SDO HMI 2014-08-01 17:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 15.11 | 38.85 | 8.54 | 21.96 | -20.30 | 248.88 | -12.31 | 155.64 | 0.4829 | 575.9 | 320.4 | |
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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 | 2.35 | 0.00 | 1.28 | -17.08 | 251.39 | -9.80 | 157.21 | 0.4220 | -775.0 | -604.7 | |
| 0.54 | 1.81 | 0.30 | 1.00 | -18.41 | 251.15 | -10.04 | 157.96 | 0.4427 | 806.5 | 705.7 | |
| 0.00 | 1.09 | 0.00 | 0.59 | -17.31 | 251.18 | -10.01 | 157.01 | 0.4267 | -496.0 | -487.0 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -18.11 | 250.97 | -10.22 | 157.34 | 0.4395 | 819.0 | 589.1 | |
| 0.00 | 1.27 | 0.00 | 0.70 | -17.75 | 250.83 | -10.36 | 156.72 | 0.4351 | 639.0 | 533.9 | |
| 0.00 | 1.00 | 0.00 | 0.53 | -14.24 | 250.73 | -10.46 | 152.72 | 0.3855 | 757.0 | 562.2 | |
| 0.00 | 1.00 | 0.00 | 0.58 | -22.91 | 249.02 | -12.17 | 157.90 | 0.5183 | 719.0 | 489.7 | |
| 0.00 | 1.09 | 0.00 | 0.63 | -22.94 | 248.88 | -12.31 | 157.70 | 0.5196 | 648.0 | 559.8 | |
| 14.57 | 22.71 | 8.24 | 12.84 | -20.47 | 249.00 | -12.20 | 155.81 | 0.4849 | 990.7 | 645.4 | |
| 0.00 | 1.99 | 0.00 | 1.11 | -18.95 | 248.88 | -12.31 | 154.18 | 0.4647 | 828.0 | 664.2 | |
| 0.00 | 1.00 | 0.00 | 0.61 | -27.82 | 247.18 | -14.01 | 158.78 | 0.5935 | -579.0 | -467.4 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -19.22 | 247.34 | -13.85 | 151.73 | 0.4792 | 686.0 | 542.9 | |
| 0.00 | 1.45 | 0.00 | 0.93 | -27.08 | 238.00 | -23.19 | 146.80 | 0.6425 | -629.0 | -547.4 | |
| 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. | |