SDO HMI 2014-10-05 22:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 2.28 | 18.16 | 1.65 | 13.41 | -18.16 | 78.36 | -41.49 | 121.79 | 0.7431 | 538.4 | 456.7 | |
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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 | 1.14 | 0.00 | 0.83 | -21.19 | 80.92 | -38.94 | 126.98 | 0.7358 | 84.0 | 83.2 | |
| 0.00 | 1.14 | 0.00 | 0.84 | -20.07 | 79.85 | -40.00 | 124.97 | 0.7391 | 627.0 | 551.8 | |
| 0.00 | 1.05 | 0.00 | 0.78 | -20.46 | 79.56 | -40.29 | 125.24 | 0.7442 | 543.0 | 409.3 | |
| 2.28 | 4.92 | 1.65 | 3.55 | -18.21 | 79.66 | -40.20 | 122.62 | 0.7303 | 826.2 | 652.1 | |
| 0.00 | 1.05 | 0.00 | 0.76 | -18.06 | 79.41 | -40.45 | 122.29 | 0.7320 | 647.0 | 573.3 | |
| 0.00 | 1.32 | 0.00 | 0.93 | -15.36 | 79.57 | -40.28 | 119.05 | 0.7155 | 726.0 | 646.8 | |
| 0.00 | 0.70 | 0.00 | 0.49 | -12.33 | 78.87 | -40.98 | 114.76 | 0.7079 | 572.0 | 488.1 | |
| 0.00 | 1.05 | 0.00 | 0.81 | -19.97 | 76.55 | -43.31 | 122.87 | 0.7699 | 396.0 | 262.6 | |
| 0.00 | 2.46 | 0.00 | 1.84 | -16.86 | 76.83 | -43.02 | 119.36 | 0.7515 | 680.0 | 519.9 | |
| 0.00 | 2.37 | 0.00 | 1.85 | -19.56 | 75.89 | -43.96 | 122.03 | 0.7739 | 209.0 | 279.6 | |
| 0.00 | 0.26 | 0.00 | 0.20 | -16.82 | 76.15 | -43.70 | 118.94 | 0.7580 | 523.0 | 517.7 | |
| 0.00 | 0.70 | 0.00 | 0.53 | -14.51 | 74.96 | -44.89 | 115.54 | 0.7596 | 440.0 | 402.2 | |
| 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. | |