SDO HMI 2011-07-02 09:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 0.64 | 16.63 | 0.34 | 8.81 | 16.75 | 23.38 | 15.48 | 313.26 | 0.3543 | -170.2 | 41.4 | |
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back to the solar disc SDO HMI 2011-07-02 09:59:11 UT
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 | 0.82 | 0.00 | 0.44 | 16.29 | 27.83 | 19.93 | 305.47 | 0.4035 | -747.0 | -591.4 | |
| 0.64 | 2.36 | 0.34 | 1.26 | 13.35 | 26.82 | 18.92 | 300.06 | 0.3661 | 1015.6 | 796.3 | |
| 0.00 | 1.64 | 0.00 | 0.87 | 16.43 | 25.30 | 17.40 | 309.30 | 0.3722 | -824.0 | -578.9 | |
| 0.00 | 0.82 | 0.00 | 0.45 | 21.05 | 25.73 | 17.83 | 317.56 | 0.4251 | -782.0 | -680.7 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 16.86 | 23.78 | 15.87 | 312.71 | 0.3578 | -843.0 | -615.2 | |
| 0.00 | 1.54 | 0.00 | 0.81 | 15.83 | 23.29 | 15.39 | 311.27 | 0.3412 | -967.0 | -763.2 | |
| 0.00 | 1.00 | 0.00 | 0.55 | 23.51 | 23.00 | 15.10 | 325.86 | 0.4275 | -730.0 | -526.2 | |
| 0.00 | 0.91 | 0.00 | 0.48 | 17.58 | 21.59 | 13.69 | 318.32 | 0.3407 | -698.0 | -519.7 | |
| 0.00 | 3.91 | 0.00 | 2.04 | 16.38 | 21.30 | 13.40 | 316.35 | 0.3236 | 780.0 | 669.3 | |
| 0.00 | 1.27 | 0.00 | 0.67 | 16.76 | 21.17 | 13.27 | 317.47 | 0.3264 | 616.0 | 448.1 | |
| 0.00 | 1.45 | 0.00 | 0.76 | 16.93 | 20.26 | 12.36 | 319.77 | 0.3185 | 904.0 | 628.1 | |
| 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. | |