SDO HMI 2014-09-04 11:00:36 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 23.93 | 0.00 | 12.08 | 9.59 | 184.46 | 9.32 | 255.31 | 0.1830 | -638.7 | -582.6 | |
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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 | 1.16 | 0.00 | 0.59 | 11.45 | 188.09 | 12.96 | 289.26 | 0.2339 | -878.0 | -713.2 | |
| 0.00 | 1.34 | 0.00 | 0.68 | 11.82 | 186.63 | 11.49 | 292.97 | 0.2128 | -788.0 | -605.0 | |
| 0.00 | 0.98 | 0.00 | 0.50 | 10.89 | 186.27 | 11.14 | 289.26 | 0.2019 | -807.0 | -666.5 | |
| 0.00 | 1.07 | 0.00 | 0.54 | 10.74 | 186.17 | 11.04 | 288.70 | 0.1995 | -842.0 | -719.0 | |
| 0.00 | 1.25 | 0.00 | 0.63 | 11.41 | 186.14 | 11.00 | 291.92 | 0.2026 | -673.0 | -571.9 | |
| 0.00 | 2.59 | 0.00 | 1.31 | 11.20 | 186.10 | 10.96 | 290.99 | 0.2008 | -1052.0 | -894.9 | |
| 0.00 | 0.98 | 0.00 | 0.50 | 10.92 | 186.09 | 10.95 | 289.71 | 0.1991 | -1001.0 | -792.7 | |
| 0.00 | 1.97 | 0.00 | 0.99 | 10.78 | 185.86 | 10.73 | 289.35 | 0.1947 | -889.0 | -683.2 | |
| 0.00 | 1.25 | 0.00 | 0.63 | 5.73 | 185.69 | 10.55 | 262.53 | 0.1846 | -900.0 | -736.4 | |
| 0.00 | 3.84 | 0.00 | 1.94 | 5.92 | 185.38 | 10.25 | 263.32 | 0.1790 | -782.0 | -714.6 | |
| 0.00 | 1.16 | 0.00 | 0.59 | 10.61 | 185.23 | 10.10 | 289.51 | 0.1837 | -953.0 | -762.2 | |
| 0.00 | 2.32 | 0.00 | 1.17 | 5.96 | 185.04 | 9.91 | 263.27 | 0.1731 | -835.0 | -766.1 | |
| 0.00 | 1.52 | 0.00 | 0.77 | 11.22 | 184.94 | 9.81 | 293.20 | 0.1826 | -808.0 | -614.5 | |
| 0.00 | 1.25 | 0.00 | 0.62 | 12.55 | 173.64 | -1.49 | 15.32 | 0.0968 | 780.0 | 583.7 | |
| 0.00 | 1.25 | 0.00 | 0.62 | 11.33 | 171.14 | -3.99 | 43.49 | 0.0996 | 847.0 | 676.9 | |
| 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. | |