SDO HMI 2014-10-10 20:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 60.60 | 401.48 | 42.39 | 281.00 | -20.53 | 18.33 | -36.66 | 127.53 | 0.7075 | 1065.7 | 299.6 | |
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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 | 1.31 | 0.00 | 0.88 | -18.96 | 20.61 | -34.38 | 127.32 | 0.6739 | 799.0 | 713.2 | |
| 0.00 | 1.75 | 0.00 | 1.17 | -18.72 | 20.32 | -34.67 | 126.79 | 0.6751 | 767.0 | 650.3 | |
| 0.70 | 390.62 | 0.48 | 273.62 | -20.51 | 19.75 | -35.24 | 128.55 | 0.6934 | 932.2 | 292.6 | |
| 0.00 | 1.05 | 0.00 | 0.71 | -18.95 | 19.76 | -35.23 | 126.66 | 0.6825 | 783.0 | 644.0 | |
| 2.54 | -3.00 | 1.75 | -3.00 | -20.34 | 19.21 | -35.79 | 127.95 | 0.6976 | 1163.8 | 999999 | |
| 1.49 | -3.00 | 1.03 | -3.00 | -20.59 | 19.02 | -35.97 | 128.11 | 0.7011 | 1070.4 | 999999 | |
| 0.00 | 3.50 | 0.00 | 2.35 | -17.65 | 19.56 | -35.43 | 124.89 | 0.6757 | 885.0 | 733.6 | |
| 55.87 | -3.00 | 39.13 | -3.00 | -20.61 | 18.22 | -36.77 | 127.55 | 0.7091 | 1165.5 | 999999 | |
| 0.00 | 1.23 | 0.00 | 0.83 | -17.19 | 18.78 | -36.21 | 123.73 | 0.6810 | 289.0 | 307.6 | |
| 0.00 | 1.23 | 0.00 | 0.84 | -17.61 | 18.21 | -36.78 | 123.87 | 0.6897 | 427.0 | 307.4 | |
| 0.00 | 0.79 | 0.00 | 0.60 | -17.66 | 11.26 | -43.73 | 119.71 | 0.7607 | -376.0 | -403.2 | |
| 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. | |