SDO HMI 2014-10-03 13:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 40.29 | 153.77 | 24.87 | 94.96 | -13.26 | 120.12 | -31.09 | 122.80 | 0.5999 | 481.8 | 210.2 | |
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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 |
| 28.15 | 127.64 | 17.25 | 78.24 | -13.02 | 120.75 | -30.45 | 122.97 | 0.5908 | 978.4 | 337.2 | |
| 7.21 | -1.00 | 4.45 | -1.00 | -13.33 | 120.39 | -30.82 | 123.10 | 0.5973 | 513.5 | 999999 | |
| 0.00 | 3.34 | 0.00 | 2.08 | -13.69 | 119.72 | -31.49 | 123.06 | 0.6077 | 483.0 | 304.1 | |
| 0.44 | 1.58 | 0.27 | 0.98 | -11.76 | 118.65 | -32.55 | 119.43 | 0.6071 | 691.0 | 574.5 | |
| 1.76 | 8.44 | 1.13 | 5.41 | -15.05 | 118.03 | -33.18 | 123.57 | 0.6365 | -704.8 | -614.3 | |
| 1.32 | -5.00 | 0.85 | -5.00 | -14.74 | 117.79 | -33.42 | 122.96 | 0.6372 | -645.9 | 999999 | |
| 0.00 | 1.32 | 0.00 | 0.84 | -14.11 | 117.71 | -33.50 | 122.04 | 0.6337 | 529.0 | 339.5 | |
| 0.00 | 1.50 | 0.00 | 0.94 | -12.67 | 117.83 | -33.38 | 120.12 | 0.6228 | -745.0 | -629.8 | |
| 0.00 | 0.53 | 0.00 | 0.34 | -15.46 | 117.13 | -34.08 | 123.43 | 0.6494 | -774.0 | -674.3 | |
| 0.00 | 0.62 | 0.00 | 0.40 | -13.73 | 116.61 | -34.59 | 120.71 | 0.6438 | -661.0 | -538.7 | |
| 0.79 | 3.34 | 0.52 | 2.18 | -14.77 | 116.31 | -34.89 | 121.91 | 0.6539 | -712.4 | -604.3 | |
| 0.00 | 1.50 | 0.00 | 0.98 | -14.18 | 116.08 | -35.13 | 120.94 | 0.6527 | -314.0 | -235.5 | |
| 0.62 | 3.96 | 0.40 | 2.57 | -13.40 | 115.92 | -35.29 | 119.76 | 0.6497 | -717.3 | -582.2 | |
| 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. | |