SDO HMI 2014-11-10 16:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.77 | 0.00 | 9.25 | -8.83 | 338.60 | -29.77 | 112.61 | 0.5334 | 180.4 | 136.7 | |
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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 | 0.95 | 0.00 | 0.54 | -9.98 | 342.43 | -25.94 | 117.58 | 0.4881 | 905.0 | 604.0 | |
| 0.00 | 1.98 | 0.00 | 1.10 | -5.20 | 342.61 | -25.76 | 108.31 | 0.4578 | 742.0 | 567.0 | |
| 0.00 | 1.03 | 0.00 | 0.59 | -9.74 | 342.05 | -26.33 | 116.82 | 0.4917 | 133.0 | 176.2 | |
| 0.00 | 1.46 | 0.00 | 0.82 | -5.69 | 342.26 | -26.11 | 109.08 | 0.4654 | 634.0 | 543.1 | |
| 0.00 | 0.78 | 0.00 | 0.45 | -10.08 | 340.97 | -27.40 | 116.52 | 0.5085 | 716.0 | 625.0 | |
| 0.00 | 1.38 | 0.00 | 0.80 | -12.51 | 340.68 | -27.70 | 120.48 | 0.5286 | 694.0 | 439.6 | |
| 0.00 | 0.95 | 0.00 | 0.55 | -11.48 | 339.87 | -28.51 | 118.07 | 0.5322 | 688.0 | 493.1 | |
| 0.00 | 0.95 | 0.00 | 0.54 | -6.86 | 339.83 | -28.54 | 109.79 | 0.5061 | 657.0 | 528.9 | |
| 0.00 | 0.86 | 0.00 | 0.50 | -6.80 | 338.81 | -29.56 | 109.04 | 0.5203 | 409.0 | 384.9 | |
| 0.00 | 0.60 | 0.00 | 0.37 | -9.63 | 335.43 | -32.94 | 111.91 | 0.5801 | -561.0 | -578.0 | |
| 0.00 | 0.86 | 0.00 | 0.53 | -10.86 | 334.96 | -33.42 | 113.61 | 0.5925 | -653.0 | -564.4 | |
| 0.00 | 1.21 | 0.00 | 0.74 | -9.60 | 334.57 | -33.81 | 111.37 | 0.5913 | -671.0 | -556.1 | |
| 0.00 | 1.55 | 0.00 | 0.96 | -10.92 | 334.22 | -34.15 | 113.26 | 0.6023 | -593.0 | -359.9 | |
| 0.00 | 1.21 | 0.00 | 0.76 | -6.95 | 331.45 | -36.92 | 105.68 | 0.6216 | -575.0 | -462.3 | |
| 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. | |