SDO HMI 2014-07-07 22:00:40 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.53 | 92.96 | 23.54 | 108.11 | 8.90 | 164.27 | -64.91 | 81.84 | 0.9053 | -382.3 | -52.4 | |
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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 | 1.45 | 0.00 | 1.47 | 9.05 | 168.26 | -60.92 | 81.63 | 0.8743 | -382.0 | -400.1 | |
| 0.00 | 1.63 | 0.00 | 1.66 | 8.74 | 168.16 | -61.02 | 81.99 | 0.8751 | -468.0 | -319.7 | |
| 1.00 | 2.27 | 1.02 | 2.32 | 9.28 | 167.94 | -61.24 | 81.37 | 0.8770 | -282.9 | -296.5 | |
| 0.00 | 1.54 | 0.00 | 1.60 | 8.28 | 167.57 | -61.61 | 82.53 | 0.8800 | 455.0 | 472.1 | |
| 0.00 | 1.09 | 0.00 | 1.14 | 8.20 | 167.27 | -61.92 | 82.62 | 0.8825 | 551.0 | 495.8 | |
| 0.00 | 0.91 | 0.00 | 0.99 | 11.49 | 165.89 | -63.29 | 78.93 | 0.8938 | -593.0 | -467.8 | |
| 5.54 | 11.98 | 6.15 | 13.28 | 8.81 | 165.45 | -63.73 | 81.94 | 0.8968 | -738.0 | -431.2 | |
| 0.00 | 0.91 | 0.00 | 1.07 | 11.62 | 163.80 | -65.38 | 78.85 | 0.9093 | 283.0 | 289.7 | |
| 0.00 | 0.27 | 0.00 | 0.32 | 10.65 | 164.07 | -65.11 | 79.92 | 0.9073 | 310.0 | 305.0 | |
| 0.00 | 0.27 | 0.00 | 0.32 | 11.43 | 163.66 | -65.52 | 79.06 | 0.9103 | 263.0 | 237.0 | |
| 0.82 | 2.00 | 0.96 | 2.35 | 10.79 | 163.86 | -65.32 | 79.76 | 0.9088 | 465.2 | 415.8 | |
| 12.17 | 65.37 | 14.23 | 76.97 | 8.88 | 163.98 | -65.20 | 81.87 | 0.9078 | -606.8 | -47.7 | |
| 1.00 | -12.00 | 1.18 | -12.00 | 8.59 | 163.86 | -65.33 | 82.18 | 0.9087 | -544.1 | 999999 | |
| 0.00 | 1.73 | 0.00 | 2.12 | 10.51 | 162.68 | -66.51 | 80.09 | 0.9171 | 180.0 | 289.2 | |
| 0.00 | 1.54 | 0.00 | 2.50 | 5.15 | 156.82 | -72.37 | 85.74 | 0.9531 | 237.0 | 225.6 | |
| 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. | |