SDO HMI 2011-06-12 23:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.00 | 30.43 | 0.00 | 16.68 | -15.72 | 245.84 | -19.04 | 132.37 | 0.4246 | 213.9 | 247.8 | |
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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 | 2.08 | 0.00 | 1.11 | -15.24 | 250.60 | -14.29 | 139.07 | 0.3651 | 933.0 | 791.5 | |
| 0.00 | 0.45 | 0.00 | 0.24 | -15.09 | 250.51 | -14.38 | 138.60 | 0.3642 | 378.0 | 470.2 | |
| 0.00 | 1.63 | 0.00 | 0.87 | -15.28 | 250.40 | -14.49 | 138.74 | 0.3676 | 1070.0 | 793.9 | |
| 0.00 | 3.62 | 0.00 | 1.93 | -15.06 | 250.19 | -14.70 | 137.92 | 0.3673 | 1103.0 | 890.5 | |
| 0.00 | 1.18 | 0.00 | 0.64 | -15.22 | 247.41 | -17.47 | 133.42 | 0.4006 | 814.0 | 622.0 | |
| 0.00 | 2.45 | 0.00 | 1.32 | -14.75 | 247.39 | -17.50 | 132.47 | 0.3959 | 888.0 | 755.4 | |
| 0.00 | 1.99 | 0.00 | 1.08 | -15.35 | 247.11 | -17.78 | 133.17 | 0.4055 | 845.0 | 620.6 | |
| 0.00 | 1.18 | 0.00 | 0.64 | -15.51 | 246.99 | -17.90 | 133.29 | 0.4085 | 697.0 | 540.9 | |
| 0.00 | 3.71 | 0.00 | 2.03 | -14.85 | 245.45 | -19.44 | 129.78 | 0.4203 | 731.0 | 629.9 | |
| 0.00 | 1.99 | 0.00 | 1.13 | -18.92 | 243.56 | -21.32 | 134.27 | 0.4823 | 718.0 | 537.7 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -15.53 | 243.26 | -21.63 | 128.15 | 0.4535 | -827.0 | -615.3 | |
| 0.00 | 1.00 | 0.00 | 0.55 | -15.72 | 243.03 | -21.85 | 128.22 | 0.4579 | -797.0 | -571.4 | |
| 0.00 | 1.27 | 0.00 | 0.71 | -15.56 | 242.51 | -22.38 | 127.30 | 0.4631 | -795.0 | -652.8 | |
| 0.00 | 1.99 | 0.00 | 1.12 | -16.84 | 242.28 | -22.61 | 129.27 | 0.4771 | -735.0 | -609.0 | |
| 0.00 | 1.45 | 0.00 | 0.81 | -15.34 | 242.16 | -22.73 | 126.50 | 0.4655 | -764.0 | -567.6 | |
| 0.00 | 3.35 | 0.00 | 1.90 | -16.75 | 241.60 | -23.29 | 128.32 | 0.4844 | -836.0 | -666.3 | |
| 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. | |