SDO HMI 2014-10-09 10:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.63 | 0.00 | 12.95 | -17.77 | 102.10 | 28.41 | 227.52 | 0.6096 | 176.5 | -7.1 | |
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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 | 0.88 | 0.00 | 0.60 | -15.72 | 112.19 | 38.50 | 239.62 | 0.6970 | 434.0 | 410.3 | |
| 0.00 | 0.79 | 0.00 | 0.54 | -16.12 | 111.96 | 38.28 | 238.96 | 0.6969 | 548.0 | 373.7 | |
| 0.00 | 0.79 | 0.00 | 0.52 | -13.33 | 110.38 | 36.70 | 241.62 | 0.6632 | 612.0 | 471.4 | |
| 0.00 | 1.05 | 0.00 | 0.69 | -13.47 | 110.18 | 36.49 | 241.29 | 0.6617 | 711.0 | 589.0 | |
| 0.00 | 1.58 | 0.00 | 1.04 | -13.30 | 109.99 | 36.31 | 241.40 | 0.6586 | 687.0 | 676.8 | |
| 0.00 | 1.23 | 0.00 | 0.82 | -15.93 | 110.23 | 36.54 | 238.05 | 0.6771 | 741.0 | 572.6 | |
| 0.00 | 0.53 | 0.00 | 0.34 | -15.88 | 107.58 | 33.90 | 236.20 | 0.6478 | 544.0 | 473.3 | |
| 0.00 | 0.96 | 0.00 | 0.65 | -19.00 | 108.02 | 34.33 | 232.53 | 0.6742 | 608.0 | 476.9 | |
| 0.00 | 1.40 | 0.00 | 0.96 | -21.26 | 108.39 | 34.71 | 230.09 | 0.6941 | 456.0 | 311.8 | |
| 0.00 | 0.88 | 0.00 | 0.61 | -22.20 | 108.38 | 34.69 | 228.97 | 0.7009 | 422.0 | 438.4 | |
| 0.00 | 1.32 | 0.00 | 0.82 | -20.12 | 100.66 | 26.97 | 224.52 | 0.6097 | -720.0 | -623.3 | |
| 0.00 | 1.32 | 0.00 | 0.82 | -20.84 | 99.72 | 26.03 | 222.66 | 0.6075 | -98.0 | -175.8 | |
| 0.00 | 1.58 | 0.00 | 0.89 | -13.29 | 95.07 | 21.38 | 227.31 | 0.4846 | -824.0 | -579.8 | |
| 0.00 | 2.72 | 0.00 | 1.59 | -19.55 | 92.74 | 19.05 | 215.60 | 0.5306 | -723.0 | -546.7 | |
| 0.00 | 3.60 | 0.00 | 2.06 | -19.74 | 88.77 | 15.08 | 209.38 | 0.5011 | -750.0 | -664.7 | |
| 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. | |