SDO HMI 2014-11-09 13:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.37 | 21.37 | 0.71 | 11.22 | -15.18 | 20.18 | -3.03 | 172.71 | 0.3329 | -13.8 | 65.6 | |
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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 | 1.47 | 0.00 | 0.75 | -11.40 | 28.31 | 5.11 | 198.77 | 0.2724 | 942.0 | 804.9 | |
| 0.00 | 1.12 | 0.00 | 0.58 | -14.20 | 26.25 | 3.04 | 189.61 | 0.3096 | 848.0 | 645.1 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -14.42 | 25.30 | 2.09 | 186.57 | 0.3109 | 777.0 | 663.2 | |
| 1.03 | 3.79 | 0.53 | 1.96 | -13.08 | 23.16 | -0.05 | 179.83 | 0.2864 | 1161.3 | 919.2 | |
| 0.00 | 0.78 | 0.00 | 0.40 | -13.79 | 23.00 | -0.20 | 179.33 | 0.2984 | 896.0 | 685.6 | |
| 0.00 | 1.55 | 0.00 | 0.80 | -13.42 | 22.76 | -0.45 | 178.51 | 0.2922 | 996.0 | 753.1 | |
| 0.34 | 2.33 | 0.18 | 1.21 | -14.16 | 22.08 | -1.12 | 176.42 | 0.3052 | 861.5 | 761.9 | |
| 0.00 | 0.86 | 0.00 | 0.45 | -14.82 | 19.81 | -3.40 | 169.65 | 0.3207 | -740.0 | -576.0 | |
| 0.00 | 1.03 | 0.00 | 0.55 | -16.12 | 16.37 | -6.84 | 161.16 | 0.3558 | -799.0 | -637.2 | |
| 0.00 | 2.76 | 0.00 | 1.49 | -18.55 | 15.33 | -7.88 | 160.87 | 0.3983 | -987.0 | -904.8 | |
| 0.00 | 0.86 | 0.00 | 0.46 | -18.29 | 15.28 | -7.93 | 160.53 | 0.3947 | -794.0 | -666.2 | |
| 0.00 | 0.43 | 0.00 | 0.23 | -19.19 | 14.98 | -8.23 | 160.66 | 0.4098 | -556.0 | -447.4 | |
| 0.00 | 1.21 | 0.00 | 0.65 | -18.74 | 14.97 | -8.24 | 160.24 | 0.4031 | -861.0 | -716.2 | |
| 0.00 | 0.43 | 0.00 | 0.23 | -18.88 | 14.46 | -8.75 | 159.24 | 0.4080 | -760.0 | -666.0 | |
| 0.00 | 1.72 | 0.00 | 0.92 | -15.49 | 13.59 | -9.62 | 153.60 | 0.3637 | -797.0 | -692.1 | |
| 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. | |