SDO HMI 2011-10-06 00:59:03 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.55 | 197.38 | 17.52 | 103.18 | -11.49 | 179.32 | -4.76 | 165.37 | 0.3208 | 488.3 | 361.1 | |
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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 |
| 33.55 | 181.30 | 17.52 | 94.63 | -11.37 | 179.69 | -4.39 | 166.24 | 0.3169 | 1243.1 | 439.5 | |
| 0.00 | 3.25 | 0.00 | 1.70 | -11.82 | 178.67 | -5.41 | 163.60 | 0.3285 | 853.0 | 695.1 | |
| 0.00 | 1.67 | 0.00 | 0.88 | -12.29 | 177.09 | -7.00 | 159.67 | 0.3440 | -947.0 | -694.3 | |
| 0.00 | 1.58 | 0.00 | 0.84 | -12.57 | 176.87 | -7.22 | 159.37 | 0.3497 | -887.0 | -714.8 | |
| 0.00 | 1.05 | 0.00 | 0.57 | -14.79 | 174.13 | -9.96 | 155.18 | 0.3999 | -555.0 | -377.5 | |
| 0.00 | 0.35 | 0.00 | 0.19 | -12.59 | 174.13 | -9.95 | 152.59 | 0.3681 | -565.0 | -612.8 | |
| 0.00 | 1.23 | 0.00 | 0.66 | -14.64 | 174.01 | -10.07 | 154.75 | 0.3984 | -732.0 | -574.1 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -14.42 | 173.64 | -10.44 | 153.70 | 0.3979 | -664.0 | -467.7 | |
| 0.00 | 2.11 | 0.00 | 1.12 | -12.38 | 173.67 | -10.41 | 151.24 | 0.3685 | -981.0 | -751.3 | |
| 0.00 | 0.88 | 0.00 | 0.47 | -12.76 | 173.47 | -10.62 | 151.28 | 0.3756 | -779.0 | -615.6 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -13.02 | 173.33 | -10.75 | 151.31 | 0.3803 | -859.0 | -621.7 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -12.18 | 172.52 | -11.56 | 148.37 | 0.3751 | -526.0 | -454.2 | |
| 0.00 | 0.97 | 0.00 | 0.52 | -11.96 | 172.53 | -11.55 | 148.07 | 0.3720 | -723.0 | -537.9 | |
| 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. | |