SDO HMI 2014-07-09 23:00:40 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!)
| group | Proj. U | Proj. WS | Corr. U | Corr. WS | B | L | LCM | Pos. angle | r | MU | MP |
| 33.22 | 118.23 | 20.58 | 73.72 | 9.28 | 165.03 | -37.13 | 79.64 | 0.6071 | -219.1 | -56.6 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-07-09 23:00:40 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 |
| 0.00 | 1.18 | 0.00 | 0.69 | 8.09 | 170.12 | -32.04 | 80.82 | 0.5342 | -882.0 | -684.8 | |
| 0.00 | 1.27 | 0.00 | 0.74 | 7.88 | 170.06 | -32.10 | 81.24 | 0.5346 | -869.0 | -651.6 | |
| 2.27 | 3.63 | 1.33 | 2.13 | 9.06 | 169.84 | -32.32 | 79.08 | 0.5398 | -989.0 | -760.9 | |
| 0.00 | 1.36 | 0.00 | 0.80 | 9.09 | 169.55 | -32.61 | 79.11 | 0.5440 | -814.0 | -651.2 | |
| 3.99 | 7.81 | 2.35 | 4.60 | 8.50 | 169.50 | -32.67 | 80.19 | 0.5438 | -1011.8 | -769.6 | |
| 0.00 | 1.63 | 0.00 | 0.97 | 9.39 | 169.37 | -32.79 | 78.60 | 0.5472 | -787.0 | -649.6 | |
| 0.00 | 1.91 | 0.00 | 1.12 | 8.10 | 169.46 | -32.70 | 80.93 | 0.5437 | -903.0 | -728.4 | |
| 0.00 | 0.91 | 0.00 | 0.54 | 8.74 | 169.18 | -32.98 | 79.83 | 0.5488 | -459.0 | -391.9 | |
| 0.00 | 1.63 | 0.00 | 0.97 | 7.88 | 169.26 | -32.90 | 81.37 | 0.5463 | -711.0 | -601.5 | |
| 0.00 | 2.18 | 0.00 | 1.29 | 8.09 | 169.20 | -32.96 | 80.99 | 0.5474 | -799.0 | -724.6 | |
| 0.00 | 1.36 | 0.00 | 0.81 | 8.52 | 169.13 | -33.03 | 80.23 | 0.5492 | -619.0 | -566.5 | |
| 0.00 | 0.36 | 0.00 | 0.21 | 8.33 | 169.07 | -33.09 | 80.58 | 0.5497 | -526.0 | -455.8 | |
| 0.00 | 0.64 | 0.00 | 0.38 | 10.20 | 168.80 | -33.36 | 77.29 | 0.5570 | -659.0 | -684.3 | |
| 0.00 | 2.09 | 0.00 | 1.25 | 10.38 | 168.70 | -33.46 | 76.99 | 0.5587 | -654.0 | -578.8 | |
| 0.00 | 1.27 | 0.00 | 0.75 | 7.78 | 168.97 | -33.19 | 81.60 | 0.5503 | -678.0 | -488.7 | |
| 0.00 | 0.82 | 0.00 | 0.49 | 10.90 | 168.60 | -33.56 | 76.10 | 0.5613 | -607.0 | -481.1 | |
| 0.00 | 0.73 | 0.00 | 0.43 | 7.27 | 168.39 | -33.77 | 82.60 | 0.5582 | -645.0 | -462.0 | |
| 0.00 | 2.54 | 0.00 | 1.56 | 11.35 | 166.54 | -35.62 | 75.90 | 0.5910 | -471.0 | -462.9 | |
| 0.00 | 0.82 | 0.00 | 0.50 | 9.11 | 166.02 | -36.14 | 79.76 | 0.5939 | -276.0 | -208.7 | |
| 1.45 | 3.00 | 0.90 | 1.85 | 9.44 | 165.83 | -36.33 | 79.25 | 0.5971 | 748.9 | 547.3 | |
| 6.36 | 8.72 | 3.92 | 5.38 | 8.64 | 165.58 | -36.58 | 80.64 | 0.5994 | -778.7 | -422.8 | |
| 0.00 | 1.36 | 0.00 | 0.85 | 9.44 | 164.86 | -37.30 | 79.43 | 0.6103 | 844.0 | 640.0 | |
| 0.45 | 1.54 | 0.28 | 0.97 | 9.34 | 164.68 | -37.48 | 79.62 | 0.6126 | 850.2 | 722.1 | |
| 0.00 | 1.27 | 0.00 | 0.80 | 9.76 | 164.59 | -37.57 | 78.94 | 0.6145 | 603.0 | 434.2 | |
| 0.36 | 2.18 | 0.23 | 1.37 | 9.14 | 164.32 | -37.85 | 80.00 | 0.6173 | 826.8 | 561.7 | |
| 0.00 | 1.82 | 0.00 | 1.15 | 11.77 | 163.86 | -38.30 | 75.89 | 0.6279 | 668.0 | 570.0 | |
| 14.25 | 30.78 | 8.97 | 19.36 | 8.37 | 164.17 | -37.99 | 81.27 | 0.6183 | -955.6 | -509.3 | |
| 0.00 | 1.54 | 0.00 | 0.98 | 9.97 | 163.65 | -38.51 | 78.78 | 0.6274 | 785.0 | 665.1 | |
| 0.73 | 2.18 | 0.46 | 1.39 | 11.44 | 163.27 | -38.89 | 76.54 | 0.6349 | 854.9 | 760.4 | |
| 0.64 | 1.91 | 0.40 | 1.21 | 8.92 | 163.51 | -38.65 | 80.47 | 0.6278 | -600.9 | -432.3 | |
| 0.00 | 1.72 | 0.00 | 1.11 | 11.34 | 163.09 | -39.07 | 76.74 | 0.6372 | 409.0 | 585.6 | |
| 0.27 | 9.26 | 0.17 | 5.94 | 10.53 | 163.05 | -39.11 | 78.00 | 0.6362 | 984.3 | 723.9 | |
| 0.00 | 0.91 | 0.00 | 0.58 | 10.93 | 162.99 | -39.17 | 77.39 | 0.6377 | 642.0 | 611.1 | |
| 2.45 | -32.00 | 1.57 | -32.00 | 10.62 | 162.92 | -39.24 | 77.89 | 0.6381 | 973.1 | 999999 | |
| 0.00 | 0.91 | 0.00 | 0.58 | 9.24 | 163.04 | -39.12 | 80.03 | 0.6346 | -518.0 | -436.8 | |
| 0.00 | 4.45 | 0.00 | 2.87 | 10.98 | 162.66 | -39.50 | 77.38 | 0.6421 | 528.0 | 545.4 | |
| 0.00 | 1.45 | 0.00 | 0.94 | 10.77 | 162.70 | -39.46 | 77.70 | 0.6413 | 710.0 | 571.7 | |
| 0.00 | 2.09 | 0.00 | 1.37 | 12.55 | 161.90 | -40.26 | 75.13 | 0.6549 | 600.0 | 472.5 | |
| 0.00 | 2.27 | 0.00 | 1.48 | 12.25 | 161.92 | -40.24 | 75.59 | 0.6541 | 701.0 | 569.4 | |
| 0.00 | 1.00 | 0.00 | 0.65 | 9.55 | 161.46 | -40.70 | 79.78 | 0.6557 | 657.0 | 625.5 | |
| 0.00 | 0.73 | 0.00 | 0.47 | 6.08 | 161.42 | -40.74 | 85.09 | 0.6537 | -599.0 | -531.5 | |
| 0.00 | 1.27 | 0.00 | 0.90 | 8.06 | 156.27 | -45.89 | 82.45 | 0.7194 | 691.0 | 615.9 | |
| 0.00 | 0.91 | 0.00 | 0.66 | 7.49 | 155.28 | -46.88 | 83.29 | 0.7310 | 704.0 | 650.3 | |
| 0.00 | 0.82 | 0.00 | 0.63 | 8.79 | 152.23 | -49.93 | 81.71 | 0.7666 | 553.0 | 524.0 | |
| 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. | |