SDO HMI 2014-11-03 04:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.54 | 41.87 | 6.66 | 22.58 | -17.10 | 99.07 | -8.16 | 160.49 | 0.3928 | -38.6 | 103.1 | |
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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 |
| 3.46 | 15.14 | 1.83 | 8.02 | -16.30 | 103.67 | -3.57 | 170.31 | 0.3564 | 1103.9 | 757.3 | |
| 5.19 | -1.00 | 2.75 | -1.00 | -16.30 | 103.51 | -3.72 | 169.90 | 0.3568 | 994.7 | 999999 | |
| 0.00 | 1.12 | 0.00 | 0.60 | -16.60 | 100.55 | -6.69 | 162.51 | 0.3732 | 817.0 | 613.8 | |
| 3.89 | 12.37 | 2.08 | 6.61 | -16.64 | 100.23 | -7.00 | 161.78 | 0.3752 | 1163.8 | 747.5 | |
| 0.00 | 2.42 | 0.00 | 1.32 | -17.35 | 95.98 | -11.26 | 152.99 | 0.4123 | -832.0 | -705.4 | |
| 0.00 | 0.87 | 0.00 | 0.47 | -17.07 | 95.87 | -11.37 | 152.43 | 0.4090 | -768.0 | -638.1 | |
| 0.00 | 1.04 | 0.00 | 0.57 | -18.02 | 94.14 | -13.10 | 150.18 | 0.4353 | -885.0 | -752.9 | |
| 0.00 | 1.21 | 0.00 | 0.67 | -18.00 | 93.85 | -13.39 | 149.62 | 0.4372 | -980.0 | -739.1 | |
| 0.00 | 0.43 | 0.00 | 0.24 | -19.62 | 93.39 | -13.85 | 150.69 | 0.4624 | -734.0 | -590.6 | |
| 0.00 | 1.12 | 0.00 | 0.60 | -13.44 | 93.53 | -13.71 | 142.54 | 0.3805 | -824.0 | -595.2 | |
| 0.00 | 0.87 | 0.00 | 0.49 | -19.23 | 91.77 | -15.47 | 147.46 | 0.4702 | -836.0 | -675.0 | |
| 0.00 | 0.87 | 0.00 | 0.49 | -19.66 | 91.26 | -15.98 | 147.16 | 0.4799 | -797.0 | -538.2 | |
| 0.00 | 2.68 | 0.00 | 1.52 | -19.99 | 91.06 | -16.18 | 147.23 | 0.4857 | -662.0 | -609.9 | |
| 0.00 | 1.30 | 0.00 | 0.73 | -19.77 | 90.82 | -16.41 | 146.58 | 0.4849 | -809.0 | -577.5 | |
| 0.00 | 0.43 | 0.00 | 0.25 | -21.86 | 89.41 | -17.83 | 146.89 | 0.5224 | -587.0 | -508.6 | |
| 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. | |