SDO HMI 2014-10-13 23:00:31 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 64.79 | 354.37 | 57.81 | 319.18 | -8.95 | 319.03 | -54.73 | 104.93 | 0.8346 | 599.6 | 241.6 | |
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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 |
| 24.39 | 303.49 | 20.83 | 260.00 | -8.56 | 321.03 | -52.72 | 104.97 | 0.8167 | 1034.5 | 314.7 | |
| 33.14 | -1.00 | 28.52 | -1.00 | -9.10 | 320.87 | -52.89 | 105.57 | 0.8196 | 835.1 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.72 | -9.86 | 318.51 | -55.25 | 105.78 | 0.8433 | 484.0 | 404.9 | |
| 0.00 | 0.96 | 0.00 | 0.99 | -10.02 | 314.26 | -59.49 | 104.86 | 0.8797 | -557.0 | -416.3 | |
| 0.44 | 2.01 | 0.45 | 2.08 | -8.60 | 314.01 | -59.75 | 103.21 | 0.8793 | -569.8 | -476.4 | |
| 0.00 | 1.75 | 0.00 | 1.90 | -10.10 | 312.76 | -61.00 | 104.59 | 0.8916 | -480.0 | -433.5 | |
| 0.00 | 1.22 | 0.00 | 1.34 | -10.22 | 312.46 | -61.29 | 104.65 | 0.8941 | -371.0 | -350.5 | |
| 0.00 | 1.22 | 0.00 | 1.35 | -10.06 | 312.20 | -61.56 | 104.41 | 0.8958 | -247.0 | -208.1 | |
| 0.00 | 1.05 | 0.00 | 1.15 | -8.34 | 312.14 | -61.61 | 102.51 | 0.8935 | -353.0 | -316.1 | |
| 3.85 | 21.68 | 4.50 | 25.37 | -8.97 | 310.37 | -63.39 | 102.83 | 0.9075 | -582.2 | -156.7 | |
| 1.57 | -10.00 | 1.84 | -10.00 | -8.79 | 310.29 | -63.47 | 102.62 | 0.9078 | -415.4 | 999999 | |
| 1.40 | 15.04 | 1.67 | 18.06 | -9.77 | 309.96 | -63.80 | 103.61 | 0.9116 | -322.3 | 37.6 | |
| 0.00 | 5.16 | 0.00 | 6.22 | -9.10 | 309.56 | -64.20 | 102.81 | 0.9134 | 365.0 | 327.4 | |
| 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. | |