SDO HMI 2014-11-08 22:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.66 | 0.00 | 11.72 | -22.32 | 9.26 | -22.16 | 141.09 | 0.5578 | 560.9 | 512.5 | |
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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 | 1.12 | 0.00 | 0.65 | -20.56 | 10.57 | -20.86 | 140.55 | 0.5267 | 613.0 | 582.2 | |
| 0.00 | 1.55 | 0.00 | 0.90 | -20.01 | 10.51 | -20.91 | 139.75 | 0.5213 | 706.0 | 529.6 | |
| 0.00 | 0.86 | 0.00 | 0.50 | -20.43 | 10.42 | -21.01 | 140.18 | 0.5268 | 592.0 | 585.4 | |
| 0.00 | 1.47 | 0.00 | 0.86 | -21.32 | 10.18 | -21.24 | 141.01 | 0.5386 | 769.0 | 666.0 | |
| 0.00 | 1.03 | 0.00 | 0.60 | -19.98 | 10.31 | -21.11 | 139.45 | 0.5229 | 833.0 | 650.1 | |
| 0.00 | 1.98 | 0.00 | 1.16 | -20.40 | 10.22 | -21.21 | 139.89 | 0.5284 | 540.0 | 503.7 | |
| 0.00 | 1.47 | 0.00 | 0.89 | -24.62 | 9.41 | -22.01 | 143.96 | 0.5815 | 718.0 | 652.6 | |
| 0.00 | 2.59 | 0.00 | 1.54 | -22.31 | 9.64 | -21.78 | 141.57 | 0.5544 | 857.0 | 675.6 | |
| 0.00 | 1.21 | 0.00 | 0.73 | -24.32 | 9.26 | -22.17 | 143.44 | 0.5795 | 731.0 | 583.4 | |
| 0.00 | 1.38 | 0.00 | 0.84 | -24.50 | 8.98 | -22.45 | 143.31 | 0.5838 | 657.0 | 607.8 | |
| 0.00 | 1.81 | 0.00 | 1.09 | -23.13 | 8.70 | -22.72 | 141.40 | 0.5716 | 631.0 | 412.9 | |
| 0.00 | 1.03 | 0.00 | 0.63 | -24.24 | 8.32 | -23.11 | 142.25 | 0.5868 | 324.0 | 348.1 | |
| 0.00 | 1.21 | 0.00 | 0.73 | -21.65 | 7.15 | -24.28 | 137.78 | 0.5709 | 434.0 | 475.9 | |
| 0.00 | 0.95 | 0.00 | 0.60 | -25.29 | 4.55 | -26.88 | 139.39 | 0.6303 | -553.0 | -432.5 | |
| 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. | |