SDO HMI 2014-10-02 08:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 30.30 | 92.75 | 17.53 | 53.98 | -10.15 | 140.24 | -26.90 | 121.84 | 0.5264 | 633.3 | 286.3 | |
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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 | 1.94 | 0.00 | 1.13 | -11.90 | 141.17 | -25.97 | 125.60 | 0.5292 | 717.0 | 560.8 | |
| 0.00 | 1.06 | 0.00 | 0.63 | -13.76 | 140.37 | -26.77 | 127.58 | 0.5543 | 576.0 | 477.6 | |
| 0.00 | 1.23 | 0.00 | 0.72 | -12.07 | 140.40 | -26.75 | 125.07 | 0.5398 | 674.0 | 586.5 | |
| 7.40 | 78.30 | 4.28 | 45.31 | -9.61 | 140.60 | -26.54 | 121.32 | 0.5177 | 1081.2 | 395.8 | |
| 9.60 | -4.00 | 5.54 | -4.00 | -9.23 | 140.60 | -26.54 | 120.69 | 0.5149 | 987.2 | 999999 | |
| 7.84 | -4.00 | 4.55 | -4.00 | -9.99 | 140.43 | -26.71 | 121.79 | 0.5228 | 832.0 | 999999 | |
| 5.46 | -4.00 | 3.16 | -4.00 | -9.77 | 140.45 | -26.69 | 121.45 | 0.5209 | 1061.6 | 999999 | |
| 0.00 | 1.32 | 0.00 | 0.78 | -11.50 | 139.91 | -27.24 | 123.69 | 0.5411 | 817.0 | 740.9 | |
| 0.00 | 0.88 | 0.00 | 0.52 | -12.87 | 139.68 | -27.46 | 125.57 | 0.5549 | 578.0 | 470.4 | |
| 0.00 | 1.41 | 0.00 | 0.87 | -16.47 | 137.96 | -29.18 | 129.01 | 0.6039 | -507.0 | -389.8 | |
| 0.00 | 0.97 | 0.00 | 0.59 | -14.43 | 138.14 | -29.00 | 126.36 | 0.5853 | -472.0 | -397.5 | |
| 0.00 | 2.99 | 0.00 | 1.81 | -12.63 | 137.71 | -29.43 | 123.37 | 0.5763 | -745.0 | -632.9 | |
| 0.00 | 1.59 | 0.00 | 0.97 | -12.34 | 136.76 | -30.39 | 122.10 | 0.5855 | -865.0 | -706.6 | |
| 0.00 | 1.06 | 0.00 | 0.65 | -12.51 | 136.59 | -30.55 | 122.21 | 0.5887 | -576.0 | -513.5 | |
| 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. | |