SDO HMI 2014-04-06 16:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.62 | 26.48 | 0.31 | 13.14 | -7.92 | 6.87 | -2.32 | 138.90 | 0.0680 | -6.2 | -275.2 | |
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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 | 1.76 | 0.00 | 0.87 | -8.25 | 12.60 | 3.41 | 238.83 | 0.0692 | 1056.0 | 831.3 | |
| 0.62 | 1.67 | 0.31 | 0.83 | -9.70 | 10.12 | 0.93 | 194.73 | 0.0630 | 1036.9 | 944.2 | |
| 0.00 | 1.23 | 0.00 | 0.61 | -9.12 | 9.96 | 0.77 | 194.74 | 0.0527 | 867.0 | 783.8 | |
| 0.00 | 1.06 | 0.00 | 0.52 | -9.27 | 9.84 | 0.65 | 191.91 | 0.0548 | 833.0 | 712.3 | |
| 0.00 | 2.29 | 0.00 | 1.13 | -9.06 | 9.75 | 0.56 | 191.03 | 0.0509 | 843.0 | 615.7 | |
| 0.00 | 1.23 | 0.00 | 0.61 | -7.53 | 9.24 | 0.05 | 182.06 | 0.0231 | 898.0 | 725.0 | |
| 0.00 | 1.14 | 0.00 | 0.57 | -7.49 | 6.21 | -2.98 | 113.51 | 0.0564 | -785.0 | -649.2 | |
| 0.00 | 0.97 | 0.00 | 0.48 | -7.49 | 5.73 | -3.46 | 110.51 | 0.0642 | -973.0 | -792.1 | |
| 0.00 | 5.19 | 0.00 | 2.58 | -6.86 | 5.52 | -3.67 | 100.18 | 0.0648 | -660.0 | -833.1 | |
| 0.00 | 4.84 | 0.00 | 2.40 | -7.48 | 4.97 | -4.22 | 107.06 | 0.0767 | -895.0 | -926.2 | |
| 0.00 | 1.58 | 0.00 | 0.79 | -7.60 | 4.54 | -4.65 | 106.95 | 0.0843 | -793.0 | -658.8 | |
| 0.00 | 1.50 | 0.00 | 0.74 | -8.44 | 4.41 | -4.78 | 115.40 | 0.0916 | -922.0 | -755.0 | |
| 0.00 | 2.02 | 0.00 | 1.01 | -7.77 | 3.66 | -5.53 | 106.12 | 0.0998 | -910.0 | -542.7 | |
| 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. | |