SDO HMI 2014-12-09 07:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 62.07 | 334.20 | 31.30 | 168.54 | -3.87 | 1.28 | 10.21 | 249.89 | 0.1892 | 1231.9 | 409.7 | |
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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 | 1.11 | 0.00 | 0.57 | -4.98 | 4.88 | 13.81 | 250.51 | 0.2533 | 976.0 | 832.8 | |
| 0.00 | 1.45 | 0.00 | 0.74 | -4.80 | 4.72 | 13.65 | 250.99 | 0.2499 | 863.0 | 702.3 | |
| 35.30 | 320.04 | 17.82 | 161.39 | -4.00 | 1.53 | 10.46 | 249.68 | 0.1940 | 1385.3 | 411.7 | |
| 1.53 | -3.00 | 0.77 | -3.00 | -3.59 | 1.28 | 10.21 | 251.32 | 0.1877 | 1013.2 | 999999 | |
| 9.12 | -3.00 | 4.60 | -3.00 | -4.03 | 1.17 | 10.10 | 248.88 | 0.1884 | 1407.9 | 999999 | |
| 0.00 | 4.78 | 0.00 | 2.40 | -2.52 | 1.12 | 10.05 | 256.68 | 0.1801 | 987.0 | 565.9 | |
| 0.00 | 0.51 | 0.00 | 0.26 | -2.17 | 1.00 | 9.93 | 258.49 | 0.1767 | 231.0 | 169.5 | |
| 0.00 | 2.05 | 0.00 | 1.03 | -1.84 | 0.82 | 9.75 | 260.14 | 0.1726 | -795.0 | -694.2 | |
| 16.12 | -3.00 | 8.11 | -3.00 | -3.59 | 0.77 | 9.70 | 250.42 | 0.1794 | 1505.2 | 999999 | |
| 0.00 | 2.05 | 0.00 | 1.03 | -3.76 | 0.02 | 8.95 | 247.95 | 0.1684 | 164.0 | 117.2 | |
| 0.00 | 0.85 | 0.00 | 0.43 | -5.39 | 359.68 | 8.61 | 238.54 | 0.1756 | 1015.0 | 867.8 | |
| 0.00 | 1.36 | 0.00 | 0.69 | -5.36 | 359.23 | 8.16 | 237.32 | 0.1688 | 825.0 | 709.9 | |
| 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. | |