SDO HMI 2014-11-02 22:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.91 | 36.85 | 4.77 | 20.12 | -17.13 | 98.41 | -12.13 | 151.99 | 0.4191 | 157.6 | 48.5 | |
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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 |
| 1.99 | 11.16 | 1.06 | 5.94 | -16.27 | 103.58 | -6.96 | 161.60 | 0.3700 | 1076.3 | 848.8 | |
| 3.20 | -1.00 | 1.71 | -1.00 | -16.24 | 103.36 | -7.18 | 161.04 | 0.3707 | 982.2 | 999999 | |
| 0.00 | 1.04 | 0.00 | 0.56 | -16.46 | 100.50 | -10.04 | 154.61 | 0.3915 | 920.0 | 820.2 | |
| 3.72 | 9.17 | 2.00 | 4.94 | -16.50 | 100.12 | -10.42 | 153.82 | 0.3947 | 1060.0 | 784.2 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -16.57 | 99.90 | -10.64 | 153.41 | 0.3972 | 738.0 | 615.6 | |
| 0.00 | 1.56 | 0.00 | 0.84 | -16.40 | 98.36 | -12.18 | 149.99 | 0.4065 | -829.0 | -689.1 | |
| 0.00 | 6.14 | 0.00 | 3.43 | -17.94 | 94.12 | -16.42 | 144.31 | 0.4629 | -824.0 | -686.4 | |
| 0.00 | 1.90 | 0.00 | 1.06 | -17.57 | 93.53 | -17.00 | 142.86 | 0.4637 | -628.0 | -555.3 | |
| 0.00 | 1.73 | 0.00 | 0.99 | -19.20 | 91.28 | -19.26 | 141.63 | 0.5040 | -835.0 | -658.8 | |
| 0.00 | 1.21 | 0.00 | 0.70 | -19.44 | 90.78 | -19.76 | 141.24 | 0.5114 | -681.0 | -487.2 | |
| 0.00 | 1.82 | 0.00 | 1.05 | -19.83 | 90.66 | -19.88 | 141.59 | 0.5169 | -789.0 | -546.2 | |
| 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. | |