| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 72.25 | 378.46 | 49.98 | 261.15 | -13.54 | 169.23 | -44.39 | 102.32 | 0.6980 | 569.8 | 322.1 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-03-22 04:00:30 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 |
| 27.14 | 228.27 | 18.27 | 154.07 | -14.32 | 170.82 | -42.80 | 103.58 | 0.6796 | 1160.6 | 365.8 | |
| 1.48 | -1.00 | 1.00 | -1.00 | -14.50 | 170.44 | -43.18 | 103.79 | 0.6845 | 490.0 | 999999 | |
| 0.00 | 0.52 | 0.00 | 0.35 | -11.82 | 170.66 | -42.97 | 99.88 | 0.6795 | 715.0 | 623.5 | |
| 11.78 | -1.00 | 8.02 | -1.00 | -14.20 | 170.09 | -43.53 | 103.31 | 0.6885 | 755.3 | 999999 | |
| 0.00 | 0.79 | 0.00 | 0.53 | -11.64 | 170.65 | -42.97 | 99.61 | 0.6795 | 660.0 | 580.9 | |
| 0.00 | 1.22 | 0.00 | 0.83 | -12.04 | 170.32 | -43.30 | 100.17 | 0.6838 | 585.0 | 527.3 | |
| 0.00 | 6.63 | 0.00 | 4.49 | -11.58 | 170.28 | -43.34 | 99.50 | 0.6840 | 760.0 | 698.2 | |
| 0.00 | 0.79 | 0.00 | 0.54 | -14.48 | 169.46 | -44.16 | 103.64 | 0.6964 | 375.0 | 260.1 | |
| 0.00 | 1.22 | 0.00 | 0.84 | -13.42 | 169.12 | -44.50 | 102.08 | 0.6996 | -555.0 | -469.2 | |
| 0.00 | 0.35 | 0.00 | 0.25 | -14.28 | 168.20 | -45.42 | 103.21 | 0.7113 | 529.0 | 470.2 | |
| 22.60 | 97.47 | 15.78 | 68.03 | -12.54 | 168.45 | -45.17 | 100.78 | 0.7070 | 1044.6 | 371.8 | |
| 1.05 | 2.18 | 0.74 | 1.54 | -13.64 | 167.75 | -45.87 | 102.26 | 0.7162 | 457.7 | 320.5 | |
| 0.00 | 1.31 | 0.00 | 0.93 | -12.65 | 167.55 | -46.07 | 100.87 | 0.7179 | 415.0 | 311.3 | |
| 0.00 | 1.05 | 0.00 | 0.76 | -15.19 | 166.74 | -46.88 | 104.32 | 0.7293 | 427.0 | 362.9 | |
| 0.00 | 1.83 | 0.00 | 1.30 | -11.88 | 167.46 | -46.16 | 99.80 | 0.7186 | 443.0 | 341.8 | |
| 0.00 | 1.05 | 0.00 | 0.75 | -13.28 | 166.81 | -46.81 | 101.70 | 0.7270 | -729.0 | -603.0 | |
| 0.00 | 0.96 | 0.00 | 0.69 | -12.87 | 166.92 | -46.71 | 101.13 | 0.7255 | 424.0 | 289.4 | |
| 0.00 | 0.96 | 0.00 | 0.69 | -12.98 | 166.53 | -47.09 | 101.27 | 0.7301 | -568.0 | -508.5 | |
| 0.00 | 0.87 | 0.00 | 0.63 | -12.87 | 166.24 | -47.38 | 101.09 | 0.7334 | -614.0 | -514.7 | |
| 4.97 | 8.64 | 3.68 | 6.39 | -13.56 | 165.18 | -48.44 | 101.97 | 0.7459 | -785.6 | -542.0 | |
| 0.00 | 0.61 | 0.00 | 0.45 | -13.07 | 165.17 | -48.45 | 101.32 | 0.7457 | -570.0 | -519.9 | |
| 0.00 | 1.75 | 0.00 | 1.30 | -13.93 | 164.89 | -48.73 | 102.45 | 0.7494 | -537.0 | -464.1 | |
| 0.00 | 0.79 | 0.00 | 0.58 | -11.75 | 165.28 | -48.35 | 99.54 | 0.7441 | 526.0 | 458.4 | |
| 0.00 | 1.83 | 0.00 | 1.38 | -10.10 | 164.44 | -49.19 | 97.32 | 0.7535 | 445.0 | 442.9 | |
| 0.00 | 0.79 | 0.00 | 0.59 | -9.70 | 164.29 | -49.34 | 96.79 | 0.7553 | 537.0 | 479.1 | |
| 1.83 | 3.75 | 1.39 | 2.84 | -9.97 | 164.00 | -49.63 | 97.15 | 0.7585 | 556.0 | 324.6 | |
| 0.96 | 3.32 | 0.74 | 2.54 | -11.64 | 163.38 | -50.25 | 99.35 | 0.7655 | -679.3 | -512.6 | |
| 0.00 | 1.22 | 0.00 | 0.95 | -10.25 | 162.84 | -50.79 | 97.54 | 0.7714 | 688.0 | 599.1 | |
| 0.00 | 1.57 | 0.00 | 1.22 | -9.95 | 162.81 | -50.81 | 97.15 | 0.7717 | 546.0 | 417.6 | |
| 0.00 | 0.87 | 0.00 | 0.69 | -10.07 | 161.81 | -51.82 | 97.32 | 0.7826 | 410.0 | 328.1 | |
| 0.00 | 0.61 | 0.00 | 0.49 | -10.55 | 161.14 | -52.48 | 97.94 | 0.7895 | 441.0 | 329.6 | |
| 0.44 | 1.66 | 0.36 | 1.39 | -15.71 | 159.45 | -54.17 | 104.38 | 0.8079 | -692.2 | -606.1 | |
| 0.00 | 0.79 | 0.00 | 0.66 | -16.36 | 159.14 | -54.48 | 105.16 | 0.8114 | -600.0 | -569.8 | |
| 0.00 | 0.87 | 0.00 | 0.76 | -12.01 | 157.58 | -56.04 | 99.80 | 0.8255 | -432.0 | -383.0 | |
| 0.00 | 0.87 | 0.00 | 0.76 | -11.16 | 157.57 | -56.05 | 98.76 | 0.8257 | -473.0 | -372.9 | |
| 0.00 | 1.05 | 0.00 | 0.94 | -11.91 | 156.27 | -57.35 | 99.69 | 0.8379 | -427.0 | -370.3 | |
| 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. | |