SDO HMI 2014-11-11 08:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 15.84 | 0.00 | 8.84 | -15.58 | 18.78 | 19.21 | 224.14 | 0.4566 | -172.2 | 70.4 | |
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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 | 1.46 | 0.00 | 0.83 | -13.65 | 23.15 | 23.58 | 233.59 | 0.4850 | 578.0 | 439.2 | |
| 0.00 | 3.96 | 0.00 | 2.24 | -13.64 | 22.75 | 23.18 | 233.15 | 0.4800 | 951.0 | 782.0 | |
| 0.00 | 1.21 | 0.00 | 0.68 | -14.16 | 22.40 | 22.83 | 231.85 | 0.4804 | 635.0 | 629.6 | |
| 0.00 | 1.12 | 0.00 | 0.63 | -16.43 | 20.13 | 20.56 | 225.26 | 0.4761 | 767.0 | 508.8 | |
| 0.00 | 0.86 | 0.00 | 0.48 | -16.87 | 17.32 | 17.75 | 220.46 | 0.4514 | -681.0 | -589.4 | |
| 0.00 | 1.29 | 0.00 | 0.72 | -17.47 | 16.99 | 17.41 | 219.05 | 0.4550 | -295.0 | -325.8 | |
| 0.00 | 0.78 | 0.00 | 0.43 | -17.24 | 16.70 | 17.13 | 218.94 | 0.4495 | -625.0 | -535.2 | |
| 0.00 | 1.46 | 0.00 | 0.82 | -18.07 | 16.72 | 17.15 | 217.77 | 0.4595 | -540.0 | -461.9 | |
| 0.00 | 0.95 | 0.00 | 0.52 | -17.57 | 15.56 | 15.99 | 216.58 | 0.4426 | -622.0 | -495.0 | |
| 0.00 | 0.86 | 0.00 | 0.47 | -16.34 | 13.98 | 14.41 | 215.56 | 0.4125 | -832.0 | -679.7 | |
| 0.00 | 1.29 | 0.00 | 0.70 | -15.86 | 13.28 | 13.71 | 214.94 | 0.3998 | -804.0 | -545.5 | |
| 0.00 | 0.60 | 0.00 | 0.32 | -15.70 | 7.89 | 8.32 | 203.23 | 0.3548 | -598.0 | -500.0 | |
| 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. | |