SDO HMI 2014-11-03 03:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.55 | 36.58 | 6.67 | 19.66 | -16.86 | 99.96 | -7.83 | 160.78 | 0.3862 | 214.9 | 265.3 | |
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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 |
| 1.21 | 13.32 | 0.64 | 7.06 | -16.39 | 103.69 | -4.10 | 168.96 | 0.3594 | 924.9 | 840.9 | |
| 2.34 | -1.00 | 1.24 | -1.00 | -16.23 | 103.63 | -4.16 | 168.71 | 0.3571 | 1217.1 | 999999 | |
| 4.59 | -1.00 | 2.43 | -1.00 | -16.29 | 103.47 | -4.31 | 168.34 | 0.3586 | 1030.6 | 999999 | |
| 0.00 | 1.12 | 0.00 | 0.60 | -16.37 | 101.17 | -6.62 | 162.50 | 0.3693 | 772.0 | 528.0 | |
| 0.00 | 0.43 | 0.00 | 0.23 | -15.74 | 100.63 | -7.16 | 160.59 | 0.3624 | 591.0 | 424.8 | |
| 0.00 | 1.21 | 0.00 | 0.65 | -16.60 | 100.53 | -7.25 | 161.15 | 0.3760 | 798.0 | 658.2 | |
| 4.41 | 12.80 | 2.36 | 6.85 | -16.60 | 100.22 | -7.57 | 160.40 | 0.3777 | 1118.0 | 728.3 | |
| 0.00 | 1.21 | 0.00 | 0.66 | -17.38 | 95.92 | -11.87 | 151.81 | 0.4172 | -931.0 | -789.5 | |
| 0.00 | 0.95 | 0.00 | 0.52 | -16.95 | 94.70 | -13.08 | 148.90 | 0.4209 | -944.0 | -736.8 | |
| 0.00 | 1.47 | 0.00 | 0.81 | -18.02 | 94.14 | -13.64 | 149.18 | 0.4397 | -863.0 | -723.8 | |
| 0.00 | 1.12 | 0.00 | 0.62 | -17.96 | 93.89 | -13.90 | 148.64 | 0.4409 | -916.0 | -761.0 | |
| 0.00 | 1.30 | 0.00 | 0.73 | -19.16 | 91.73 | -16.05 | 146.43 | 0.4744 | -769.0 | -671.0 | |
| 0.00 | 0.78 | 0.00 | 0.44 | -20.09 | 90.77 | -17.01 | 146.05 | 0.4941 | -659.0 | -502.6 | |
| 0.00 | 0.87 | 0.00 | 0.49 | -19.77 | 90.78 | -17.01 | 145.66 | 0.4900 | -740.0 | -619.1 | |
| 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. | |