| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.85 | 202.82 | 42.70 | 198.08 | 14.11 | 252.05 | -59.14 | 74.98 | 0.8640 | -379.3 | -182.6 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-19 23:58:57 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 |
| 32.09 | 183.42 | 31.02 | 178.02 | 14.20 | 252.41 | -58.78 | 74.83 | 0.8610 | -777.0 | -226.5 | |
| 0.77 | -1.00 | 0.75 | -1.00 | 13.67 | 252.10 | -59.10 | 75.47 | 0.8633 | 462.9 | 999999 | |
| 6.26 | -1.00 | 6.19 | -1.00 | 13.84 | 251.66 | -59.53 | 75.33 | 0.8671 | 482.2 | 999999 | |
| 1.72 | -1.00 | 1.69 | -1.00 | 13.51 | 251.74 | -59.45 | 75.70 | 0.8662 | -294.4 | 999999 | |
| 0.00 | 1.63 | 0.00 | 1.64 | 14.25 | 251.06 | -60.13 | 74.92 | 0.8725 | 467.0 | 355.1 | |
| 1.89 | 3.86 | 1.92 | 3.93 | 14.63 | 250.76 | -60.43 | 74.52 | 0.8753 | -359.4 | -258.3 | |
| 0.00 | 4.46 | 0.00 | 4.58 | 14.59 | 250.40 | -60.79 | 74.60 | 0.8781 | 21.0 | -70.9 | |
| 1.12 | 1.89 | 1.13 | 1.91 | 13.17 | 250.72 | -60.47 | 76.19 | 0.8745 | 439.1 | 431.8 | |
| 0.00 | 3.09 | 0.00 | 3.18 | 14.10 | 250.31 | -60.88 | 75.17 | 0.8785 | 343.0 | 302.0 | |
| 0.00 | 0.69 | 0.00 | 0.72 | 14.45 | 249.77 | -61.43 | 74.83 | 0.8831 | 483.0 | 421.6 | |
| 0.00 | 1.20 | 0.00 | 1.28 | 14.16 | 249.25 | -61.94 | 75.21 | 0.8869 | 467.0 | 403.1 | |
| 0.00 | 1.12 | 0.00 | 1.25 | 15.54 | 247.86 | -63.33 | 73.79 | 0.8984 | 444.0 | 356.7 | |
| 0.00 | 1.46 | 0.00 | 1.57 | 11.32 | 248.71 | -62.48 | 78.45 | 0.8895 | 387.0 | 421.2 | |
| Proj. U | - Projected umbra area in millionths of solar disc, negative values indicate | |
|
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. |
||
| Proj. WS | - Projected whole spot area in millionths of solar disc, negative values indicate | |
|
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. |
||
| 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. | |