SDO HMI 2014-11-29 09:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 22.41 | 0.00 | 13.79 | -23.36 | 94.11 | -27.65 | 134.15 | 0.5953 | -164.1 | 43.0 | |
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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 |
| 0.00 | 0.68 | 0.00 | 0.40 | -24.10 | 101.13 | -20.63 | 142.87 | 0.5349 | 712.0 | 562.2 | |
| 0.00 | 2.91 | 0.00 | 1.74 | -23.12 | 97.11 | -24.65 | 136.82 | 0.5627 | 193.0 | 273.9 | |
| 0.00 | 0.77 | 0.00 | 0.46 | -22.31 | 96.92 | -24.84 | 135.52 | 0.5569 | 774.0 | 573.2 | |
| 0.00 | 1.63 | 0.00 | 1.00 | -23.92 | 94.83 | -26.93 | 135.48 | 0.5928 | 660.0 | 481.8 | |
| 0.00 | 5.47 | 0.00 | 3.35 | -23.66 | 94.78 | -26.98 | 135.09 | 0.5910 | 750.0 | 707.0 | |
| 0.00 | 1.37 | 0.00 | 0.83 | -22.20 | 95.09 | -26.67 | 133.45 | 0.5746 | -493.0 | -425.4 | |
| 0.00 | 0.94 | 0.00 | 0.58 | -24.06 | 93.55 | -28.21 | 134.43 | 0.6067 | -603.0 | -467.3 | |
| 0.00 | 0.86 | 0.00 | 0.53 | -23.71 | 93.01 | -28.75 | 133.47 | 0.6091 | -594.0 | -519.2 | |
| 0.00 | 1.20 | 0.00 | 0.75 | -24.30 | 92.75 | -29.01 | 133.99 | 0.6167 | -673.0 | -590.0 | |
| 0.00 | 2.22 | 0.00 | 1.40 | -23.78 | 91.91 | -29.85 | 132.58 | 0.6208 | -731.0 | -584.3 | |
| 0.00 | 1.28 | 0.00 | 0.81 | -23.46 | 91.47 | -30.29 | 131.78 | 0.6227 | -227.0 | -273.5 | |
| 0.00 | 1.03 | 0.00 | 0.65 | -23.36 | 91.24 | -30.53 | 131.45 | 0.6244 | -478.0 | -386.6 | |
| 0.00 | 0.68 | 0.00 | 0.42 | -20.18 | 91.77 | -30.00 | 127.54 | 0.5941 | -602.0 | -460.1 | |
| 0.00 | 0.60 | 0.00 | 0.37 | -19.96 | 91.48 | -30.28 | 126.99 | 0.5956 | -585.0 | -377.4 | |
| 0.00 | 0.77 | 0.00 | 0.50 | -24.72 | 89.88 | -31.88 | 132.06 | 0.6486 | -564.0 | -504.9 | |
| 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. | |