| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 12.72 | 40.52 | 6.94 | 22.36 | -12.69 | 59.93 | -17.59 | 137.76 | 0.4383 | 371.9 | -10.5 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-10-09 03:00:32 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 | 1.49 | 0.00 | 0.82 | -14.25 | 62.76 | -14.76 | 144.59 | 0.4280 | 665.0 | 517.6 | |
| 0.00 | 1.05 | 0.00 | 0.56 | -7.23 | 62.49 | -15.03 | 131.83 | 0.3467 | -830.0 | -661.2 | |
| 2.11 | 17.98 | 1.15 | 9.82 | -12.72 | 61.71 | -15.81 | 140.44 | 0.4191 | 1185.6 | 859.5 | |
| 3.33 | -3.00 | 1.82 | -3.00 | -12.97 | 61.69 | -15.83 | 140.80 | 0.4223 | 1070.6 | 999999 | |
| 6.58 | -3.00 | 3.59 | -3.00 | -12.82 | 61.45 | -16.07 | 140.14 | 0.4229 | 972.2 | 999999 | |
| 0.00 | 1.14 | 0.00 | 0.62 | -12.50 | 61.44 | -16.08 | 139.62 | 0.4193 | 369.0 | 369.9 | |
| 0.00 | 1.14 | 0.00 | 0.63 | -14.16 | 61.19 | -16.33 | 141.71 | 0.4417 | 729.0 | 543.5 | |
| 0.00 | 1.40 | 0.00 | 0.78 | -14.27 | 60.86 | -16.66 | 141.30 | 0.4462 | 649.0 | 499.8 | |
| 0.00 | 0.88 | 0.00 | 0.49 | -14.40 | 60.69 | -16.83 | 141.21 | 0.4495 | 699.0 | 547.2 | |
| 0.70 | 10.79 | 0.38 | 5.92 | -11.93 | 59.68 | -17.84 | 135.74 | 0.4313 | -939.6 | -709.0 | |
| 0.00 | 1.58 | 0.00 | 0.88 | -14.43 | 59.10 | -18.42 | 138.70 | 0.4656 | 839.0 | 687.2 | |
| 0.00 | 1.49 | 0.00 | 0.87 | -13.00 | 52.05 | -25.47 | 127.37 | 0.5294 | -822.0 | -613.0 | |
| 0.00 | 0.70 | 0.00 | 0.43 | -12.45 | 46.35 | -31.17 | 121.18 | 0.5930 | -691.0 | -408.5 | |
| 0.00 | 0.88 | 0.00 | 0.54 | -12.96 | 45.77 | -31.74 | 121.46 | 0.6033 | -441.0 | -395.0 | |
| 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. | |