SDO HMI 2011-11-06 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 |
| 28.08 | 141.46 | 55.18 | 264.03 | 17.92 | 59.72 | -74.94 | 72.47 | 0.9634 | -38.1 | 5.9 | |
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back to the solar disc SDO HMI 2011-11-06 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 |
| 2.42 | 79.80 | 3.72 | 128.58 | 16.62 | 63.11 | -71.56 | 73.77 | 0.9482 | -604.6 | -238.1 | |
| 6.05 | -1.00 | 9.47 | -1.00 | 16.90 | 62.74 | -71.92 | 73.48 | 0.9502 | -629.0 | 999999 | |
| 1.04 | -1.00 | 1.64 | -1.00 | 17.14 | 62.52 | -72.15 | 73.23 | 0.9514 | -604.2 | 999999 | |
| 2.59 | -1.00 | 4.42 | -1.00 | 17.61 | 61.17 | -73.49 | 72.77 | 0.9581 | -227.2 | 999999 | |
| 3.45 | -1.00 | 5.68 | -1.00 | 16.97 | 61.84 | -72.82 | 73.43 | 0.9547 | -346.6 | 999999 | |
| 1.30 | 4.75 | 2.33 | 8.78 | 17.93 | 60.24 | -74.42 | 72.46 | 0.9624 | -147.7 | 329.1 | |
| 0.00 | 1.21 | 0.00 | 2.07 | 17.23 | 61.02 | -73.64 | 73.17 | 0.9587 | -201.0 | -112.9 | |
| 0.00 | 1.21 | 0.00 | 2.22 | 17.75 | 59.86 | -74.81 | 72.65 | 0.9641 | 540.0 | 391.3 | |
| 0.00 | 18.39 | 0.00 | 32.13 | 16.84 | 60.76 | -73.90 | 73.58 | 0.9599 | 310.0 | 231.8 | |
| 0.00 | 1.21 | 0.00 | 2.23 | 17.46 | 59.71 | -74.95 | 72.96 | 0.9647 | 375.0 | 369.8 | |
| 8.90 | 33.68 | 21.60 | 84.71 | 19.62 | 55.84 | -78.83 | 70.76 | 0.9797 | 484.5 | 268.5 | |
| 2.33 | -11.00 | 6.32 | -11.00 | 19.82 | 54.55 | -80.11 | 70.55 | 0.9837 | -173.8 | 999999 | |
| 0.00 | 1.21 | 0.00 | 3.31 | 19.49 | 54.30 | -80.36 | 70.89 | 0.9845 | -169.0 | -112.8 | |
| 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. | |