SDO HMI 2014-11-03 22:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 11.58 | 32.86 | 6.17 | 17.56 | -17.34 | 98.90 | 1.55 | 184.50 | 0.3775 | -27.9 | -189.9 | |
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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 |
| 9.25 | 14.35 | 4.93 | 7.64 | -16.48 | 103.95 | 6.59 | 197.40 | 0.3698 | 1024.8 | 732.7 | |
| 2.33 | 3.63 | 1.24 | 1.93 | -16.87 | 100.41 | 3.05 | 188.10 | 0.3632 | 1037.1 | 822.2 | |
| 0.00 | 1.04 | 0.00 | 0.55 | -16.99 | 99.16 | 1.81 | 184.80 | 0.3629 | 653.0 | 603.4 | |
| 0.00 | 0.78 | 0.00 | 0.42 | -18.17 | 96.51 | -0.84 | 177.90 | 0.3811 | -712.0 | -585.7 | |
| 0.00 | 0.78 | 0.00 | 0.41 | -16.73 | 94.32 | -3.04 | 171.89 | 0.3610 | -695.0 | -577.8 | |
| 0.00 | 2.85 | 0.00 | 1.52 | -17.53 | 94.27 | -3.08 | 172.09 | 0.3739 | -547.0 | -689.9 | |
| 0.00 | 1.73 | 0.00 | 0.92 | -17.63 | 93.99 | -3.36 | 171.41 | 0.3762 | -795.0 | -641.2 | |
| 0.00 | 2.77 | 0.00 | 1.48 | -18.20 | 93.79 | -3.56 | 171.16 | 0.3859 | -747.0 | -736.3 | |
| 0.00 | 0.95 | 0.00 | 0.51 | -17.47 | 93.62 | -3.74 | 170.41 | 0.3746 | -802.0 | -720.0 | |
| 0.00 | 0.78 | 0.00 | 0.41 | -13.90 | 93.38 | -3.97 | 167.72 | 0.3177 | -871.0 | -684.1 | |
| 0.00 | 0.86 | 0.00 | 0.47 | -19.54 | 91.42 | -5.94 | 166.33 | 0.4144 | -846.0 | -797.9 | |
| 0.00 | 1.73 | 0.00 | 0.96 | -21.54 | 90.88 | -6.47 | 166.38 | 0.4470 | -870.0 | -667.5 | |
| 0.00 | 0.61 | 0.00 | 0.34 | -23.26 | 88.91 | -8.44 | 163.62 | 0.4805 | -585.0 | -523.1 | |
| 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. | |