SDO HMI 2014-11-03 02:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.05 | 0.00 | 9.31 | -19.63 | 79.97 | -28.36 | 131.70 | 0.5994 | 654.0 | 535.8 | |
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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 | 0.87 | 0.00 | 0.52 | -21.07 | 85.02 | -23.32 | 138.75 | 0.5624 | 682.0 | 532.0 | |
| 0.00 | 0.26 | 0.00 | 0.16 | -20.90 | 84.98 | -23.36 | 138.49 | 0.5611 | 700.0 | 764.7 | |
| 0.00 | 1.30 | 0.00 | 0.75 | -16.64 | 84.96 | -23.38 | 132.63 | 0.5188 | 801.0 | 579.3 | |
| 0.00 | 0.95 | 0.00 | 0.56 | -17.80 | 84.60 | -23.74 | 133.89 | 0.5339 | 694.0 | 528.3 | |
| 0.00 | 1.21 | 0.00 | 0.71 | -18.16 | 84.41 | -23.93 | 134.17 | 0.5394 | 417.0 | 314.1 | |
| 0.00 | 0.95 | 0.00 | 0.58 | -20.57 | 82.02 | -26.32 | 134.77 | 0.5869 | 574.0 | 482.4 | |
| 0.00 | 0.95 | 0.00 | 0.59 | -20.20 | 79.62 | -28.72 | 131.89 | 0.6081 | 741.0 | 601.2 | |
| 0.00 | 1.82 | 0.00 | 1.13 | -20.04 | 79.51 | -28.83 | 131.58 | 0.6079 | 776.0 | 584.3 | |
| 0.00 | 1.73 | 0.00 | 1.09 | -20.47 | 78.43 | -29.90 | 131.15 | 0.6226 | 707.0 | 616.3 | |
| 0.00 | 0.69 | 0.00 | 0.44 | -20.01 | 76.87 | -31.46 | 129.19 | 0.6351 | 582.0 | 457.6 | |
| 0.00 | 1.64 | 0.00 | 1.06 | -20.37 | 76.60 | -31.73 | 129.44 | 0.6407 | 656.0 | 557.5 | |
| 0.00 | 1.21 | 0.00 | 0.78 | -19.81 | 76.13 | -32.20 | 128.32 | 0.6413 | 760.0 | 565.4 | |
| 0.00 | 0.69 | 0.00 | 0.44 | -19.58 | 76.11 | -32.22 | 128.00 | 0.6399 | 495.0 | 416.9 | |
| 0.00 | 0.78 | 0.00 | 0.50 | -19.72 | 75.85 | -32.48 | 127.98 | 0.6436 | 571.0 | 510.1 | |
| 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. | |