SDO HMI 2014-11-10 10:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.21 | 0.00 | 10.07 | -9.37 | 336.89 | -34.77 | 110.45 | 0.6022 | -19.6 | -149.8 | |
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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 | 0.71 | -9.94 | 342.31 | -29.36 | 114.80 | 0.5340 | 701.0 | 593.9 | |
| 0.00 | 1.12 | 0.00 | 0.64 | -5.04 | 342.61 | -29.05 | 106.04 | 0.5054 | 659.0 | 530.4 | |
| 0.00 | 0.86 | 0.00 | 0.50 | -5.86 | 342.02 | -29.65 | 107.28 | 0.5174 | 720.0 | 565.1 | |
| 0.00 | 1.12 | 0.00 | 0.66 | -6.98 | 339.96 | -31.71 | 108.17 | 0.5512 | 671.0 | 523.5 | |
| 0.00 | 1.38 | 0.00 | 0.82 | -6.96 | 339.71 | -31.95 | 108.00 | 0.5545 | 646.0 | 514.8 | |
| 0.00 | 1.21 | 0.00 | 0.77 | -11.89 | 335.88 | -35.79 | 113.82 | 0.6278 | -486.0 | -449.1 | |
| 0.00 | 1.81 | 0.00 | 1.14 | -11.09 | 335.88 | -35.78 | 112.62 | 0.6239 | -612.0 | -425.0 | |
| 0.00 | 1.64 | 0.00 | 1.05 | -10.92 | 334.74 | -36.92 | 111.76 | 0.6374 | -659.0 | -549.6 | |
| 0.00 | 1.12 | 0.00 | 0.72 | -10.25 | 334.65 | -37.02 | 110.72 | 0.6357 | -519.0 | -413.4 | |
| 0.00 | 2.76 | 0.00 | 1.77 | -9.44 | 334.38 | -37.29 | 109.37 | 0.6357 | -784.0 | -571.7 | |
| 0.00 | 1.98 | 0.00 | 1.29 | -10.47 | 333.66 | -38.00 | 110.57 | 0.6490 | -553.0 | -469.0 | |
| 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. | |