line broadening वाक्य
उदाहरण वाक्य
मोबाइल
- However, the different line broadening mechanisms are not always independent.
- This spectral line broadening has many different causes.
- This leads to line broadening and insufficiency.
- What a high Q factor rids you of is line broadening, but it does not enforce a pure sine.
- Differential rotation affects stellar optical absorption-line spectra through line broadening caused by lines being differently Doppler-shifted across the stellar surface.
- It, along with ? Librae, were the first stars on which rotational line broadening was observed, by Frank Schlesinger in 1909.
- However, care must be taken if silver behenate is to be used as a peak-profile calibration standard because of line broadening.
- As of August 27, 2007 discoveries concerning asymmetric iron line broadening and their implications for relativity have been a topic of much excitement.
- Chiral lanthanide shift reagents cause a clear separation of chemical shift, but they must be used in low concentrations to avoid line broadening.
- As of August 27, 2007 . discoveries concerning asymmetric iron line broadening and their implications for relativity have been a topic of much excitement.
- These probabilities are also useful for calculating the " quantum broadening " of spectral lines ( see line broadening ) and particle decay in particle physics and nuclear physics.
- If the line broadening mechanism is known and the shape of then spectral density is clearly visible in the spectrum, it is possible to get the desired data.
- "' Johan Peter Holtsmark "'( February 13, 1894 December 10, 1975 ) was a Norwegian physicist, who studied spectral line broadening and electron scattering.
- It is believed that the shell stars belong to somewhere in the range of main sequence up to giant star size, although the exact luminosity class is uncertain due to rotational line broadening.
- Interactions between RNA and metal ions can be probed by a number of methods, including observing changes in chemical shift upon ion binding, observing line broadening for paramagnetic ion species, and observing intermolecular NOE contacts for organometallic mimics of the metal ions.
- With respect to the asymmetric iron line broadening, Edward Cackett of the University of Michigan commented, " We're seeing the gas whipping around just outside the neutron star's surface, " . " And since the inner part of the disk obviously can't orbit any closer than the neutron star's surface, these measurements give us a maximum size of the neutron star's diameter.
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