SDO HMI 2014-11-10 19:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 21.97 | 0.00 | 11.82 | -15.05 | 19.93 | 13.22 | 214.70 | 0.3921 | -252.2 | 104.5 | |
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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 | 1.46 | 0.00 | 0.81 | -11.86 | 28.30 | 21.59 | 234.32 | 0.4452 | 783.0 | 635.5 | |
| 0.00 | 2.24 | 0.00 | 1.21 | -13.97 | 22.99 | 16.28 | 222.60 | 0.4035 | 861.0 | 691.7 | |
| 0.00 | 2.07 | 0.00 | 1.11 | -13.69 | 22.69 | 15.97 | 222.56 | 0.3969 | 765.0 | 569.8 | |
| 0.00 | 6.29 | 0.00 | 3.38 | -13.77 | 22.18 | 15.47 | 221.51 | 0.3925 | 479.0 | 762.8 | |
| 0.00 | 1.64 | 0.00 | 0.88 | -16.89 | 17.32 | 10.60 | 207.02 | 0.3893 | -743.0 | -526.6 | |
| 0.00 | 2.15 | 0.00 | 1.16 | -17.30 | 17.00 | 10.28 | 205.82 | 0.3928 | -725.0 | -558.6 | |
| 0.00 | 1.81 | 0.00 | 0.97 | -16.10 | 16.77 | 10.06 | 206.79 | 0.3740 | -878.0 | -686.4 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -16.34 | 16.07 | 9.35 | 204.86 | 0.3725 | -750.0 | -687.5 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -20.33 | 15.26 | 8.54 | 199.14 | 0.4266 | -851.0 | -652.5 | |
| 0.00 | 1.21 | 0.00 | 0.64 | -15.04 | 14.27 | 7.55 | 201.93 | 0.3413 | -909.0 | -796.9 | |
| 0.00 | 1.12 | 0.00 | 0.59 | -16.12 | 12.94 | 6.22 | 197.35 | 0.3508 | -806.0 | -572.5 | |
| 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. | |