SDO HMI 2011-06-13 10:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 5.08 | 41.96 | 2.70 | 22.22 | -15.24 | 245.86 | -12.99 | 142.11 | 0.3536 | 213.2 | 361.7 | |
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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 | 1.90 | 0.00 | 0.99 | -14.94 | 252.26 | -6.59 | 157.76 | 0.2941 | 667.0 | 452.0 | |
| 0.00 | 1.27 | 0.00 | 0.67 | -17.04 | 251.01 | -7.84 | 156.91 | 0.3342 | 781.0 | 603.5 | |
| 0.00 | 1.36 | 0.00 | 0.71 | -14.44 | 248.02 | -10.83 | 145.27 | 0.3208 | 922.0 | 712.9 | |
| 0.00 | 1.45 | 0.00 | 0.76 | -14.63 | 247.85 | -11.00 | 145.20 | 0.3250 | 883.0 | 657.0 | |
| 0.00 | 3.35 | 0.00 | 1.77 | -15.62 | 247.41 | -11.44 | 145.90 | 0.3422 | 1011.0 | 792.8 | |
| 0.00 | 1.18 | 0.00 | 0.62 | -15.33 | 247.33 | -11.52 | 145.22 | 0.3392 | 781.0 | 583.5 | |
| 0.00 | 1.54 | 0.00 | 0.82 | -16.83 | 246.88 | -11.97 | 146.72 | 0.3633 | 96.0 | 134.8 | |
| 1.27 | 15.23 | 0.67 | 8.04 | -14.73 | 245.81 | -13.04 | 140.78 | 0.3465 | 989.4 | 727.5 | |
| 0.00 | 1.54 | 0.00 | 0.81 | -14.45 | 245.57 | -13.28 | 139.73 | 0.3455 | 865.0 | 650.6 | |
| 0.91 | -8.00 | 0.48 | -8.00 | -14.70 | 245.43 | -13.42 | 139.92 | 0.3502 | 934.2 | 999999 | |
| 0.00 | 2.99 | 0.00 | 1.58 | -14.89 | 245.06 | -13.79 | 139.53 | 0.3564 | 641.0 | 369.8 | |
| 0.00 | 3.44 | 0.00 | 1.84 | -15.91 | 243.81 | -15.04 | 139.00 | 0.3819 | -804.0 | -722.0 | |
| 0.00 | 1.36 | 0.00 | 0.73 | -15.25 | 243.67 | -15.18 | 137.51 | 0.3757 | -1076.0 | -837.9 | |
| 2.90 | 3.17 | 1.55 | 1.70 | -15.53 | 243.55 | -15.30 | 137.82 | 0.3803 | -1077.6 | -988.0 | |
| 0.00 | 0.91 | 0.00 | 0.49 | -15.92 | 242.66 | -16.19 | 136.95 | 0.3944 | -921.0 | -740.6 | |
| 0.00 | 1.27 | 0.00 | 0.69 | -17.49 | 241.79 | -17.06 | 138.21 | 0.4216 | -661.0 | -505.7 | |
| 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. | |