SDO HMI 2014-11-09 22:00:27 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 19.57 | 0.00 | 10.29 | -15.54 | 18.74 | 0.50 | 182.25 | 0.3346 | -79.6 | -67.4 | |
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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 | 1.55 | 0.00 | 0.81 | -13.64 | 23.67 | 5.42 | 197.35 | 0.3094 | 940.0 | 819.0 | |
| 0.00 | 1.55 | 0.00 | 0.81 | -13.18 | 23.38 | 5.14 | 196.95 | 0.3005 | 786.0 | 629.3 | |
| 0.00 | 1.03 | 0.00 | 0.54 | -14.57 | 23.32 | 5.08 | 195.47 | 0.3226 | 957.0 | 715.8 | |
| 0.00 | 2.33 | 0.00 | 1.21 | -14.32 | 23.19 | 4.95 | 195.31 | 0.3180 | 850.0 | 618.7 | |
| 0.00 | 1.21 | 0.00 | 0.63 | -14.07 | 22.23 | 3.99 | 192.63 | 0.3100 | 840.0 | 615.2 | |
| 0.00 | 1.55 | 0.00 | 0.81 | -13.91 | 21.62 | 3.38 | 190.84 | 0.3054 | 825.0 | 554.3 | |
| 0.00 | 1.21 | 0.00 | 0.63 | -15.49 | 17.05 | -1.19 | 176.47 | 0.3270 | -696.0 | -590.4 | |
| 0.00 | 1.90 | 0.00 | 1.00 | -16.25 | 16.80 | -1.45 | 175.89 | 0.3397 | -948.0 | -723.1 | |
| 0.00 | 0.34 | 0.00 | 0.18 | -18.63 | 15.52 | -2.72 | 173.18 | 0.3805 | -720.0 | -577.2 | |
| 0.00 | 2.67 | 0.00 | 1.43 | -18.47 | 15.27 | -2.97 | 172.51 | 0.3785 | -1009.0 | -871.7 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -18.86 | 15.08 | -3.17 | 172.17 | 0.3851 | -621.0 | -590.1 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -18.67 | 15.02 | -3.22 | 171.95 | 0.3821 | -973.0 | -801.7 | |
| 0.00 | 1.38 | 0.00 | 0.72 | -12.98 | 12.58 | -5.66 | 161.23 | 0.3001 | -836.0 | -657.7 | |
| 0.00 | 0.95 | 0.00 | 0.50 | -17.12 | 11.90 | -6.34 | 163.27 | 0.3684 | -510.0 | -415.1 | |
| 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. | |