SDO HMI 2014-11-10 11:00:27 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 | 9.02 | -9.26 | 337.92 | -33.20 | 111.17 | 0.5809 | 6.4 | -42.5 | |
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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 | 1.03 | 0.00 | 0.59 | -6.61 | 342.93 | -28.19 | 109.54 | 0.4999 | 238.0 | 185.6 | |
| 0.00 | 0.95 | 0.00 | 0.55 | -9.99 | 342.28 | -28.84 | 115.25 | 0.5273 | 833.0 | 685.5 | |
| 0.00 | 0.69 | 0.00 | 0.39 | -5.26 | 342.64 | -28.48 | 106.78 | 0.4980 | 685.0 | 643.9 | |
| 0.00 | 1.29 | 0.00 | 0.74 | -5.54 | 342.21 | -28.91 | 107.08 | 0.5054 | 648.0 | 566.5 | |
| 0.00 | 1.12 | 0.00 | 0.66 | -10.12 | 340.98 | -30.13 | 114.54 | 0.5454 | 666.0 | 562.9 | |
| 0.00 | 1.12 | 0.00 | 0.67 | -11.38 | 339.78 | -31.34 | 115.79 | 0.5684 | 732.0 | 581.8 | |
| 0.00 | 0.95 | 0.00 | 0.56 | -6.96 | 339.94 | -31.18 | 108.42 | 0.5437 | 712.0 | 558.8 | |
| 0.00 | 0.78 | 0.00 | 0.48 | -9.86 | 336.65 | -34.46 | 111.43 | 0.6012 | -659.0 | -556.4 | |
| 0.00 | 1.03 | 0.00 | 0.65 | -11.71 | 336.00 | -35.12 | 113.93 | 0.6186 | -698.0 | -535.4 | |
| 0.00 | 0.95 | 0.00 | 0.60 | -10.13 | 334.92 | -36.20 | 110.94 | 0.6248 | -569.0 | -547.2 | |
| 0.00 | 0.95 | 0.00 | 0.60 | -10.87 | 334.78 | -36.34 | 111.98 | 0.6299 | -697.0 | -536.3 | |
| 0.00 | 1.12 | 0.00 | 0.71 | -10.02 | 334.48 | -36.64 | 110.56 | 0.6299 | -600.0 | -466.5 | |
| 0.00 | 1.98 | 0.00 | 1.26 | -9.45 | 334.44 | -36.68 | 109.66 | 0.6280 | -669.0 | -590.3 | |
| 0.00 | 0.86 | 0.00 | 0.56 | -10.45 | 333.66 | -37.46 | 110.79 | 0.6421 | -533.0 | -501.0 | |
| 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. | |