SDO HMI 2014-09-03 12:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.22 | 0.00 | 9.56 | 9.12 | 186.20 | -1.59 | 71.87 | 0.0585 | -839.2 | -725.5 | |
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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 |
| 0.00 | 2.77 | 0.00 | 1.37 | 6.12 | 187.32 | -0.47 | 156.86 | 0.0208 | -1164.0 | -980.6 | |
| 0.00 | 2.06 | 0.00 | 1.02 | 6.09 | 187.08 | -0.71 | 147.70 | 0.0232 | -971.0 | -789.3 | |
| 0.00 | 1.25 | 0.00 | 0.62 | 12.20 | 187.04 | -0.75 | 8.33 | 0.0884 | -831.0 | -682.1 | |
| 0.00 | 1.79 | 0.00 | 0.89 | 8.30 | 186.87 | -0.93 | 40.12 | 0.0249 | -785.0 | -639.4 | |
| 0.00 | 0.36 | 0.00 | 0.18 | 10.75 | 186.77 | -1.02 | 15.85 | 0.0645 | -343.0 | -558.0 | |
| 0.00 | 1.16 | 0.00 | 0.58 | 11.50 | 186.24 | -1.55 | 19.46 | 0.0798 | -859.0 | -675.2 | |
| 0.00 | 0.89 | 0.00 | 0.45 | 12.35 | 185.90 | -1.89 | 19.78 | 0.0958 | -603.0 | -466.9 | |
| 0.00 | 0.72 | 0.00 | 0.36 | 11.02 | 185.78 | -2.01 | 27.36 | 0.0752 | -896.0 | -775.4 | |
| 0.00 | 1.16 | 0.00 | 0.58 | 5.57 | 185.77 | -2.02 | 129.10 | 0.0454 | -877.0 | -789.2 | |
| 0.00 | 1.97 | 0.00 | 0.98 | 12.11 | 185.71 | -2.08 | 22.51 | 0.0930 | -874.0 | -590.6 | |
| 0.00 | 1.34 | 0.00 | 0.67 | 5.73 | 185.71 | -2.08 | 125.59 | 0.0446 | -948.0 | -652.6 | |
| 0.00 | 2.50 | 0.00 | 1.24 | 10.89 | 185.01 | -2.78 | 36.47 | 0.0804 | -994.0 | -796.8 | |
| 0.00 | 1.25 | 0.00 | 0.62 | 11.38 | 184.86 | -2.94 | 34.59 | 0.0889 | -765.0 | -563.3 | |
| 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. | |