| 2.14 | -4.00 | 4.10 | -4.00 | -13.44 | 160.30 | -74.04 | 104.54 | 0.9672 | -478.0 | 999999 | |
| 0.00 | 4.20 | 0.00 | 8.90 | -14.50 | 158.95 | -75.38 | 105.49 | 0.9732 | 396.0 | 261.2 | |
| 1.03 | 3.09 | 2.23 | 6.70 | -14.15 | 158.56 | -75.78 | 105.09 | 0.9745 | -108.1 | -23.2 | |
| 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. | |