SDO HMI 2014-01-11 22:00:24 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 76.28 | 464.92 | 45.38 | 277.24 | -16.35 | 13.60 | -32.11 | 113.44 | 0.5580 | 964.2 | 347.0 | |
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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 |
| 45.79 | 454.16 | 27.10 | 270.23 | -16.40 | 14.28 | -31.44 | 113.86 | 0.5493 | 1327.7 | 368.6 | |
| 1.44 | -1.00 | 0.86 | -1.00 | -16.50 | 13.75 | -31.96 | 113.76 | 0.5567 | 781.0 | 999999 | |
| 0.00 | 0.85 | 0.00 | 0.51 | -19.09 | 13.11 | -32.60 | 117.73 | 0.5775 | 703.0 | 568.4 | |
| 0.00 | 0.93 | 0.00 | 0.56 | -14.91 | 13.35 | -32.37 | 110.81 | 0.5556 | 622.0 | 479.0 | |
| 29.05 | -1.00 | 17.42 | -1.00 | -16.23 | 13.00 | -32.71 | 112.91 | 0.5655 | 1154.1 | 999999 | |
| 0.00 | 0.59 | 0.00 | 0.38 | -16.66 | 7.54 | -38.17 | 111.28 | 0.6377 | -590.0 | -514.3 | |
| 0.00 | 1.61 | 0.00 | 1.05 | -17.62 | 6.62 | -39.09 | 112.39 | 0.6523 | -48.0 | -105.7 | |
| 0.00 | 1.61 | 0.00 | 1.04 | -14.52 | 7.07 | -38.64 | 107.84 | 0.6373 | -635.0 | -583.2 | |
| 0.00 | 0.93 | 0.00 | 0.61 | -17.21 | 6.21 | -39.50 | 111.62 | 0.6560 | -631.0 | -542.1 | |
| 0.00 | 1.19 | 0.00 | 0.78 | -15.31 | 5.76 | -39.96 | 108.64 | 0.6560 | -804.0 | -694.2 | |
| 0.00 | 0.76 | 0.00 | 0.52 | -19.02 | 4.39 | -41.32 | 113.61 | 0.6836 | -565.0 | -551.2 | |
| 0.00 | 1.02 | 0.00 | 0.69 | -18.22 | 4.38 | -41.33 | 112.47 | 0.6811 | -629.0 | -574.9 | |
| 0.00 | 1.27 | 0.00 | 0.87 | -17.99 | 3.41 | -42.30 | 111.82 | 0.6919 | -784.0 | -593.5 | |
| 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. | |