SDO HMI 2014-11-08 08:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 20.36 | 49.96 | 17.05 | 40.32 | -5.22 | 90.49 | 51.37 | 260.44 | 0.7900 | 220.1 | 90.5 | |
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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 |
| 14.32 | 22.78 | 12.29 | 19.54 | -4.78 | 93.27 | 54.15 | 261.55 | 0.8188 | 639.5 | 421.4 | |
| 0.00 | 1.90 | 0.00 | 1.55 | -3.42 | 91.34 | 52.22 | 262.91 | 0.7973 | 597.0 | 497.1 | |
| 1.55 | 7.25 | 1.24 | 5.79 | -5.70 | 90.03 | 50.90 | 259.82 | 0.7869 | 682.8 | 503.0 | |
| 2.16 | -3.00 | 1.73 | -3.00 | -5.97 | 90.01 | 50.89 | 259.48 | 0.7872 | 590.2 | 999999 | |
| 0.00 | 1.47 | 0.00 | 1.17 | -5.65 | 89.78 | 50.66 | 259.82 | 0.7842 | 761.0 | 657.4 | |
| 0.00 | 1.55 | 0.00 | 1.21 | -6.32 | 88.70 | 49.57 | 258.74 | 0.7737 | -385.0 | -238.6 | |
| 0.00 | 1.98 | 0.00 | 1.53 | -6.12 | 88.30 | 49.18 | 258.91 | 0.7690 | -495.0 | -384.2 | |
| 2.33 | 4.31 | 1.79 | 3.31 | -6.25 | 87.95 | 48.83 | 258.66 | 0.7655 | -662.9 | -488.6 | |
| 0.00 | 1.64 | 0.00 | 1.20 | -5.44 | 85.94 | 46.81 | 259.27 | 0.7411 | -84.0 | -94.5 | |
| 0.00 | 1.55 | 0.00 | 1.13 | -4.52 | 85.59 | 46.47 | 260.42 | 0.7353 | -720.0 | -620.7 | |
| 0.00 | 1.12 | 0.00 | 0.81 | -4.54 | 85.38 | 46.25 | 260.35 | 0.7328 | -457.0 | -516.2 | |
| 0.00 | 1.47 | 0.00 | 1.06 | -4.11 | 85.30 | 46.18 | 260.90 | 0.7311 | -219.0 | -203.3 | |
| 0.00 | 0.95 | 0.00 | 0.69 | -4.47 | 85.24 | 46.12 | 260.41 | 0.7311 | -525.0 | -500.7 | |
| 0.00 | 0.95 | 0.00 | 0.64 | -8.07 | 80.79 | 41.66 | 254.16 | 0.6865 | -340.0 | -291.9 | |
| 0.00 | 1.04 | 0.00 | 0.69 | -8.05 | 79.62 | 40.50 | 253.77 | 0.6721 | -501.0 | -438.3 | |
| 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. | |