SDO HMI 2014-11-10 12:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 17.05 | 0.00 | 10.39 | -9.65 | 337.72 | -32.85 | 112.10 | 0.5784 | -2.8 | -22.1 | |
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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 | 1.72 | 0.00 | 1.00 | -9.93 | 342.56 | -28.01 | 115.79 | 0.5158 | 670.0 | 575.0 | |
| 0.00 | 1.72 | 0.00 | 0.98 | -5.25 | 342.66 | -27.91 | 107.07 | 0.4896 | 806.0 | 598.9 | |
| 0.00 | 1.12 | 0.00 | 0.65 | -9.94 | 342.32 | -28.25 | 115.61 | 0.5191 | 855.0 | 587.5 | |
| 0.00 | 1.29 | 0.00 | 0.76 | -9.91 | 341.25 | -29.32 | 114.76 | 0.5333 | 631.0 | 494.9 | |
| 0.00 | 1.64 | 0.00 | 0.98 | -11.39 | 339.80 | -30.77 | 116.20 | 0.5612 | 723.0 | 565.9 | |
| 0.00 | 0.52 | 0.00 | 0.30 | -6.92 | 339.71 | -30.86 | 108.52 | 0.5392 | 496.0 | 543.0 | |
| 0.00 | 0.60 | 0.00 | 0.38 | -11.72 | 336.04 | -34.53 | 114.28 | 0.6112 | -550.0 | -470.7 | |
| 0.00 | 0.86 | 0.00 | 0.54 | -8.86 | 335.12 | -35.45 | 109.34 | 0.6097 | -649.0 | -540.2 | |
| 0.00 | 1.03 | 0.00 | 0.65 | -10.85 | 334.83 | -35.74 | 112.26 | 0.6222 | -721.0 | -556.8 | |
| 0.00 | 0.95 | 0.00 | 0.60 | -10.00 | 334.53 | -36.04 | 110.82 | 0.6222 | -510.0 | -485.7 | |
| 0.00 | 1.46 | 0.00 | 0.93 | -10.98 | 334.40 | -36.17 | 112.24 | 0.6283 | -419.0 | -387.3 | |
| 0.00 | 3.36 | 0.00 | 2.12 | -9.49 | 334.41 | -36.16 | 109.97 | 0.6215 | -732.0 | -529.6 | |
| 0.00 | 0.78 | 0.00 | 0.50 | -10.77 | 333.64 | -36.94 | 111.52 | 0.6369 | -636.0 | -514.0 | |
| 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. | |