SDO HMI 2014-11-10 04:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.46 | 0.00 | 10.35 | -23.60 | 8.32 | -6.62 | 167.15 | 0.4690 | 535.2 | 425.5 | |
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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 | 1.21 | 0.00 | 0.66 | -21.25 | 10.35 | -4.59 | 169.86 | 0.4257 | 737.0 | 603.6 | |
| 0.00 | 1.21 | 0.00 | 0.66 | -20.40 | 10.22 | -4.72 | 169.18 | 0.4128 | 863.0 | 605.0 | |
| 0.00 | 1.12 | 0.00 | 0.62 | -22.37 | 10.08 | -4.86 | 169.80 | 0.4437 | 847.0 | 701.4 | |
| 0.00 | 2.59 | 0.00 | 1.43 | -22.60 | 9.75 | -5.19 | 169.22 | 0.4483 | 817.0 | 686.2 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -21.45 | 9.80 | -5.14 | 168.77 | 0.4304 | 703.0 | 494.9 | |
| 0.00 | 1.21 | 0.00 | 0.67 | -22.73 | 9.49 | -5.45 | 168.75 | 0.4511 | 860.0 | 755.3 | |
| 0.00 | 0.78 | 0.00 | 0.44 | -24.74 | 9.11 | -5.83 | 168.93 | 0.4826 | 725.0 | 611.2 | |
| 0.00 | 2.50 | 0.00 | 1.41 | -24.40 | 9.09 | -5.85 | 168.75 | 0.4776 | 479.0 | 582.6 | |
| 0.00 | 1.03 | 0.00 | 0.58 | -24.03 | 9.07 | -5.87 | 168.55 | 0.4721 | 839.0 | 719.2 | |
| 0.00 | 1.55 | 0.00 | 0.88 | -25.25 | 8.75 | -6.19 | 168.50 | 0.4913 | 678.0 | 541.2 | |
| 0.00 | 1.21 | 0.00 | 0.69 | -25.38 | 8.64 | -6.30 | 168.37 | 0.4937 | 695.0 | 562.9 | |
| 0.00 | 2.33 | 0.00 | 1.36 | -26.32 | 2.78 | -12.16 | 159.12 | 0.5319 | -760.0 | -628.7 | |
| 0.00 | 0.60 | 0.00 | 0.34 | -22.01 | 1.36 | -13.58 | 153.04 | 0.4822 | -525.0 | -392.7 | |
| 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. | |