SDO HMI 2014-11-09 07:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.25 | 60.30 | 22.49 | 203.78 | -11.19 | 306.09 | -80.40 | 101.90 | 0.9888 | -188.3 | -358.6 | |
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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 | 0.26 | 0.00 | 0.37 | -11.50 | 317.89 | -68.60 | 103.61 | 0.9402 | 372.0 | 364.7 | |
| 1.90 | 3.80 | 3.98 | 7.95 | -11.62 | 311.26 | -75.23 | 102.87 | 0.9726 | 147.0 | 51.1 | |
| 0.00 | 1.21 | 0.00 | 2.97 | -12.45 | 309.21 | -77.27 | 103.48 | 0.9804 | -18.0 | -19.0 | |
| 0.60 | 2.16 | 1.75 | 6.24 | -13.26 | 307.56 | -78.93 | 104.12 | 0.9858 | 32.0 | -47.3 | |
| 0.00 | 1.81 | 0.00 | 4.51 | -11.70 | 308.95 | -77.53 | 102.69 | 0.9810 | -159.0 | -134.3 | |
| 0.00 | 2.33 | 0.00 | 7.71 | -13.46 | 306.24 | -80.24 | 104.19 | 0.9893 | -466.0 | -410.2 | |
| 0.00 | 2.67 | 0.00 | 8.49 | -13.17 | 306.47 | -80.02 | 103.92 | 0.9887 | -404.0 | -358.8 | |
| 0.00 | 5.09 | 0.00 | 17.89 | -12.15 | 305.61 | -80.88 | 102.81 | 0.9905 | -499.0 | -478.0 | |
| 1.81 | 32.86 | 6.09 | 115.12 | -11.03 | 305.90 | -80.59 | 101.71 | 0.9896 | -546.4 | -450.9 | |
| 0.52 | -9.00 | 1.66 | -9.00 | -10.68 | 306.12 | -80.36 | 101.38 | 0.9889 | -551.8 | 999999 | |
| 0.00 | 0.78 | 0.00 | 3.07 | -10.20 | 304.47 | -82.01 | 100.76 | 0.9927 | -168.0 | -185.4 | |
| 0.00 | 0.60 | 0.00 | 2.75 | -10.69 | 303.52 | -82.96 | 101.17 | 0.9946 | -41.0 | -57.6 | |
| 2.42 | 5.26 | 9.01 | 19.70 | -9.51 | 304.91 | -81.58 | 100.10 | 0.9916 | -112.8 | -112.4 | |
| 0.00 | 1.47 | 0.00 | 7.01 | -9.92 | 303.16 | -83.33 | 100.37 | 0.9951 | 74.0 | 89.9 | |
| 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. | |