SDO HMI 2014-11-07 05:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 3.19 | 16.23 | 2.14 | 10.84 | -16.12 | 16.44 | -37.51 | 119.22 | 0.6720 | -522.6 | -468.4 | |
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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 | 0.86 | 0.00 | 0.52 | -13.87 | 23.86 | -30.09 | 121.15 | 0.5709 | 726.0 | 638.6 | |
| 0.00 | 1.12 | 0.00 | 0.73 | -14.71 | 17.96 | -35.98 | 118.19 | 0.6471 | 673.0 | 362.2 | |
| 0.00 | 0.43 | 0.00 | 0.29 | -17.17 | 16.23 | -37.72 | 120.48 | 0.6806 | -713.0 | -651.0 | |
| 0.00 | 1.47 | 0.00 | 0.98 | -16.50 | 16.31 | -37.64 | 119.64 | 0.6760 | -733.0 | -672.1 | |
| 0.00 | 1.73 | 0.00 | 1.16 | -16.16 | 16.23 | -37.72 | 119.13 | 0.6750 | -714.0 | -623.2 | |
| 0.00 | 1.30 | 0.00 | 0.87 | -16.61 | 16.13 | -37.82 | 119.66 | 0.6786 | -746.0 | -643.1 | |
| 0.00 | 1.12 | 0.00 | 0.76 | -16.52 | 16.03 | -37.92 | 119.48 | 0.6792 | -796.0 | -644.6 | |
| 3.19 | 5.18 | 2.14 | 3.48 | -16.14 | 16.04 | -37.91 | 118.98 | 0.6770 | -945.5 | -736.7 | |
| 0.00 | 1.04 | 0.00 | 0.70 | -16.69 | 15.59 | -38.35 | 119.46 | 0.6850 | -676.0 | -510.8 | |
| 0.00 | 1.38 | 0.00 | 0.93 | -16.19 | 15.63 | -38.31 | 118.81 | 0.6818 | -813.0 | -549.8 | |
| 0.00 | 0.60 | 0.00 | 0.42 | -16.56 | 13.57 | -40.37 | 118.14 | 0.7065 | -529.0 | -464.9 | |
| 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. | |