Experimental Stark Profile Determination of Some Plasma Broadened He I-and He II-Lines

1979 ◽  
Vol 34 (3) ◽  
pp. 300-309 ◽  
Author(s):  
H. Soltwisch ◽  
H. J. Kusch

Abstract Line profiles of the plasma broadened lines He I: 3188, 3889, and 5016 Å and He II: 3203, 4686 Å have been determined from measurements using a wall-stabilized quasistationary pulsed discharge as a plasma source of sufficient homogeneity. The profiles were recorded applying the rapid-scan technique to enable single-shot registration of the spectral data. Electron density values were obtained from plasma-refractivity measurements at two different wavelengths using rare gas ion-lasers as background light-sources. The electron density range in this experiment was (0.7 -1.2) · 1017 cm−3. Temperature values of pure helium plasmas resulted from absolute radiation measurements (line intensities of He II 3203 Å and 4686 Å), yielding ~ 4 · 104 K. In helium-hydrogen mixtures further used for plasma generation in the lower temperature region, temperature values could be estimated from the optically thick Balmer line Hα, yielding ~ 2 · 104 K. Experimental line shapes and half-widths are compared with the theoretical predictions of several authors and with the results of previous measurements. In case of neutral helium lines experimental and theoretical values agree within experimental accuracy (10%), whereas for the He II-lines the measured line shapes deviate considerably from the theoretical predictions.

2021 ◽  
Vol 11 (12) ◽  
pp. 5358
Author(s):  
Ju-Hong Cha ◽  
Sang-Woo Kim ◽  
Ho-Jun Lee

For a conventional linear microwave plasma source (LMPS) with a quasi-coaxial line transverse electromagnetic (TEM) waveguide, a linearly extended plasma is sustained by the surface wave outside the tube. Due to the characteristics of the quasi-coaxial line MPS, it is easy to generate a uniform plasma with radially omnidirectional surfaces, but it is difficult to maximize the electron density in a curved selected region. For the purpose of concentrating the plasma density in the deposition area, a novel LMPS which is suitable for curved structure deposition has been developed and compared with the conventional LMPS. As the shape of a circular waveguide, it is filled with relatively high-permittivity dielectric instead of a quasi-coaxial line waveguide. Microwave power at 2.45 GHz is transferred to the plasma through the continuous cylindrical-slotted line antenna, and the radiated electric field in the radial direction is made almost parallel to the tangential plane of the window surface. This research includes the advanced 3D numerical analysis and compares the results with the experiment. It shows that the electron density in the deposition area is higher than that of the conventional quasi-coaxial line plasma MPS.


2021 ◽  
Vol 75 (2) ◽  
Author(s):  
A. Raji ◽  
J. Rosato ◽  
R. Stamm ◽  
Y. Marandet
Keyword(s):  

2021 ◽  
Author(s):  
Robert Cryderman ◽  
Finn Bamrud

Abstract A micro-alloyed 1045 steel was commercially rolled into 54 mm diameter bars by conventional hot rolling at 1000 °C and by lower temperature thermomechanical rolling at 800 °C. The lower rolling temperature refined the ferrite-pearlite microstructure and influenced the microstructural response to rapid heating at 200 °C·s-1, a rate that is commonly encountered during single shot induction heating for case hardening. Specimens of both materials were rapidly heated to increasing temperatures in a dilatometer to determine the Ac1 and Ac3 transformation temperatures. Microscopy was used to characterize the dissolution of ferrite and cementite. Continuous cooling transformation (CCT) diagrams were developed for rapid austenitizing temperatures 25 °C above the Ac3 determined by dilatometry. Dilatometry and microstructure evaluation along with hardness tests showed that thermomechanical rolling reduced the austenite grain size and lowered the heating temperature needed to dissolve the ferrite. With complete austenitization at 25 °C above the Ac3 there was little effect on the CCT behavior.


1980 ◽  
Vol 5 ◽  
pp. 811-815
Author(s):  
Lawrence H. Aller

AbstractThe chemical compositions of external galaxies are usually found from their HII regions or composite absorption line spectra of their nuclei. In the Magellanic Clouds, however, individual stars are observable, but objects heretofore studied necessarily have been luminous la supergiants which border on the brink of instability. The image photon counting system on the Anglo-Australian Telescope makes it possible to observe fainter, more stable Ib supergiants. Energy distributions and Balmer line profiles for these stars can be fitted with theoretical predictions by Kurucz. A joint effort by J.E. Ross and B.J. O’Mara of the University of Queensland, Bruce Peterson of the Anglo-Australian Observatory, and a group at the University of California, Los Angeles to analyze three lb supergiants suggests that metals of the iron group are depleted by a factor of 2-3.5 with respect to the normal chemical composition of our own galaxy.


2009 ◽  
Vol 37 (4) ◽  
pp. 475-480 ◽  
Author(s):  
P. Di Lazzaro ◽  
S. Bollanti ◽  
F. Flora ◽  
L. Mezi ◽  
D. Murra ◽  
...  

1973 ◽  
Vol 28 (11) ◽  
pp. 1794-1800 ◽  
Author(s):  
Horst Ehrich ◽  
Hans Jürgen Kusch

The profiles of the Stark broadened Balmer lines Hα and Hβ have been measured in a wide range of temperature and electron density. By the use of different light sources (3 wallstabilized arcs of different design, a pulsed discharge tube and a plexiglass-capillary discharge) the range was ex- tended to 1.0·104≦T≦3.2·104 °K for the plasma temperature and to 1·1016≦ne≦55·1016 cm−3 for the electron density in the Hβ-scale. The experimental profiles of the Hα-line agree with generalized impact approximations if the condition: ne2/3/T>2·107 cm−2 grad−1 is fulfilled. Disagreements between the Hα and Hβ electron density scale can be removed applying an empirical correction-factor to the electron density obtained from the half-width of Hα.


1994 ◽  
Vol 159 ◽  
pp. 462-462
Author(s):  
Rodger I. Thompson

This paper presents the complete spectrum of NGC 4151 from 0.87 to 2.5 μm as well as detail of the Paschen α profile in 3C273 at a resolution of about 5000. Analysis of the several observed Fe II lines yields a most probable electron density of 104 and a most likely temperature of 104. The Fe II to H ratio is 2+/− 1 × 10−6 which is 5–7% of the available iron if the Fe/H ratio is solar.


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