SDO HMI 2011-07-04 19:59:11 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.78 | 130.55 | 26.67 | 103.36 | 15.52 | 26.50 | 50.60 | 287.38 | 0.7822 | -319.0 | -285.5 | |
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back to the solar disc SDO HMI 2011-07-04 19:59:11 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 | 1.54 | 0.00 | 1.30 | 16.90 | 28.99 | 53.09 | 288.63 | 0.8095 | -480.0 | -360.9 | |
| 18.25 | 88.71 | 14.71 | 71.27 | 15.36 | 27.37 | 51.47 | 287.00 | 0.7910 | -858.4 | -451.5 | |
| 0.00 | 0.36 | 0.00 | 0.29 | 16.08 | 27.52 | 51.62 | 287.87 | 0.7937 | -530.0 | -459.0 | |
| 0.00 | 1.45 | 0.00 | 1.18 | 16.24 | 27.47 | 51.57 | 288.08 | 0.7935 | -500.0 | -406.5 | |
| 4.36 | -2.00 | 3.48 | -2.00 | 14.97 | 26.98 | 51.08 | 286.58 | 0.7864 | -859.1 | 999999 | |
| 0.00 | 0.91 | 0.00 | 0.71 | 15.80 | 25.91 | 50.01 | 287.82 | 0.7766 | -553.0 | -499.8 | |
| 2.18 | 9.62 | 1.70 | 7.51 | 15.37 | 25.67 | 49.77 | 287.32 | 0.7733 | 298.9 | -347.4 | |
| 0.00 | 1.18 | 0.00 | 0.90 | 16.28 | 24.31 | 48.41 | 288.77 | 0.7605 | 217.0 | 111.9 | |
| 0.00 | 4.54 | 0.00 | 3.43 | 15.78 | 24.06 | 48.16 | 288.18 | 0.7568 | 558.0 | 470.7 | |
| 5.45 | 20.88 | 4.11 | 15.76 | 16.51 | 23.96 | 48.06 | 289.15 | 0.7572 | 688.7 | 357.5 | |
| 3.54 | -10.00 | 2.67 | -10.00 | 16.14 | 23.84 | 47.94 | 288.69 | 0.7551 | 766.3 | 999999 | |
| 0.00 | 1.36 | 0.00 | 1.01 | 15.72 | 23.32 | 47.42 | 288.25 | 0.7487 | 778.0 | 593.3 | |
| 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. | |