SDO HMI 2014-11-06 19:00:28 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 7.94 | 35.90 | 4.08 | 18.44 | 5.52 | 73.92 | 14.46 | 279.14 | 0.2531 | -155.8 | -87.8 | |
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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 | 3.97 | 0.00 | 2.10 | 2.98 | 79.83 | 20.37 | 268.29 | 0.3493 | 5.0 | 6.5 | |
| 0.00 | 2.85 | 0.00 | 1.50 | 3.93 | 79.85 | 20.39 | 271.02 | 0.3492 | 40.0 | 16.6 | |
| 0.00 | 1.81 | 0.00 | 0.95 | 11.39 | 76.71 | 17.25 | 294.88 | 0.3219 | -852.0 | -646.8 | |
| 0.00 | 0.86 | 0.00 | 0.45 | 4.60 | 76.34 | 16.89 | 273.29 | 0.2914 | -766.0 | -566.0 | |
| 6.04 | 11.48 | 3.11 | 5.91 | 5.63 | 75.38 | 15.92 | 277.16 | 0.2764 | -1090.4 | -779.2 | |
| 1.90 | 5.00 | 0.97 | 2.57 | 5.35 | 74.56 | 15.11 | 276.40 | 0.2623 | -1053.6 | -733.6 | |
| 0.00 | 1.04 | 0.00 | 0.52 | 5.24 | 70.31 | 10.85 | 277.93 | 0.1901 | -750.0 | -595.8 | |
| 0.00 | 2.16 | 0.00 | 1.08 | 5.63 | 67.32 | 7.86 | 283.38 | 0.1406 | 859.0 | 745.3 | |
| 0.00 | 1.81 | 0.00 | 0.91 | 6.11 | 66.57 | 7.12 | 288.28 | 0.1304 | 1039.0 | 829.0 | |
| 0.00 | 1.21 | 0.00 | 0.60 | 5.58 | 66.48 | 7.02 | 284.46 | 0.1262 | 881.0 | 775.1 | |
| 0.00 | 2.24 | 0.00 | 1.12 | 6.50 | 66.01 | 6.55 | 292.71 | 0.1235 | 892.0 | 679.7 | |
| 0.00 | 1.47 | 0.00 | 0.73 | 6.36 | 65.31 | 5.86 | 293.86 | 0.1114 | 872.0 | 610.1 | |
| 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. | |