SDO HMI 2014-11-10 07:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.83 | 0.00 | 9.46 | -16.97 | 15.44 | 2.14 | 185.93 | 0.3597 | -615.9 | -476.4 | |
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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 | 2.41 | 0.00 | 1.28 | -14.41 | 23.39 | 10.08 | 209.07 | 0.3506 | 920.0 | 790.2 | |
| 0.00 | 1.12 | 0.00 | 0.59 | -16.62 | 17.49 | 4.19 | 191.57 | 0.3509 | -742.0 | -639.4 | |
| 0.00 | 2.24 | 0.00 | 1.18 | -16.14 | 16.71 | 3.41 | 189.69 | 0.3408 | -1002.0 | -777.3 | |
| 0.00 | 1.12 | 0.00 | 0.59 | -16.87 | 16.69 | 3.39 | 189.28 | 0.3525 | -976.0 | -811.6 | |
| 0.00 | 1.81 | 0.00 | 0.96 | -17.06 | 16.54 | 3.24 | 188.78 | 0.3552 | -739.0 | -599.0 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -18.52 | 16.41 | 3.11 | 187.83 | 0.3785 | -851.0 | -704.5 | |
| 0.00 | 1.21 | 0.00 | 0.64 | -18.49 | 15.22 | 1.91 | 184.86 | 0.3758 | -720.0 | -661.6 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -19.03 | 15.19 | 1.89 | 184.67 | 0.3846 | -708.0 | -605.3 | |
| 0.00 | 1.72 | 0.00 | 0.93 | -20.29 | 14.92 | 1.62 | 183.77 | 0.4044 | -740.0 | -599.8 | |
| 0.00 | 0.78 | 0.00 | 0.41 | -15.38 | 14.02 | 0.72 | 182.14 | 0.3236 | -335.0 | -389.0 | |
| 0.00 | 3.53 | 0.00 | 1.87 | -16.55 | 8.00 | -5.30 | 165.45 | 0.3539 | -882.0 | -724.0 | |
| 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. | |