| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 80.58 | 269.74 | 44.89 | 150.66 | -22.49 | 136.66 | -3.50 | 173.05 | 0.4637 | -56.9 | -129.3 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2011-07-19 14:59:11 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 |
| 1.36 | 1.81 | 0.75 | 1.01 | -21.84 | 143.23 | 3.07 | 186.34 | 0.4515 | 796.7 | 793.2 | |
| 0.00 | 1.27 | 0.00 | 0.68 | -18.05 | 142.58 | 2.42 | 185.91 | 0.3905 | 694.0 | 595.3 | |
| 0.00 | 1.09 | 0.00 | 0.60 | -20.49 | 142.49 | 2.32 | 185.10 | 0.4291 | 861.0 | 672.1 | |
| 0.00 | 2.09 | 0.00 | 1.17 | -23.14 | 142.00 | 1.84 | 183.61 | 0.4700 | 834.0 | 618.0 | |
| 0.00 | 2.45 | 0.00 | 1.37 | -23.28 | 141.74 | 1.57 | 183.07 | 0.4719 | 710.0 | 622.0 | |
| 0.00 | 2.18 | 0.00 | 1.24 | -24.74 | 140.71 | 0.55 | 181.02 | 0.4937 | 682.0 | 550.8 | |
| 0.00 | 0.54 | 0.00 | 0.31 | -24.56 | 140.61 | 0.45 | 180.83 | 0.4910 | 737.0 | 698.7 | |
| 0.00 | 2.18 | 0.00 | 1.22 | -22.83 | 140.41 | 0.24 | 180.49 | 0.4643 | 843.0 | 654.2 | |
| 0.00 | 1.54 | 0.00 | 0.88 | -24.49 | 140.41 | 0.25 | 180.46 | 0.4899 | 772.0 | 567.1 | |
| 2.72 | 10.16 | 1.52 | 5.66 | -22.49 | 139.95 | -0.22 | 179.56 | 0.4589 | 1041.6 | 804.8 | |
| 0.00 | 1.00 | 0.00 | 0.56 | -23.69 | 139.94 | -0.22 | 179.58 | 0.4776 | 808.0 | 641.9 | |
| 2.00 | -10.00 | 1.11 | -10.00 | -22.21 | 139.85 | -0.32 | 179.35 | 0.4547 | 969.0 | 999999 | |
| 0.00 | 0.91 | 0.00 | 0.50 | -20.04 | 139.40 | -0.77 | 178.28 | 0.4207 | 645.0 | 653.9 | |
| 8.71 | 44.45 | 4.84 | 24.66 | -22.25 | 139.26 | -0.91 | 178.14 | 0.4554 | 1030.8 | 614.3 | |
| 0.00 | 3.63 | 0.00 | 2.04 | -23.62 | 139.11 | -1.05 | 177.97 | 0.4768 | 587.0 | 639.2 | |
| 0.00 | 1.36 | 0.00 | 0.76 | -23.11 | 139.12 | -1.05 | 177.94 | 0.4688 | 458.0 | 396.6 | |
| 2.18 | -14.00 | 1.21 | -14.00 | -22.35 | 139.02 | -1.14 | 177.68 | 0.4572 | 811.1 | 999999 | |
| 0.00 | 1.00 | 0.00 | 0.54 | -20.11 | 139.04 | -1.12 | 177.49 | 0.4220 | 793.0 | 690.9 | |
| 0.00 | 3.54 | 0.00 | 1.98 | -22.87 | 138.99 | -1.18 | 177.66 | 0.4652 | 613.0 | 610.7 | |
| 0.00 | 1.45 | 0.00 | 0.82 | -23.56 | 138.95 | -1.22 | 177.65 | 0.4759 | 727.0 | 565.4 | |
| 0.00 | 1.18 | 0.00 | 0.65 | -20.31 | 138.91 | -1.25 | 177.22 | 0.4253 | 782.0 | 670.6 | |
| 0.00 | 1.09 | 0.00 | 0.59 | -20.08 | 138.82 | -1.35 | 176.98 | 0.4216 | 787.0 | 578.8 | |
| 7.98 | -14.00 | 4.41 | -14.00 | -21.60 | 138.67 | -1.49 | 176.87 | 0.4457 | 1061.6 | 999999 | |
| 3.45 | 7.26 | 1.92 | 4.03 | -22.15 | 138.27 | -1.90 | 176.12 | 0.4546 | 734.2 | 291.5 | |
| 0.00 | 1.00 | 0.00 | 0.57 | -24.92 | 137.96 | -2.20 | 175.96 | 0.4975 | 541.0 | 465.4 | |
| 0.00 | 1.18 | 0.00 | 0.67 | -24.78 | 137.90 | -2.27 | 175.82 | 0.4955 | 675.0 | 575.8 | |
| 0.00 | 0.82 | 0.00 | 0.46 | -24.57 | 137.90 | -2.27 | 175.79 | 0.4923 | 601.0 | 615.1 | |
| 0.00 | 1.81 | 0.00 | 1.03 | -24.11 | 137.71 | -2.46 | 175.36 | 0.4856 | 806.0 | 646.3 | |
| 0.00 | 0.82 | 0.00 | 0.46 | -22.90 | 137.63 | -2.53 | 174.98 | 0.4671 | 190.0 | 144.4 | |
| 0.00 | 0.91 | 0.00 | 0.51 | -24.33 | 137.03 | -3.13 | 174.14 | 0.4898 | 705.0 | 479.1 | |
| 3.63 | 46.18 | 2.01 | 25.68 | -21.68 | 136.73 | -3.43 | 172.86 | 0.4496 | -1019.8 | -457.7 | |
| 6.17 | -31.00 | 3.44 | -31.00 | -22.43 | 136.65 | -3.52 | 172.91 | 0.4614 | -796.9 | 999999 | |
| 2.45 | -31.00 | 1.36 | -31.00 | -21.75 | 136.40 | -3.76 | 172.21 | 0.4514 | -928.8 | 999999 | |
| 1.27 | -31.00 | 0.71 | -31.00 | -22.16 | 136.36 | -3.81 | 172.25 | 0.4578 | -749.1 | 999999 | |
| 0.00 | 1.63 | 0.00 | 0.91 | -22.36 | 136.25 | -3.91 | 172.11 | 0.4612 | -553.0 | -482.7 | |
| 4.99 | 44.09 | 2.78 | 24.62 | -22.36 | 135.86 | -4.31 | 171.32 | 0.4621 | -841.9 | -611.0 | |
| 1.36 | -36.00 | 0.76 | -36.00 | -22.16 | 135.77 | -4.40 | 171.06 | 0.4592 | -981.3 | 999999 | |
| 0.00 | 1.00 | 0.00 | 0.57 | -23.92 | 135.37 | -4.79 | 170.94 | 0.4869 | -738.0 | -574.6 | |
| 4.63 | -36.00 | 2.58 | -36.00 | -22.26 | 135.40 | -4.77 | 170.37 | 0.4617 | -1125.3 | 999999 | |
| 5.90 | -36.00 | 3.30 | -36.00 | -22.47 | 135.23 | -4.94 | 170.12 | 0.4653 | -926.5 | 999999 | |
| 0.64 | -36.00 | 0.35 | -36.00 | -21.99 | 135.24 | -4.92 | 169.95 | 0.4579 | -977.3 | 999999 | |
| 0.00 | 3.72 | 0.00 | 2.09 | -22.95 | 134.94 | -5.22 | 169.76 | 0.4734 | -657.0 | -570.4 | |
| 1.54 | 2.18 | 0.86 | 1.22 | -22.30 | 134.77 | -5.40 | 169.15 | 0.4640 | -845.6 | -778.3 | |
| 0.91 | 3.81 | 0.52 | 2.17 | -24.24 | 134.59 | -5.58 | 169.62 | 0.4937 | -899.6 | -714.7 | |
| 0.00 | 2.99 | 0.00 | 1.70 | -23.89 | 134.54 | -5.63 | 169.38 | 0.4886 | -816.0 | -639.7 | |
| 17.15 | 52.62 | 9.60 | 29.40 | -22.44 | 134.37 | -5.80 | 168.43 | 0.4674 | -1072.6 | -641.6 | |
| 1.54 | -46.00 | 0.86 | -46.00 | -22.21 | 134.11 | -6.05 | 167.82 | 0.4646 | -871.4 | 999999 | |
| 0.00 | 2.09 | 0.00 | 1.19 | -24.63 | 133.73 | -6.44 | 168.24 | 0.5020 | -785.0 | -616.9 | |
| 0.00 | 1.18 | 0.00 | 0.67 | -23.56 | 132.64 | -7.52 | 165.77 | 0.4900 | -825.0 | -643.8 | |
| 0.00 | 1.27 | 0.00 | 0.73 | -24.61 | 132.55 | -7.62 | 166.16 | 0.5056 | -755.0 | -607.1 | |
| 0.00 | 4.72 | 0.00 | 2.70 | -24.51 | 132.25 | -7.91 | 165.58 | 0.5053 | -721.0 | -532.8 | |
| 0.00 | 0.91 | 0.00 | 0.52 | -24.90 | 131.78 | -8.38 | 165.00 | 0.5127 | -582.0 | -425.7 | |
| 0.00 | 1.09 | 0.00 | 0.63 | -24.97 | 131.40 | -8.76 | 164.40 | 0.5153 | -712.0 | -562.1 | |
| 0.00 | 1.54 | 0.00 | 0.89 | -23.75 | 128.95 | -11.21 | 159.47 | 0.5094 | 624.0 | 461.2 | |
| 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. | |