SDO HMI 2014-10-04 19:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.44 | 0.00 | 10.48 | -19.88 | 106.25 | -28.46 | 134.34 | 0.6289 | 278.8 | 197.4 | |
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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 | 1.76 | 0.00 | 1.08 | -22.68 | 113.33 | -21.37 | 145.05 | 0.5891 | 758.0 | 531.5 | |
| 0.00 | 2.11 | 0.00 | 1.30 | -22.70 | 112.21 | -22.50 | 143.70 | 0.5985 | 717.0 | 507.5 | |
| 0.00 | 0.88 | 0.00 | 0.54 | -22.56 | 111.56 | -23.14 | 142.79 | 0.6023 | 530.0 | 475.6 | |
| 0.00 | 1.05 | 0.00 | 0.66 | -22.41 | 110.42 | -24.28 | 141.31 | 0.6105 | 710.0 | 512.3 | |
| 0.00 | 0.97 | 0.00 | 0.63 | -24.84 | 107.54 | -27.17 | 140.87 | 0.6589 | 562.0 | 501.5 | |
| 0.00 | 0.44 | 0.00 | 0.27 | -16.94 | 108.46 | -26.24 | 132.47 | 0.5757 | 313.0 | 372.6 | |
| 0.00 | 1.41 | 0.00 | 0.85 | -16.82 | 108.24 | -26.47 | 132.07 | 0.5770 | 759.0 | 538.9 | |
| 0.00 | 1.41 | 0.00 | 0.84 | -15.10 | 108.24 | -26.46 | 129.71 | 0.5615 | 711.0 | 582.9 | |
| 0.00 | 0.35 | 0.00 | 0.22 | -18.25 | 107.30 | -27.41 | 132.96 | 0.5996 | 634.0 | 592.5 | |
| 0.00 | 1.32 | 0.00 | 0.88 | -23.20 | 104.64 | -30.06 | 136.32 | 0.6690 | 555.0 | 472.9 | |
| 0.00 | 1.05 | 0.00 | 0.71 | -17.25 | 99.05 | -35.65 | 124.53 | 0.6780 | -468.0 | -551.2 | |
| 0.00 | 1.05 | 0.00 | 0.71 | -17.52 | 98.91 | -35.79 | 124.77 | 0.6813 | -735.0 | -547.8 | |
| 0.00 | 1.67 | 0.00 | 1.13 | -17.53 | 98.72 | -35.99 | 124.65 | 0.6834 | -614.0 | -561.1 | |
| 0.00 | 0.97 | 0.00 | 0.66 | -17.03 | 97.50 | -37.21 | 123.16 | 0.6930 | -529.0 | -384.8 | |
| 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. | |