SDO HMI 2014-06-28 20:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.96 | 156.14 | 129.81 | 524.69 | -10.49 | 268.54 | -80.87 | 101.02 | 0.9892 | 181.4 | 129.8 | |
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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 | 3.72 | 0.00 | 8.57 | -11.82 | 272.69 | -76.72 | 102.70 | 0.9775 | -276.0 | -190.3 | |
| 0.00 | 2.18 | 0.00 | 5.80 | -11.93 | 270.95 | -78.46 | 102.66 | 0.9834 | 462.0 | 405.5 | |
| 0.00 | 2.63 | 0.00 | 8.42 | -12.23 | 269.22 | -80.20 | 102.82 | 0.9884 | -98.0 | -151.8 | |
| 2.09 | 101.58 | 5.63 | 295.50 | -10.15 | 270.79 | -78.63 | 100.85 | 0.9834 | 652.5 | 176.9 | |
| 0.00 | 2.00 | 0.00 | 8.30 | -12.49 | 266.89 | -82.52 | 102.90 | 0.9936 | 14.0 | -90.8 | |
| 12.35 | -4.00 | 36.18 | -4.00 | -10.17 | 269.76 | -79.65 | 100.78 | 0.9864 | -14.3 | 999999 | |
| 0.00 | 1.45 | 0.00 | 3.86 | -9.10 | 270.74 | -78.67 | 99.77 | 0.9833 | 298.0 | 288.0 | |
| 18.52 | 29.05 | 88.00 | 137.34 | -11.37 | 265.98 | -83.43 | 101.72 | 0.9951 | 246.5 | 126.3 | |
| 0.00 | 3.36 | 0.00 | 13.18 | -10.41 | 267.26 | -82.16 | 100.84 | 0.9926 | -77.0 | -80.2 | |
| 0.00 | 0.27 | 0.00 | 0.96 | -9.75 | 268.10 | -81.32 | 100.23 | 0.9906 | -352.0 | -343.7 | |
| 0.00 | 9.90 | 0.00 | 42.76 | -8.88 | 266.61 | -82.81 | 99.26 | 0.9937 | 177.0 | 40.5 | |
| 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. | |