SDO HMI 2014-09-30 07:00:33 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 4.15 | 33.51 | 2.11 | 17.09 | 7.68 | 207.83 | 13.75 | 274.96 | 0.2377 | -73.8 | 14.4 | |
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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 | 1.15 | 0.00 | 0.59 | 7.52 | 210.70 | 16.61 | 273.68 | 0.2853 | -850.0 | -701.2 | |
| 0.00 | 0.44 | 0.00 | 0.23 | 7.50 | 210.50 | 16.42 | 273.62 | 0.2821 | -744.0 | -631.0 | |
| 0.00 | 1.50 | 0.00 | 0.77 | 8.10 | 210.44 | 16.35 | 275.78 | 0.2814 | -807.0 | -733.6 | |
| 0.00 | 1.15 | 0.00 | 0.59 | 7.74 | 210.39 | 16.31 | 274.50 | 0.2803 | -963.0 | -773.9 | |
| 0.00 | 1.59 | 0.00 | 0.82 | 7.42 | 210.31 | 16.23 | 273.34 | 0.2789 | -989.0 | -807.6 | |
| 0.71 | 1.94 | 0.36 | 1.00 | 7.25 | 209.74 | 15.66 | 272.78 | 0.2693 | -823.5 | -686.1 | |
| 0.00 | 4.85 | 0.00 | 2.48 | 6.64 | 208.37 | 14.29 | 270.36 | 0.2463 | -478.0 | -704.7 | |
| 0.00 | 2.29 | 0.00 | 1.17 | 6.65 | 208.09 | 14.01 | 270.36 | 0.2416 | -778.0 | -599.6 | |
| 0.00 | 0.79 | 0.00 | 0.40 | 6.50 | 207.99 | 13.91 | 269.74 | 0.2400 | -908.0 | -786.4 | |
| 2.91 | 8.91 | 1.48 | 4.53 | 8.09 | 207.02 | 12.94 | 276.74 | 0.2242 | 1078.8 | 863.7 | |
| 0.00 | 2.82 | 0.00 | 1.43 | 8.61 | 206.72 | 12.64 | 279.21 | 0.2202 | 1000.0 | 754.5 | |
| 0.00 | 1.68 | 0.00 | 0.85 | 7.80 | 206.63 | 12.55 | 275.56 | 0.2173 | 1001.0 | 808.8 | |
| 0.53 | 1.85 | 0.27 | 0.94 | 8.28 | 206.37 | 12.29 | 277.93 | 0.2136 | 1011.8 | 789.1 | |
| 0.00 | 1.23 | 0.00 | 0.63 | 7.72 | 206.10 | 12.02 | 275.36 | 0.2083 | 772.0 | 550.4 | |
| 0.00 | 1.32 | 0.00 | 0.66 | 8.86 | 203.67 | 9.58 | 283.10 | 0.1697 | 793.0 | 586.3 | |
| 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. | |