SDO HMI 2014-10-02 15:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.90 | 0.00 | 12.21 | -5.19 | 138.75 | -24.55 | 115.19 | 0.4594 | -759.8 | -650.1 | |
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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 | 1.67 | 0.00 | 0.91 | -4.36 | 140.78 | -22.52 | 115.49 | 0.4249 | -716.0 | -546.0 | |
| 0.00 | 2.29 | 0.00 | 1.26 | -4.62 | 139.86 | -23.45 | 115.10 | 0.4398 | -923.0 | -748.3 | |
| 0.00 | 2.46 | 0.00 | 1.37 | -5.81 | 139.35 | -23.96 | 116.98 | 0.4552 | -1014.0 | -842.6 | |
| 0.00 | 2.55 | 0.00 | 1.42 | -5.51 | 139.19 | -24.11 | 116.24 | 0.4552 | -860.0 | -771.2 | |
| 0.00 | 2.29 | 0.00 | 1.26 | -3.37 | 139.17 | -24.13 | 111.87 | 0.4416 | -767.0 | -629.9 | |
| 0.00 | 2.02 | 0.00 | 1.13 | -6.37 | 139.02 | -24.28 | 117.76 | 0.4638 | -869.0 | -726.8 | |
| 0.00 | 0.79 | 0.00 | 0.44 | -4.04 | 139.09 | -24.22 | 113.19 | 0.4470 | -634.0 | -466.3 | |
| 0.00 | 1.41 | 0.00 | 0.78 | -3.47 | 138.97 | -24.33 | 111.90 | 0.4451 | -823.0 | -647.1 | |
| 0.00 | 1.23 | 0.00 | 0.69 | -6.49 | 138.48 | -24.82 | 117.45 | 0.4719 | -694.0 | -523.5 | |
| 0.00 | 1.85 | 0.00 | 1.04 | -7.25 | 138.17 | -25.13 | 118.55 | 0.4816 | -674.0 | -522.0 | |
| 0.00 | 0.79 | 0.00 | 0.45 | -3.51 | 136.84 | -26.46 | 110.27 | 0.4761 | -584.0 | -477.4 | |
| 0.00 | 1.58 | 0.00 | 0.91 | -6.09 | 136.12 | -27.19 | 114.57 | 0.5015 | -742.0 | -623.1 | |
| 0.00 | 0.97 | 0.00 | 0.55 | -5.02 | 135.49 | -27.81 | 112.12 | 0.5037 | -577.0 | -433.9 | |
| 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. | |