SDO HMI 2014-09-10 14:00:35 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 |
| 33.04 | 111.44 | 18.99 | 63.70 | -19.73 | 107.32 | 13.08 | 205.13 | 0.5010 | 479.2 | 337.2 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-09-10 14:00:35 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 | 1.16 | 0.00 | 0.68 | -20.48 | 110.84 | 16.59 | 210.18 | 0.5343 | 733.0 | 595.5 | |
| 0.00 | 3.65 | 0.00 | 2.14 | -20.82 | 110.84 | 16.60 | 209.84 | 0.5386 | 591.0 | 537.0 | |
| 0.00 | 0.98 | 0.00 | 0.57 | -20.60 | 110.48 | 16.24 | 209.52 | 0.5332 | 591.0 | 512.8 | |
| 0.00 | 2.49 | 0.00 | 1.45 | -20.34 | 110.08 | 15.84 | 209.17 | 0.5272 | 648.0 | 524.8 | |
| 0.00 | 1.07 | 0.00 | 0.62 | -20.09 | 109.56 | 15.31 | 208.61 | 0.5201 | 857.0 | 687.5 | |
| 10.42 | 13.63 | 6.07 | 7.94 | -20.77 | 109.49 | 15.25 | 207.85 | 0.5284 | 831.5 | 596.2 | |
| 0.00 | 1.16 | 0.00 | 0.68 | -21.43 | 108.96 | 14.71 | 206.42 | 0.5334 | -700.0 | -566.9 | |
| 0.98 | 2.41 | 0.57 | 1.40 | -21.08 | 108.72 | 14.48 | 206.37 | 0.5273 | 732.5 | 633.9 | |
| 17.28 | 30.29 | 9.85 | 17.25 | -18.90 | 108.45 | 14.21 | 208.00 | 0.4967 | 962.9 | 585.0 | |
| 0.00 | 0.98 | 0.00 | 0.57 | -21.35 | 108.61 | 14.37 | 205.96 | 0.5301 | 491.0 | 467.4 | |
| 0.00 | 1.78 | 0.00 | 1.04 | -21.10 | 108.42 | 14.18 | 205.88 | 0.5257 | 789.0 | 635.1 | |
| 0.00 | 0.98 | 0.00 | 0.57 | -21.58 | 108.30 | 14.06 | 205.27 | 0.5312 | 674.0 | 589.7 | |
| 2.85 | 25.83 | 1.63 | 14.77 | -20.01 | 107.19 | 12.95 | 204.85 | 0.5031 | 981.2 | 746.0 | |
| 1.51 | -13.00 | 0.87 | -13.00 | -20.03 | 106.83 | 12.59 | 204.22 | 0.5012 | 1116.2 | 999999 | |
| 0.00 | 1.07 | 0.00 | 0.61 | -20.34 | 106.86 | 12.62 | 204.00 | 0.5055 | 432.0 | 456.4 | |
| 0.00 | 0.80 | 0.00 | 0.46 | -20.39 | 106.57 | 12.32 | 203.46 | 0.5046 | 699.0 | 597.7 | |
| 0.00 | 1.34 | 0.00 | 0.77 | -20.46 | 106.31 | 12.06 | 202.97 | 0.5039 | 807.0 | 613.1 | |
| 0.00 | 1.78 | 0.00 | 1.02 | -20.52 | 106.15 | 11.90 | 202.64 | 0.5038 | 593.0 | 494.8 | |
| 0.00 | 0.71 | 0.00 | 0.40 | -19.56 | 104.48 | 10.23 | 200.45 | 0.4810 | 780.0 | 667.9 | |
| 0.00 | 0.80 | 0.00 | 0.45 | -19.79 | 104.43 | 10.18 | 200.18 | 0.4841 | 606.0 | 527.9 | |
| 0.00 | 0.89 | 0.00 | 0.50 | -18.60 | 104.03 | 9.79 | 200.36 | 0.4649 | 681.0 | 557.9 | |
| 0.00 | 1.16 | 0.00 | 0.65 | -18.65 | 103.16 | 8.92 | 198.65 | 0.4611 | -825.0 | -740.5 | |
| 0.00 | 3.30 | 0.00 | 1.84 | -19.02 | 103.05 | 8.81 | 198.17 | 0.4660 | -583.0 | -512.2 | |
| 0.00 | 2.14 | 0.00 | 1.19 | -18.68 | 102.94 | 8.69 | 198.19 | 0.4604 | -715.0 | -569.1 | |
| 0.00 | 1.78 | 0.00 | 0.99 | -18.70 | 102.58 | 8.34 | 197.48 | 0.4591 | -742.0 | -643.0 | |
| 0.00 | 1.07 | 0.00 | 0.59 | -18.16 | 102.46 | 8.22 | 197.61 | 0.4506 | -711.0 | -591.4 | |
| 0.00 | 2.49 | 0.00 | 1.38 | -18.16 | 102.04 | 7.80 | 196.78 | 0.4486 | -727.0 | -608.4 | |
| 0.00 | 3.21 | 0.00 | 1.78 | -18.48 | 101.70 | 7.46 | 195.88 | 0.4520 | -949.0 | -797.2 | |
| 0.00 | 2.49 | 0.00 | 1.39 | -19.02 | 101.44 | 7.19 | 195.01 | 0.4589 | -938.0 | -668.1 | |
| 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. | |