SDO HMI 2014-09-04 09:01:21 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.43 | 0.00 | 11.26 | 9.95 | 183.79 | 7.57 | 280.14 | 0.1543 | -268.5 | -375.0 | |
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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 | 1.07 | 0.00 | 0.54 | 11.47 | 188.05 | 11.83 | 290.88 | 0.2159 | -768.0 | -596.4 | |
| 0.00 | 1.79 | 0.00 | 0.90 | 5.98 | 187.37 | 11.15 | 264.24 | 0.1941 | -889.0 | -623.2 | |
| 0.00 | 1.88 | 0.00 | 0.95 | 12.17 | 186.79 | 10.56 | 296.21 | 0.2007 | -709.0 | -568.8 | |
| 0.00 | 4.47 | 0.00 | 2.25 | 10.85 | 186.14 | 9.92 | 291.03 | 0.1821 | -915.0 | -715.0 | |
| 0.00 | 1.43 | 0.00 | 0.72 | 11.24 | 186.03 | 9.81 | 293.28 | 0.1827 | -1098.0 | -939.6 | |
| 0.00 | 1.16 | 0.00 | 0.59 | 10.97 | 185.96 | 9.74 | 292.02 | 0.1799 | -805.0 | -679.0 | |
| 0.00 | 1.70 | 0.00 | 0.86 | 10.73 | 185.86 | 9.63 | 290.94 | 0.1769 | -922.0 | -704.4 | |
| 0.00 | 1.43 | 0.00 | 0.72 | 5.68 | 185.70 | 9.47 | 261.26 | 0.1665 | -914.0 | -706.9 | |
| 0.00 | 1.52 | 0.00 | 0.76 | 10.99 | 185.21 | 8.99 | 293.65 | 0.1682 | -1022.0 | -796.2 | |
| 0.00 | 0.80 | 0.00 | 0.40 | 11.18 | 184.87 | 8.65 | 295.49 | 0.1642 | -673.0 | -485.3 | |
| 0.00 | 1.25 | 0.00 | 0.62 | 10.23 | 178.85 | 2.63 | 319.31 | 0.0696 | 1002.0 | 734.0 | |
| 0.00 | 1.16 | 0.00 | 0.58 | 8.54 | 176.39 | 0.17 | 352.77 | 0.0233 | 1017.0 | 818.2 | |
| 0.00 | 1.07 | 0.00 | 0.53 | 9.69 | 175.78 | -0.44 | 10.01 | 0.0440 | 933.0 | 688.8 | |
| 0.00 | 0.63 | 0.00 | 0.31 | 7.18 | 173.59 | -2.64 | 90.82 | 0.0459 | 765.0 | 496.9 | |
| 0.00 | 1.07 | 0.00 | 0.53 | 9.56 | 171.58 | -4.65 | 62.79 | 0.0902 | 971.0 | 660.0 | |
| 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. | |