SDO HMI 2014-11-01 08:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 8.32 | 23.66 | 5.06 | 15.03 | -16.89 | 98.79 | -32.64 | 124.52 | 0.6248 | 128.9 | 66.5 | |
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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 |
| 3.38 | 6.67 | 2.05 | 4.04 | -16.15 | 102.43 | -29.00 | 126.23 | 0.5795 | 1012.2 | 816.9 | |
| 0.00 | 0.61 | 0.00 | 0.37 | -16.47 | 102.37 | -29.05 | 126.64 | 0.5826 | 633.0 | 464.0 | |
| 4.94 | 6.93 | 3.01 | 4.22 | -16.20 | 102.06 | -29.36 | 125.97 | 0.5840 | 833.9 | 604.6 | |
| 0.00 | 1.99 | 0.00 | 1.21 | -15.97 | 102.06 | -29.36 | 125.65 | 0.5823 | 588.0 | 548.3 | |
| 0.00 | 0.95 | 0.00 | 0.64 | -17.07 | 94.29 | -37.13 | 121.28 | 0.6775 | -720.0 | -575.4 | |
| 0.00 | 0.35 | 0.00 | 0.24 | -18.60 | 93.67 | -37.75 | 122.87 | 0.6932 | -564.0 | -441.8 | |
| 0.00 | 1.13 | 0.00 | 0.76 | -17.35 | 93.67 | -37.75 | 121.26 | 0.6860 | -541.0 | -425.6 | |
| 0.00 | 1.30 | 0.00 | 0.93 | -19.61 | 91.52 | -39.90 | 122.81 | 0.7213 | -771.0 | -624.6 | |
| 0.00 | 1.30 | 0.00 | 0.93 | -19.92 | 91.22 | -40.20 | 123.01 | 0.7261 | -582.0 | -508.5 | |
| 0.00 | 0.61 | 0.00 | 0.43 | -19.46 | 91.28 | -40.15 | 122.48 | 0.7230 | -627.0 | -527.4 | |
| 0.00 | 1.82 | 0.00 | 1.26 | -16.80 | 91.81 | -39.62 | 119.42 | 0.7032 | -188.0 | -360.8 | |
| 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. | |