SDO HMI 2014-11-10 15:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 14.82 | 0.00 | 8.86 | -9.46 | 337.58 | -31.35 | 112.62 | 0.5575 | 199.7 | -75.3 | |
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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 | -9.99 | 342.37 | -26.55 | 117.08 | 0.4964 | 848.0 | 703.9 | |
| 0.00 | 0.60 | 0.00 | 0.34 | -5.21 | 342.60 | -26.32 | 107.97 | 0.4662 | 696.0 | 643.4 | |
| 0.00 | 1.21 | 0.00 | 0.68 | -5.58 | 342.41 | -26.51 | 108.59 | 0.4706 | 646.0 | 538.8 | |
| 0.00 | 1.03 | 0.00 | 0.60 | -9.64 | 340.88 | -28.05 | 115.22 | 0.5145 | 522.0 | 476.8 | |
| 0.00 | 1.21 | 0.00 | 0.71 | -11.47 | 339.83 | -29.10 | 117.58 | 0.5398 | 744.0 | 559.7 | |
| 0.00 | 1.03 | 0.00 | 0.60 | -6.91 | 339.80 | -29.12 | 109.51 | 0.5147 | 682.0 | 494.8 | |
| 0.00 | 0.26 | 0.00 | 0.15 | -11.17 | 339.41 | -29.51 | 116.76 | 0.5434 | 582.0 | 504.7 | |
| 0.00 | 2.07 | 0.00 | 1.25 | -10.04 | 336.40 | -32.53 | 112.84 | 0.5767 | -809.0 | -662.2 | |
| 0.00 | 1.98 | 0.00 | 1.21 | -9.83 | 335.45 | -33.47 | 111.93 | 0.5881 | -363.0 | -410.6 | |
| 0.00 | 2.07 | 0.00 | 1.28 | -9.56 | 334.54 | -34.39 | 110.99 | 0.5988 | -685.0 | -470.5 | |
| 0.00 | 2.41 | 0.00 | 1.50 | -10.96 | 334.36 | -34.56 | 113.09 | 0.6078 | -666.0 | -502.4 | |
| 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. | |