SDO HMI 2014-11-05 02:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.41 | 25.67 | 2.52 | 14.46 | -17.42 | 100.18 | 18.22 | 218.87 | 0.4779 | -111.2 | 81.8 | |
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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 | 0.83 | -14.93 | 104.35 | 22.39 | 229.07 | 0.4891 | -739.0 | -677.9 | |
| 0.00 | 1.30 | 0.00 | 0.73 | -14.86 | 104.18 | 22.22 | 228.97 | 0.4865 | -792.0 | -581.0 | |
| 2.85 | 11.41 | 1.63 | 6.53 | -16.88 | 104.04 | 22.08 | 225.68 | 0.5048 | 852.3 | 743.2 | |
| 1.56 | -3.00 | 0.89 | -3.00 | -16.72 | 104.02 | 22.06 | 225.89 | 0.5030 | 1022.2 | 999999 | |
| 0.00 | 1.38 | 0.00 | 0.77 | -16.73 | 100.87 | 18.91 | 221.56 | 0.4699 | 838.0 | 637.8 | |
| 0.00 | 1.30 | 0.00 | 0.73 | -17.80 | 100.43 | 18.46 | 219.35 | 0.4776 | 505.0 | 418.4 | |
| 0.00 | 1.38 | 0.00 | 0.78 | -17.61 | 100.34 | 18.38 | 219.49 | 0.4745 | 741.0 | 483.9 | |
| 0.00 | 0.95 | 0.00 | 0.53 | -17.67 | 97.25 | 15.29 | 214.42 | 0.4463 | -689.0 | -555.9 | |
| 0.00 | 0.78 | 0.00 | 0.42 | -16.38 | 94.65 | 12.69 | 211.32 | 0.4072 | -736.0 | -511.3 | |
| 0.00 | 0.60 | 0.00 | 0.33 | -17.96 | 93.77 | 11.81 | 207.60 | 0.4219 | -844.0 | -722.4 | |
| 0.00 | 1.30 | 0.00 | 0.71 | -18.02 | 93.55 | 11.59 | 207.10 | 0.4211 | -881.0 | -699.7 | |
| 0.00 | 2.68 | 0.00 | 1.49 | -21.81 | 89.99 | 8.03 | 196.62 | 0.4553 | -483.0 | -405.9 | |
| 0.00 | 1.12 | 0.00 | 0.61 | -19.19 | 89.60 | 7.64 | 197.73 | 0.4143 | -723.0 | -560.4 | |
| 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. | |