SDO HMI 2011-11-06 00:58:59 UT
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| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 32.04 | 128.05 | 61.21 | 247.86 | 17.92 | 59.90 | -75.31 | 72.47 | 0.9648 | -113.5 | 43.7 | |
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back to the solar disc SDO HMI 2011-11-06 00:58:59 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 |
| 16.32 | 88.08 | 26.09 | 148.99 | 16.79 | 62.88 | -72.33 | 73.61 | 0.9522 | -549.8 | -119.2 | |
| 2.59 | -1.00 | 4.58 | -1.00 | 17.64 | 61.12 | -74.09 | 72.76 | 0.9609 | -272.9 | 999999 | |
| 3.28 | -1.00 | 5.59 | -1.00 | 16.99 | 61.71 | -73.50 | 73.42 | 0.9581 | -318.8 | 999999 | |
| 0.86 | -1.00 | 1.55 | -1.00 | 17.59 | 60.83 | -74.39 | 72.82 | 0.9622 | 154.7 | 999999 | |
| 0.00 | 2.85 | 0.00 | 5.25 | 17.49 | 60.34 | -74.88 | 72.92 | 0.9644 | 121.0 | 190.2 | |
| 0.00 | 0.86 | 0.00 | 1.64 | 17.77 | 59.87 | -75.34 | 72.63 | 0.9665 | 430.0 | 407.5 | |
| 0.00 | 1.12 | 0.00 | 2.17 | 17.94 | 59.53 | -75.68 | 72.47 | 0.9679 | 502.0 | 389.4 | |
| 0.00 | 1.21 | 0.00 | 2.31 | 17.54 | 59.65 | -75.56 | 72.88 | 0.9674 | 377.0 | 392.3 | |
| 0.00 | 0.86 | 0.00 | 1.65 | 17.36 | 59.75 | -75.46 | 73.06 | 0.9669 | 401.0 | 376.7 | |
| 6.74 | 33.07 | 16.99 | 85.85 | 19.59 | 55.92 | -79.29 | 70.79 | 0.9812 | 529.7 | 278.1 | |
| 2.25 | -10.00 | 6.41 | -10.00 | 19.81 | 54.52 | -80.69 | 70.55 | 0.9854 | -188.2 | 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. | |