SDO HMI 2011-10-24 04:59:01 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 20.34 | 0.00 | 10.79 | 16.93 | 321.45 | 17.00 | 305.89 | 0.3574 | 761.5 | 633.6 | |
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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 | 0.96 | 0.00 | 0.51 | 12.17 | 325.67 | 21.22 | 289.87 | 0.3779 | 602.0 | 571.6 | |
| 0.00 | 1.65 | 0.00 | 0.89 | 17.10 | 324.84 | 20.39 | 302.50 | 0.3966 | 804.0 | 475.8 | |
| 0.00 | 1.48 | 0.00 | 0.80 | 17.72 | 324.48 | 20.03 | 304.31 | 0.3967 | 877.0 | 735.6 | |
| 0.00 | 0.96 | 0.00 | 0.51 | 16.34 | 322.71 | 18.27 | 303.38 | 0.3618 | 684.0 | 547.1 | |
| 0.00 | 3.04 | 0.00 | 1.59 | 12.79 | 321.86 | 17.42 | 295.10 | 0.3238 | 908.0 | 693.3 | |
| 0.00 | 2.35 | 0.00 | 1.23 | 12.55 | 321.69 | 17.24 | 294.62 | 0.3197 | 877.0 | 801.1 | |
| 0.00 | 1.30 | 0.00 | 0.68 | 12.82 | 321.64 | 17.20 | 295.46 | 0.3207 | 845.0 | 668.7 | |
| 0.00 | 0.87 | 0.00 | 0.45 | 12.56 | 321.46 | 17.02 | 294.90 | 0.3163 | 663.0 | 688.6 | |
| 0.00 | 1.04 | 0.00 | 0.55 | 16.86 | 321.20 | 16.75 | 306.82 | 0.3460 | 718.0 | 588.1 | |
| 0.00 | 1.30 | 0.00 | 0.69 | 19.57 | 319.69 | 15.24 | 315.47 | 0.3547 | 754.0 | 481.1 | |
| 0.00 | 1.30 | 0.00 | 0.69 | 19.49 | 318.86 | 14.42 | 316.83 | 0.3445 | 813.0 | 607.3 | |
| 0.00 | 2.52 | 0.00 | 1.35 | 22.50 | 319.00 | 14.55 | 322.34 | 0.3815 | 763.0 | 651.2 | |
| 0.00 | 1.57 | 0.00 | 0.85 | 25.84 | 318.02 | 13.58 | 329.27 | 0.4152 | 591.0 | 528.2 | |
| 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. | |