SDO HMI 2014-08-05 03:00:39 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 18.46 | 0.00 | 10.97 | -18.83 | 238.59 | 22.60 | 221.15 | 0.5535 | 65.9 | 103.2 | |
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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 |
| 0.00 | 1.27 | 0.00 | 0.77 | -17.65 | 242.77 | 26.78 | 227.65 | 0.5831 | 749.0 | 604.0 | |
| 0.00 | 1.45 | 0.00 | 0.88 | -18.06 | 242.30 | 26.31 | 226.61 | 0.5820 | 643.0 | 462.8 | |
| 0.00 | 1.36 | 0.00 | 0.83 | -19.43 | 241.02 | 25.03 | 223.46 | 0.5823 | 632.0 | 517.1 | |
| 0.00 | 0.54 | 0.00 | 0.33 | -18.18 | 240.76 | 24.76 | 224.75 | 0.5674 | 675.0 | 556.5 | |
| 0.00 | 1.90 | 0.00 | 1.15 | -19.23 | 240.28 | 24.29 | 222.87 | 0.5731 | 863.0 | 747.0 | |
| 0.00 | 0.90 | 0.00 | 0.55 | -19.74 | 240.36 | 24.37 | 222.33 | 0.5789 | 665.0 | 582.7 | |
| 0.00 | 1.18 | 0.00 | 0.71 | -19.85 | 239.99 | 24.00 | 221.76 | 0.5766 | 756.0 | 651.5 | |
| 0.00 | 1.99 | 0.00 | 1.18 | -18.33 | 238.88 | 22.89 | 222.35 | 0.5503 | 760.0 | 586.3 | |
| 0.00 | 0.81 | 0.00 | 0.48 | -19.27 | 237.52 | 21.53 | 219.45 | 0.5473 | -617.0 | -485.3 | |
| 0.00 | 0.72 | 0.00 | 0.42 | -18.55 | 236.98 | 20.98 | 219.64 | 0.5343 | -626.0 | -485.4 | |
| 0.00 | 1.72 | 0.00 | 1.02 | -20.06 | 237.15 | 21.15 | 218.01 | 0.5526 | -773.0 | -664.2 | |
| 0.00 | 1.36 | 0.00 | 0.78 | -17.52 | 236.23 | 20.24 | 219.95 | 0.5158 | -739.0 | -620.2 | |
| 0.00 | 1.18 | 0.00 | 0.68 | -19.48 | 234.35 | 18.36 | 214.87 | 0.5215 | -661.0 | -598.7 | |
| 0.00 | 0.99 | 0.00 | 0.57 | -18.28 | 233.61 | 17.62 | 215.19 | 0.5007 | -692.0 | -579.1 | |
| 0.00 | 1.09 | 0.00 | 0.62 | -18.51 | 233.37 | 17.38 | 214.55 | 0.5014 | -646.0 | -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. | |