SDO HMI 2014-10-09 04:00:32 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 16.05 | 0.00 | 10.04 | -17.03 | 106.15 | 29.18 | 229.95 | 0.6100 | 109.5 | 186.5 | |
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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 | 1.75 | 0.00 | 1.15 | -16.58 | 111.01 | 34.04 | 235.37 | 0.6543 | 542.0 | 494.0 | |
| 0.00 | 1.32 | 0.00 | 0.83 | -13.36 | 110.32 | 33.35 | 239.21 | 0.6249 | 740.0 | 489.4 | |
| 0.00 | 1.40 | 0.00 | 0.89 | -13.44 | 110.00 | 33.03 | 238.86 | 0.6217 | 732.0 | 619.2 | |
| 0.00 | 1.14 | 0.00 | 0.74 | -16.64 | 110.57 | 33.60 | 234.94 | 0.6500 | 781.0 | 641.5 | |
| 0.00 | 0.88 | 0.00 | 0.55 | -13.30 | 109.83 | 32.86 | 238.93 | 0.6188 | 753.0 | 663.5 | |
| 0.00 | 1.14 | 0.00 | 0.73 | -15.85 | 110.23 | 33.26 | 235.72 | 0.6407 | 726.0 | 611.5 | |
| 0.00 | 0.88 | 0.00 | 0.55 | -13.50 | 109.54 | 32.57 | 238.41 | 0.6167 | 487.0 | 376.9 | |
| 0.00 | 1.14 | 0.00 | 0.74 | -18.60 | 108.94 | 31.97 | 231.10 | 0.6472 | 535.0 | 355.5 | |
| 0.00 | 1.23 | 0.00 | 0.82 | -22.36 | 108.34 | 31.37 | 226.02 | 0.6715 | 692.0 | 566.6 | |
| 0.00 | 0.53 | 0.00 | 0.31 | -16.03 | 100.83 | 23.86 | 226.36 | 0.5394 | -712.0 | -584.3 | |
| 0.00 | 1.14 | 0.00 | 0.68 | -19.03 | 100.01 | 23.04 | 221.41 | 0.5614 | -760.0 | -605.3 | |
| 0.00 | 1.05 | 0.00 | 0.64 | -21.09 | 99.84 | 22.87 | 218.75 | 0.5815 | -663.0 | -571.5 | |
| 0.00 | 0.96 | 0.00 | 0.56 | -18.02 | 97.19 | 20.22 | 219.04 | 0.5238 | -769.0 | -657.5 | |
| 0.00 | 0.70 | 0.00 | 0.40 | -19.37 | 92.71 | 15.74 | 210.81 | 0.5016 | -778.0 | -684.6 | |
| 0.00 | 0.79 | 0.00 | 0.45 | -19.82 | 92.29 | 15.32 | 209.66 | 0.5043 | -664.0 | -601.9 | |
| 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. | |