| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 29.17 | 65.17 | 18.98 | 42.54 | 20.06 | 65.17 | -31.20 | 48.34 | 0.6530 | -27.6 | 58.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-02-09 09:58:56 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 |
| 8.30 | 23.69 | 5.28 | 15.11 | 19.67 | 67.21 | -29.15 | 46.98 | 0.6297 | -885.6 | -678.5 | |
| 2.57 | -1.00 | 1.64 | -1.00 | 19.53 | 66.88 | -29.48 | 47.47 | 0.6318 | -879.9 | 999999 | |
| 5.30 | -1.00 | 3.40 | -1.00 | 19.80 | 66.68 | -29.69 | 47.32 | 0.6361 | -715.5 | 999999 | |
| 0.00 | 1.54 | 0.00 | 0.99 | 20.25 | 66.40 | -29.96 | 47.04 | 0.6426 | -376.0 | -289.4 | |
| 0.00 | 5.47 | 0.00 | 3.50 | 19.26 | 66.43 | -29.94 | 48.23 | 0.6340 | -682.0 | -502.9 | |
| 0.00 | 2.82 | 0.00 | 1.82 | 20.13 | 66.21 | -30.15 | 47.36 | 0.6435 | -715.0 | -541.2 | |
| 4.36 | 17.62 | 2.90 | 11.73 | 20.91 | 64.30 | -32.07 | 48.12 | 0.6685 | 850.5 | 637.5 | |
| 0.00 | 1.37 | 0.00 | 0.91 | 21.26 | 64.02 | -32.34 | 47.94 | 0.6739 | 483.0 | 389.8 | |
| 3.25 | -7.00 | 2.16 | -7.00 | 20.51 | 63.79 | -32.57 | 49.02 | 0.6702 | 926.8 | 999999 | |
| 1.20 | 1.37 | 0.80 | 0.91 | 20.38 | 63.33 | -33.03 | 49.57 | 0.6736 | 760.3 | 793.0 | |
| 0.00 | 2.65 | 0.00 | 1.77 | 19.94 | 63.03 | -33.34 | 50.35 | 0.6733 | 768.0 | 644.0 | |
| 2.48 | 7.53 | 1.66 | 5.03 | 19.82 | 62.79 | -33.57 | 50.68 | 0.6748 | 822.4 | 660.7 | |
| 1.71 | -12.00 | 1.14 | -12.00 | 19.63 | 62.72 | -33.64 | 50.97 | 0.6741 | 843.7 | 999999 | |
| 0.00 | 0.43 | 0.00 | 0.29 | 19.96 | 62.60 | -33.76 | 50.66 | 0.6777 | 391.0 | 381.2 | |
| 0.00 | 0.68 | 0.00 | 0.48 | 20.83 | 59.23 | -37.14 | 52.18 | 0.7167 | 562.0 | 482.2 | |
| 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. | |