SDO HMI 2011-11-02 01:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 80.99 | 572.82 | 212.97 | 1923.84 | 18.84 | 107.63 | -79.78 | 71.61 | 0.9815 | 153.3 | 98.7 | |
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back to the solar disc SDO HMI 2011-11-02 01:58:59 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 |
| 2.68 | 6.49 | 6.69 | 16.17 | 22.19 | 108.06 | -79.35 | 68.22 | 0.9809 | -435.2 | -449.0 | |
| 0.00 | 1.73 | 0.00 | 5.52 | 21.57 | 105.31 | -82.09 | 68.82 | 0.9886 | 30.0 | 127.2 | |
| 12.98 | 526.00 | 26.31 | 1750.90 | 18.61 | 110.84 | -76.57 | 71.88 | 0.9710 | -631.9 | 71.3 | |
| 0.26 | -3.00 | 0.55 | -3.00 | 19.06 | 110.16 | -77.25 | 71.42 | 0.9736 | 12.0 | 999999 | |
| 14.45 | -3.00 | 31.64 | -3.00 | 19.16 | 109.72 | -77.69 | 71.32 | 0.9753 | -391.8 | 999999 | |
| 13.85 | -3.00 | 31.53 | -3.00 | 18.99 | 109.21 | -78.19 | 71.49 | 0.9771 | 323.5 | 999999 | |
| 6.14 | 38.60 | 26.32 | 151.25 | 20.71 | 102.80 | -84.60 | 69.61 | 0.9940 | 592.4 | 483.9 | |
| 0.26 | -3.00 | 0.64 | -3.00 | 18.66 | 108.14 | -79.27 | 71.81 | 0.9807 | -28.0 | 999999 | |
| 3.72 | -3.00 | 9.12 | -3.00 | 18.30 | 108.28 | -79.13 | 72.19 | 0.9803 | -170.5 | 999999 | |
| 9.69 | -3.00 | 25.01 | -3.00 | 18.37 | 107.61 | -79.80 | 72.10 | 0.9824 | 330.7 | 999999 | |
| 2.86 | -3.00 | 9.63 | -3.00 | 19.59 | 104.84 | -82.57 | 70.81 | 0.9898 | 590.7 | 999999 | |
| 1.64 | -3.00 | 4.16 | -3.00 | 17.98 | 107.80 | -79.61 | 72.51 | 0.9818 | -133.3 | 999999 | |
| 8.31 | -3.00 | 27.97 | -3.00 | 18.24 | 104.96 | -82.45 | 72.17 | 0.9896 | 767.8 | 999999 | |
| 4.15 | -3.00 | 13.40 | -3.00 | 17.73 | 105.26 | -82.15 | 72.70 | 0.9890 | 418.1 | 999999 | |
| 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. | |