SDO HMI 2014-10-02 17:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.26 | 0.00 | 10.65 | -5.32 | 138.91 | -23.29 | 116.73 | 0.4427 | -727.3 | -639.7 | |
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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 | 0.88 | 0.00 | 0.48 | -6.79 | 140.91 | -21.29 | 121.92 | 0.4265 | 726.0 | 607.9 | |
| 0.00 | 1.58 | 0.00 | 0.86 | -4.32 | 140.53 | -21.67 | 116.32 | 0.4126 | -937.0 | -689.8 | |
| 0.00 | 0.79 | 0.00 | 0.43 | -4.53 | 140.10 | -22.10 | 116.29 | 0.4201 | -845.0 | -634.6 | |
| 0.00 | 1.41 | 0.00 | 0.77 | -4.63 | 139.93 | -22.27 | 116.32 | 0.4232 | -1039.0 | -882.6 | |
| 0.00 | 1.06 | 0.00 | 0.58 | -4.54 | 139.71 | -22.49 | 115.91 | 0.4258 | -761.0 | -626.7 | |
| 0.00 | 0.88 | 0.00 | 0.48 | -4.21 | 139.62 | -22.58 | 115.12 | 0.4247 | -854.0 | -757.1 | |
| 0.00 | 2.11 | 0.00 | 1.16 | -5.78 | 139.40 | -22.80 | 118.14 | 0.4391 | -1031.0 | -853.9 | |
| 0.00 | 2.55 | 0.00 | 1.41 | -5.57 | 139.24 | -22.96 | 117.55 | 0.4397 | -1030.0 | -809.3 | |
| 0.00 | 2.11 | 0.00 | 1.17 | -6.38 | 139.07 | -23.13 | 118.98 | 0.4480 | -921.0 | -739.5 | |
| 0.00 | 1.23 | 0.00 | 0.68 | -6.17 | 139.02 | -23.18 | 118.50 | 0.4472 | -661.0 | -568.4 | |
| 0.00 | 0.70 | 0.00 | 0.39 | -3.51 | 138.99 | -23.21 | 112.99 | 0.4291 | -837.0 | -664.0 | |
| 0.00 | 1.06 | 0.00 | 0.59 | -3.36 | 136.95 | -25.25 | 110.91 | 0.4578 | -624.0 | -487.9 | |
| 0.00 | 1.58 | 0.00 | 0.90 | -6.00 | 136.14 | -26.06 | 115.37 | 0.4856 | -750.0 | -568.7 | |
| 0.00 | 1.32 | 0.00 | 0.75 | -6.13 | 136.06 | -26.14 | 115.54 | 0.4874 | -618.0 | -521.9 | |
| 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. | |