SDO HMI 2014-11-27 13:00:25 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 58.61 | 370.46 | 36.72 | 233.34 | 16.06 | 110.35 | -35.58 | 65.19 | 0.6181 | -798.1 | -271.4 | |
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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 |
| 57.41 | 356.35 | 35.96 | 223.66 | 16.04 | 110.63 | -35.30 | 65.10 | 0.6146 | -1165.3 | -310.3 | |
| 1.20 | -1.00 | 0.76 | -1.00 | 16.46 | 109.93 | -36.00 | 64.82 | 0.6252 | -494.0 | 999999 | |
| 0.00 | 1.11 | 0.00 | 0.73 | 16.51 | 107.12 | -38.82 | 66.07 | 0.6598 | 650.0 | 633.8 | |
| 0.00 | 2.82 | 0.00 | 1.87 | 17.47 | 106.80 | -39.13 | 64.85 | 0.6674 | 651.0 | 613.5 | |
| 0.00 | 1.37 | 0.00 | 0.92 | 16.13 | 105.53 | -40.41 | 67.30 | 0.6774 | 683.0 | 557.9 | |
| 0.00 | 1.45 | 0.00 | 0.99 | 16.17 | 104.53 | -41.40 | 67.62 | 0.6893 | 585.0 | 410.6 | |
| 0.00 | 1.03 | 0.00 | 0.70 | 15.96 | 104.34 | -41.59 | 67.99 | 0.6908 | -239.0 | -185.0 | |
| 0.00 | 2.22 | 0.00 | 1.56 | 16.39 | 102.72 | -43.22 | 67.97 | 0.7110 | 720.0 | 618.1 | |
| 0.00 | 1.71 | 0.00 | 1.21 | 16.36 | 102.30 | -43.63 | 68.17 | 0.7156 | 444.0 | 401.6 | |
| 0.00 | 0.60 | 0.00 | 0.42 | 16.51 | 102.22 | -43.72 | 67.99 | 0.7170 | 430.0 | 403.0 | |
| 0.00 | 0.94 | 0.00 | 0.67 | 15.67 | 101.76 | -44.17 | 69.27 | 0.7197 | 633.0 | 564.5 | |
| 0.00 | 0.86 | 0.00 | 0.61 | 15.58 | 101.49 | -44.45 | 69.49 | 0.7225 | 435.0 | 391.9 | |
| 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. | |