SDO HMI 2014-08-10 09:00:39 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 |
| 0.00 | 50.72 | 0.00 | 28.59 | 10.10 | 174.57 | 27.98 | 279.97 | 0.4703 | 108.6 | 191.5 | |
|
previous
or next observation for the same group /
back to the solar disc SDO HMI 2014-08-10 09:00:39 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 | 0.63 | 0.00 | 0.39 | 6.70 | 183.15 | 36.56 | 272.64 | 0.5945 | -597.0 | -524.6 | |
| 0.00 | 1.08 | 0.00 | 0.67 | 8.08 | 183.14 | 36.55 | 274.96 | 0.5940 | -456.0 | -354.9 | |
| 0.00 | 2.17 | 0.00 | 1.29 | 11.98 | 180.41 | 33.82 | 282.03 | 0.5588 | -868.0 | -736.6 | |
| 0.00 | 0.99 | 0.00 | 0.59 | 5.89 | 179.73 | 33.14 | 270.98 | 0.5460 | -670.0 | -616.2 | |
| 0.00 | 1.81 | 0.00 | 1.08 | 12.58 | 180.24 | 33.64 | 283.13 | 0.5574 | -749.0 | -554.3 | |
| 0.00 | 0.81 | 0.00 | 0.48 | 12.73 | 180.22 | 33.63 | 283.40 | 0.5575 | -722.0 | -607.4 | |
| 0.00 | 1.54 | 0.00 | 0.90 | 11.52 | 179.01 | 32.42 | 281.46 | 0.5381 | -744.0 | -599.5 | |
| 0.00 | 0.90 | 0.00 | 0.53 | 11.15 | 178.52 | 31.93 | 280.86 | 0.5305 | -849.0 | -697.2 | |
| 0.00 | 1.26 | 0.00 | 0.74 | 11.40 | 178.44 | 31.85 | 281.35 | 0.5297 | -827.0 | -715.0 | |
| 0.00 | 1.17 | 0.00 | 0.68 | 8.82 | 178.08 | 31.49 | 276.49 | 0.5216 | -761.0 | -629.2 | |
| 0.00 | 0.45 | 0.00 | 0.26 | 9.14 | 177.86 | 31.27 | 277.12 | 0.5185 | -664.0 | -496.8 | |
| 0.00 | 1.17 | 0.00 | 0.68 | 13.33 | 177.32 | 30.73 | 285.32 | 0.5175 | -544.0 | -427.0 | |
| 0.00 | 1.54 | 0.00 | 0.89 | 13.25 | 177.13 | 30.53 | 285.23 | 0.5146 | -712.0 | -647.6 | |
| 0.00 | 1.63 | 0.00 | 0.94 | 13.49 | 176.76 | 30.17 | 285.81 | 0.5099 | -658.0 | -477.1 | |
| 0.00 | 1.08 | 0.00 | 0.61 | 9.63 | 175.63 | 29.03 | 278.37 | 0.4856 | -831.0 | -592.6 | |
| 0.00 | 1.45 | 0.00 | 0.81 | 10.01 | 174.71 | 28.12 | 279.33 | 0.4723 | 759.0 | 522.6 | |
| 0.00 | 2.17 | 0.00 | 1.21 | 10.13 | 174.30 | 27.71 | 279.65 | 0.4663 | 842.0 | 640.5 | |
| 0.00 | 0.99 | 0.00 | 0.55 | 10.49 | 173.82 | 27.22 | 280.54 | 0.4594 | 794.0 | 642.5 | |
| 0.00 | 1.17 | 0.00 | 0.65 | 9.15 | 173.66 | 27.07 | 277.65 | 0.4552 | 617.0 | 474.2 | |
| 0.00 | 1.08 | 0.00 | 0.60 | 9.69 | 173.36 | 26.77 | 278.89 | 0.4512 | 593.0 | 557.8 | |
| 0.00 | 1.26 | 0.00 | 0.70 | 9.51 | 173.31 | 26.72 | 278.49 | 0.4502 | 807.0 | 616.1 | |
| 0.00 | 6.32 | 0.00 | 3.50 | 9.18 | 173.18 | 26.59 | 277.78 | 0.4478 | 894.0 | 735.5 | |
| 0.00 | 3.97 | 0.00 | 2.20 | 8.58 | 173.03 | 26.44 | 276.45 | 0.4449 | 768.0 | 684.0 | |
| 0.00 | 1.17 | 0.00 | 0.65 | 8.85 | 173.05 | 26.46 | 277.06 | 0.4454 | 864.0 | 661.8 | |
| 0.00 | 2.35 | 0.00 | 1.30 | 9.01 | 172.79 | 26.20 | 277.48 | 0.4415 | 788.0 | 648.2 | |
| 0.00 | 1.54 | 0.00 | 0.85 | 9.93 | 172.76 | 26.17 | 279.56 | 0.4424 | 756.0 | 607.7 | |
| 0.00 | 0.81 | 0.00 | 0.45 | 9.32 | 172.67 | 26.08 | 278.20 | 0.4402 | 901.0 | 732.3 | |
| 0.00 | 0.99 | 0.00 | 0.55 | 8.97 | 172.41 | 25.82 | 277.44 | 0.4356 | 875.0 | 695.8 | |
| 0.00 | 1.35 | 0.00 | 0.74 | 9.56 | 172.18 | 25.59 | 278.84 | 0.4328 | 842.0 | 677.6 | |
| 0.00 | 1.17 | 0.00 | 0.64 | 9.36 | 172.03 | 25.44 | 278.39 | 0.4302 | 784.0 | 636.8 | |
| 0.00 | 1.08 | 0.00 | 0.58 | 8.83 | 168.96 | 22.36 | 277.71 | 0.3810 | 745.0 | 683.8 | |
| 0.00 | 1.54 | 0.00 | 0.82 | 7.38 | 167.81 | 21.22 | 273.97 | 0.3614 | 794.0 | 607.1 | |
| 0.00 | 2.08 | 0.00 | 1.06 | 14.04 | 158.26 | 11.67 | 304.62 | 0.2395 | 814.0 | 730.3 | |
| 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. | |