| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 43.80 | 137.55 | 24.41 | 76.83 | 7.16 | 252.14 | 27.35 | 278.57 | 0.4629 | 270.4 | 82.4 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-07-08 06:00:40 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 |
| 0.73 | 9.09 | 0.41 | 5.19 | 6.80 | 254.54 | 29.76 | 277.34 | 0.4989 | -994.1 | -783.0 | |
| 0.82 | -1.00 | 0.47 | -1.00 | 6.68 | 254.43 | 29.64 | 277.12 | 0.4970 | -1005.2 | 999999 | |
| 1.09 | 4.45 | 0.62 | 2.54 | 7.26 | 254.40 | 29.61 | 278.29 | 0.4973 | -1020.2 | -791.9 | |
| 0.00 | 0.91 | 0.00 | 0.52 | 6.78 | 254.22 | 29.44 | 277.35 | 0.4940 | -1000.0 | -885.4 | |
| 0.00 | 1.18 | 0.00 | 0.67 | 7.82 | 254.23 | 29.44 | 279.44 | 0.4957 | -646.0 | -421.8 | |
| 0.00 | 0.91 | 0.00 | 0.52 | 6.66 | 254.07 | 29.29 | 277.13 | 0.4917 | -645.0 | -516.4 | |
| 7.45 | 18.35 | 4.22 | 10.39 | 6.33 | 253.80 | 29.02 | 276.50 | 0.4872 | -991.4 | -767.3 | |
| 0.00 | 2.18 | 0.00 | 1.24 | 8.11 | 253.79 | 29.01 | 280.13 | 0.4896 | -754.0 | -651.9 | |
| 0.00 | 1.54 | 0.00 | 0.87 | 7.11 | 253.50 | 28.72 | 278.15 | 0.4837 | -845.0 | -621.1 | |
| 0.00 | 0.73 | 0.00 | 0.41 | 7.99 | 253.57 | 28.79 | 279.95 | 0.4861 | -732.0 | -624.4 | |
| 0.00 | 1.09 | 0.00 | 0.62 | 7.54 | 253.46 | 28.68 | 279.04 | 0.4837 | -808.0 | -638.8 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 7.47 | 252.79 | 28.01 | 279.04 | 0.4734 | -596.0 | -526.7 | |
| 0.45 | 2.73 | 0.26 | 1.53 | 8.14 | 252.71 | 27.92 | 280.49 | 0.4734 | 679.2 | 525.2 | |
| 0.00 | 1.00 | 0.00 | 0.56 | 6.26 | 252.30 | 27.52 | 276.56 | 0.4642 | 332.0 | 147.5 | |
| 0.00 | 3.18 | 0.00 | 1.78 | 8.43 | 252.27 | 27.49 | 281.22 | 0.4674 | 549.0 | 361.2 | |
| 0.00 | 1.27 | 0.00 | 0.71 | 8.89 | 252.10 | 27.32 | 282.27 | 0.4659 | 651.0 | 482.9 | |
| 2.27 | 11.99 | 1.27 | 6.69 | 8.44 | 251.96 | 27.18 | 281.34 | 0.4627 | 796.2 | 771.1 | |
| 1.64 | -17.00 | 0.91 | -17.00 | 8.69 | 251.84 | 27.06 | 281.91 | 0.4615 | 905.3 | 999999 | |
| 0.00 | 0.91 | 0.00 | 0.50 | 6.46 | 251.69 | 26.91 | 277.10 | 0.4550 | 407.0 | 348.8 | |
| 0.00 | 0.27 | 0.00 | 0.15 | 7.37 | 251.75 | 26.97 | 279.10 | 0.4573 | 58.0 | 172.7 | |
| 0.00 | 1.54 | 0.00 | 0.86 | 8.08 | 251.76 | 26.98 | 280.62 | 0.4589 | 876.0 | 744.6 | |
| 0.27 | -17.00 | 0.15 | -17.00 | 8.60 | 251.73 | 26.95 | 281.76 | 0.4596 | 1074.7 | 999999 | |
| 0.00 | 1.45 | 0.00 | 0.81 | 8.94 | 251.73 | 26.94 | 282.49 | 0.4603 | 832.0 | 684.9 | |
| 0.64 | 1.91 | 0.35 | 1.06 | 8.70 | 251.57 | 26.79 | 282.03 | 0.4573 | 1003.3 | 802.1 | |
| 9.99 | 58.87 | 5.54 | 32.63 | 6.77 | 251.36 | 26.58 | 277.86 | 0.4504 | 837.2 | 382.6 | |
| 3.09 | -25.00 | 1.71 | -25.00 | 7.45 | 251.41 | 26.63 | 279.34 | 0.4522 | 863.8 | 999999 | |
| 13.54 | -25.00 | 7.50 | -25.00 | 7.08 | 251.21 | 26.43 | 278.59 | 0.4485 | 1008.2 | 999999 | |
| 1.82 | -25.00 | 1.00 | -25.00 | 7.00 | 250.93 | 26.15 | 278.47 | 0.4441 | 1116.8 | 999999 | |
| 0.00 | 2.09 | 0.00 | 1.15 | 7.16 | 250.74 | 25.95 | 278.87 | 0.4413 | 730.0 | 581.2 | |
| 0.00 | 2.73 | 0.00 | 1.50 | 5.94 | 250.50 | 25.71 | 276.15 | 0.4358 | 768.0 | 570.3 | |
| 0.00 | 4.91 | 0.00 | 2.69 | 6.72 | 250.10 | 25.31 | 278.02 | 0.4306 | 798.0 | 700.9 | |
| 0.00 | 1.27 | 0.00 | 0.68 | 6.50 | 246.93 | 22.15 | 278.28 | 0.3801 | 737.0 | 466.9 | |
| 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. | |