| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 17.60 | 51.92 | 11.75 | 34.89 | 7.68 | 265.03 | -42.33 | 81.10 | 0.6774 | -768.5 | -507.7 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-11-20 06:58:57 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 |
| 14.85 | 36.64 | 9.77 | 24.09 | 7.42 | 266.35 | -41.01 | 81.31 | 0.6606 | -989.0 | -519.6 | |
| 0.00 | 1.29 | 0.00 | 0.86 | 8.35 | 265.47 | -41.88 | 80.03 | 0.6730 | -515.0 | -320.3 | |
| 0.00 | 1.03 | 0.00 | 0.69 | 5.36 | 265.07 | -42.28 | 84.51 | 0.6753 | -563.0 | -493.8 | |
| 0.00 | 0.94 | 0.00 | 0.64 | 9.38 | 264.59 | -42.76 | 78.67 | 0.6855 | -559.0 | -465.1 | |
| 0.00 | 1.29 | 0.00 | 0.89 | 7.60 | 263.06 | -44.29 | 81.44 | 0.7023 | -615.0 | -470.6 | |
| 0.00 | 1.20 | 0.00 | 0.84 | 7.92 | 262.77 | -44.59 | 81.02 | 0.7063 | -559.0 | -438.2 | |
| 0.00 | 0.94 | 0.00 | 0.67 | 7.90 | 261.92 | -45.43 | 81.15 | 0.7166 | -640.0 | -552.5 | |
| 0.00 | 1.03 | 0.00 | 0.74 | 7.70 | 261.39 | -45.97 | 81.48 | 0.7228 | -643.0 | -571.8 | |
| 0.00 | 1.29 | 0.00 | 0.92 | 8.00 | 261.13 | -46.22 | 81.10 | 0.7261 | -706.0 | -536.9 | |
| 0.00 | 0.94 | 0.00 | 0.68 | 7.76 | 261.08 | -46.28 | 81.44 | 0.7265 | -465.0 | -416.7 | |
| 2.75 | 3.18 | 1.98 | 2.29 | 8.14 | 260.98 | -46.38 | 80.92 | 0.7281 | -657.7 | -577.2 | |
| 0.00 | 1.03 | 0.00 | 0.74 | 8.83 | 260.87 | -46.49 | 79.99 | 0.7300 | -607.0 | -516.2 | |
| 0.00 | 1.12 | 0.00 | 0.84 | 12.20 | 259.16 | -48.20 | 75.72 | 0.7542 | -647.0 | -565.2 | |
| 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. | |