SDO HMI 2014-10-04 07:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.77 | 213.45 | 36.54 | 119.96 | -13.16 | 121.02 | -20.27 | 134.49 | 0.4744 | 468.4 | 314.4 | |
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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 |
| 30.71 | 176.14 | 17.15 | 98.49 | -13.02 | 121.84 | -19.46 | 135.37 | 0.4639 | 1267.8 | 408.0 | |
| 1.94 | -1.00 | 1.08 | -1.00 | -12.58 | 121.68 | -19.62 | 134.45 | 0.4610 | 998.4 | 999999 | |
| 0.88 | -1.00 | 0.49 | -1.00 | -13.35 | 121.45 | -19.85 | 135.32 | 0.4717 | 840.6 | 999999 | |
| 2.99 | -1.00 | 1.67 | -1.00 | -12.59 | 121.45 | -19.85 | 134.13 | 0.4636 | 899.6 | 999999 | |
| 9.77 | -1.00 | 5.50 | -1.00 | -13.46 | 121.14 | -20.15 | 135.04 | 0.4762 | 831.0 | 999999 | |
| 2.82 | 9.77 | 1.59 | 5.52 | -13.52 | 120.48 | -20.82 | 134.21 | 0.4840 | 667.3 | 140.4 | |
| 0.00 | 1.06 | 0.00 | 0.60 | -12.89 | 118.81 | -22.48 | 131.04 | 0.4963 | 885.0 | 715.8 | |
| 0.79 | 1.85 | 0.46 | 1.08 | -15.36 | 117.98 | -23.32 | 133.67 | 0.5298 | -816.4 | -712.5 | |
| 0.00 | 1.14 | 0.00 | 0.67 | -15.33 | 117.44 | -23.86 | 132.96 | 0.5352 | -842.0 | -641.5 | |
| 0.00 | 0.79 | 0.00 | 0.46 | -14.78 | 117.47 | -23.83 | 132.22 | 0.5296 | -736.0 | -604.2 | |
| 4.05 | 21.82 | 2.34 | 12.63 | -13.66 | 117.43 | -23.87 | 130.52 | 0.5194 | -953.8 | -738.4 | |
| 0.00 | 0.88 | 0.00 | 0.51 | -12.51 | 117.55 | -23.75 | 128.89 | 0.5072 | -550.0 | -527.2 | |
| 10.82 | -11.00 | 6.26 | -11.00 | -13.22 | 117.14 | -24.16 | 129.52 | 0.5186 | -1056.9 | 999999 | |
| 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. | |