SDO HMI 2014-11-10 10:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.42 | 0.00 | 10.88 | -15.97 | 18.71 | 7.05 | 199.61 | 0.3637 | -65.1 | -70.8 | |
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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 | 0.95 | 0.00 | 0.51 | -12.36 | 26.74 | 15.07 | 223.31 | 0.3719 | 795.0 | 638.5 | |
| 0.00 | 1.03 | 0.00 | 0.56 | -15.53 | 24.44 | 12.77 | 213.42 | 0.3884 | 674.0 | 481.6 | |
| 0.00 | 0.60 | 0.00 | 0.32 | -13.77 | 23.55 | 11.89 | 214.26 | 0.3570 | 746.0 | 646.7 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -14.42 | 23.43 | 11.77 | 212.96 | 0.3646 | 805.0 | 695.2 | |
| 0.00 | 2.15 | 0.00 | 1.14 | -14.33 | 23.36 | 11.70 | 212.95 | 0.3628 | 728.0 | 495.2 | |
| 0.00 | 1.90 | 0.00 | 1.00 | -13.85 | 22.62 | 10.96 | 212.00 | 0.3498 | 799.0 | 642.2 | |
| 0.00 | 1.55 | 0.00 | 0.82 | -13.47 | 21.64 | 9.98 | 210.24 | 0.3361 | 778.0 | 649.7 | |
| 0.00 | 1.90 | 0.00 | 1.01 | -16.80 | 17.07 | 5.41 | 194.66 | 0.3581 | -833.0 | -600.8 | |
| 0.00 | 1.38 | 0.00 | 0.73 | -17.15 | 16.96 | 5.29 | 194.11 | 0.3631 | -610.0 | -529.9 | |
| 0.00 | 1.47 | 0.00 | 0.78 | -16.90 | 16.70 | 5.04 | 193.63 | 0.3581 | -967.0 | -753.0 | |
| 0.00 | 2.24 | 0.00 | 1.20 | -18.58 | 16.40 | 4.74 | 191.82 | 0.3837 | -753.0 | -569.1 | |
| 0.00 | 1.03 | 0.00 | 0.56 | -19.09 | 15.15 | 3.49 | 188.56 | 0.3882 | -666.0 | -577.3 | |
| 0.00 | 1.21 | 0.00 | 0.65 | -18.64 | 14.80 | 3.14 | 187.87 | 0.3801 | -769.0 | -548.8 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -16.53 | 8.04 | -3.62 | 169.92 | 0.3474 | -927.0 | -779.9 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -16.60 | 7.89 | -3.78 | 169.53 | 0.3489 | -776.0 | -651.3 | |
| 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. | |