| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 13.84 | 39.14 | 15.90 | 43.31 | 34.53 | 263.87 | 54.04 | 311.80 | 0.8949 | 27.7 | 122.9 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-01-04 10:58:55 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 |
| 2.80 | 3.99 | 3.67 | 5.23 | 33.24 | 270.38 | 60.55 | 308.12 | 0.9274 | -410.6 | -212.6 | |
| 1.02 | 1.78 | 1.34 | 2.35 | 33.50 | 270.39 | 60.56 | 308.38 | 0.9280 | -261.1 | -199.1 | |
| 1.95 | 3.14 | 2.29 | 3.69 | 33.73 | 266.60 | 56.76 | 309.88 | 0.9083 | -294.7 | -286.0 | |
| 1.70 | 3.31 | 1.91 | 3.72 | 33.44 | 265.16 | 55.32 | 310.11 | 0.8991 | -288.4 | -265.1 | |
| 0.00 | 1.19 | 0.00 | 1.31 | 33.05 | 264.73 | 54.90 | 309.88 | 0.8954 | -396.0 | -347.0 | |
| 0.00 | 0.76 | 0.00 | 0.84 | 34.13 | 263.85 | 54.01 | 311.32 | 0.8937 | -338.0 | -268.1 | |
| 1.44 | 2.97 | 1.54 | 3.17 | 34.54 | 262.54 | 52.71 | 312.26 | 0.8874 | -360.7 | -243.1 | |
| 2.38 | 6.71 | 2.50 | 7.04 | 34.91 | 261.69 | 51.85 | 312.99 | 0.8836 | 472.9 | 290.6 | |
| 0.00 | 2.29 | 0.00 | 2.47 | 35.57 | 262.24 | 52.40 | 313.42 | 0.8893 | 297.0 | 233.6 | |
| 0.00 | 2.55 | 0.00 | 2.67 | 35.19 | 261.36 | 51.52 | 313.41 | 0.8827 | 500.0 | 387.2 | |
| 0.00 | 1.53 | 0.00 | 1.61 | 35.71 | 261.36 | 51.52 | 313.94 | 0.8847 | 196.0 | 118.7 | |
| 2.55 | 4.25 | 2.65 | 4.42 | 35.50 | 260.94 | 51.10 | 313.91 | 0.8814 | 529.0 | 428.0 | |
| 0.00 | 1.61 | 0.00 | 1.67 | 35.78 | 260.49 | 50.66 | 314.38 | 0.8798 | 469.0 | 373.7 | |
| 0.00 | 0.51 | 0.00 | 0.53 | 35.96 | 260.31 | 50.47 | 314.64 | 0.8794 | 399.0 | 435.8 | |
| 0.00 | 2.55 | 0.00 | 2.59 | 35.53 | 259.87 | 50.03 | 314.40 | 0.8751 | 588.0 | 432.9 | |
| 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. | |