SDO HMI 2014-10-03 05:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.35 | 14.62 | 0.19 | 7.76 | -5.00 | 137.87 | -17.72 | 123.04 | 0.3632 | -847.7 | -684.7 | |
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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 | 1.06 | 0.00 | 0.55 | -4.72 | 140.31 | -15.28 | 126.27 | 0.3272 | -1000.0 | -768.4 | |
| 0.00 | 1.76 | 0.00 | 0.92 | -3.92 | 139.73 | -15.85 | 123.23 | 0.3273 | -807.0 | -771.3 | |
| 0.35 | 1.85 | 0.19 | 0.98 | -5.69 | 139.66 | -15.93 | 127.41 | 0.3454 | -1060.8 | -881.6 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -4.35 | 139.60 | -15.99 | 124.09 | 0.3331 | -817.0 | -696.5 | |
| 0.00 | 0.97 | 0.00 | 0.51 | -6.29 | 139.32 | -16.26 | 128.17 | 0.3557 | -734.0 | -606.5 | |
| 0.00 | 1.14 | 0.00 | 0.61 | -6.42 | 138.25 | -17.34 | 126.66 | 0.3708 | -777.0 | -657.7 | |
| 0.00 | 1.32 | 0.00 | 0.71 | -5.72 | 136.27 | -19.32 | 122.20 | 0.3907 | -855.0 | -694.3 | |
| 0.00 | 1.50 | 0.00 | 0.80 | -4.90 | 136.14 | -19.45 | 120.21 | 0.3855 | -997.0 | -673.8 | |
| 0.00 | 1.41 | 0.00 | 0.75 | -4.14 | 135.97 | -19.62 | 118.26 | 0.3819 | -707.0 | -578.6 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -4.84 | 135.95 | -19.64 | 119.84 | 0.3878 | -742.0 | -548.4 | |
| 0.00 | 1.41 | 0.00 | 0.76 | -4.51 | 135.93 | -19.66 | 119.05 | 0.3854 | -787.0 | -606.6 | |
| 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. | |