| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 1.27 | 57.22 | 0.75 | 34.16 | -14.03 | 206.82 | 32.67 | 250.09 | 0.5587 | -159.4 | -368.6 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-01-07 03:58:55 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 |
| 0.00 | 1.02 | 0.00 | 0.64 | -13.31 | 211.59 | 37.44 | 253.07 | 0.6207 | 743.0 | 613.7 | |
| 0.00 | 2.04 | 0.00 | 1.29 | -13.67 | 211.61 | 37.47 | 252.51 | 0.6220 | 704.0 | 617.2 | |
| 0.00 | 0.93 | 0.00 | 0.59 | -13.86 | 211.50 | 37.35 | 252.18 | 0.6210 | 613.0 | 520.5 | |
| 0.00 | 1.36 | 0.00 | 0.86 | -15.81 | 211.70 | 37.56 | 249.20 | 0.6297 | 716.0 | 647.3 | |
| 0.00 | 0.93 | 0.00 | 0.59 | -15.06 | 211.50 | 37.36 | 250.29 | 0.6247 | 834.0 | 691.0 | |
| 0.00 | 2.97 | 0.00 | 1.86 | -15.49 | 210.67 | 36.53 | 249.31 | 0.6154 | 830.0 | 645.3 | |
| 0.00 | 1.10 | 0.00 | 0.69 | -15.76 | 210.69 | 36.54 | 248.89 | 0.6166 | 549.0 | 483.6 | |
| 0.00 | 1.10 | 0.00 | 0.69 | -15.64 | 210.47 | 36.33 | 248.99 | 0.6134 | 759.0 | 661.4 | |
| 0.00 | 1.02 | 0.00 | 0.62 | -14.44 | 208.63 | 34.49 | 250.19 | 0.5850 | -543.0 | -411.1 | |
| 0.00 | 0.93 | 0.00 | 0.56 | -13.83 | 208.05 | 33.90 | 250.98 | 0.5751 | -678.0 | -542.4 | |
| 0.00 | 1.61 | 0.00 | 0.98 | -14.04 | 208.05 | 33.90 | 250.62 | 0.5758 | -544.0 | -460.4 | |
| 0.00 | 1.44 | 0.00 | 0.86 | -13.88 | 206.74 | 32.60 | 250.36 | 0.5575 | -624.0 | -524.0 | |
| 0.00 | 1.78 | 0.00 | 1.06 | -13.68 | 206.53 | 32.39 | 250.62 | 0.5539 | -571.0 | -485.1 | |
| 0.00 | 1.87 | 0.00 | 1.11 | -14.10 | 206.45 | 32.31 | 249.84 | 0.5544 | -577.0 | -494.9 | |
| 0.00 | 1.44 | 0.00 | 0.85 | -13.51 | 206.18 | 32.04 | 250.76 | 0.5485 | -634.0 | -523.4 | |
| 0.00 | 1.10 | 0.00 | 0.65 | -14.04 | 206.27 | 32.12 | 249.85 | 0.5516 | -617.0 | -486.3 | |
| 0.00 | 4.25 | 0.00 | 2.50 | -13.61 | 205.81 | 31.66 | 250.41 | 0.5436 | -695.0 | -668.0 | |
| 1.27 | 1.87 | 0.75 | 1.10 | -14.04 | 205.34 | 31.19 | 249.41 | 0.5389 | -801.4 | -768.0 | |
| 0.00 | 21.33 | 0.00 | 12.48 | -13.57 | 205.16 | 31.01 | 250.18 | 0.5345 | -355.0 | -706.5 | |
| 0.00 | 1.87 | 0.00 | 1.10 | -14.38 | 205.21 | 31.07 | 248.75 | 0.5385 | -755.0 | -682.4 | |
| 0.00 | 0.93 | 0.00 | 0.55 | -14.17 | 205.18 | 31.03 | 249.11 | 0.5372 | -737.0 | -552.9 | |
| 0.00 | 3.06 | 0.00 | 1.78 | -14.00 | 204.80 | 30.65 | 249.22 | 0.5312 | -724.0 | -703.9 | |
| 0.00 | 1.27 | 0.00 | 0.75 | -15.14 | 204.90 | 30.76 | 247.23 | 0.5376 | -720.0 | -570.8 | |
| 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. | |