Effect of magnetic field strength on deposition rate and energy flux in a dc magnetron sputtering system

2009 ◽  
Vol 27 (6) ◽  
pp. 1275-1280 ◽  
Author(s):  
Samuel D. Ekpe ◽  
Francisco J. Jimenez ◽  
David J. Field ◽  
Martin J. Davis ◽  
Steven K. Dew
2009 ◽  
Vol 45 (10) ◽  
pp. 4391-4394 ◽  
Author(s):  
Cheng-Tsung Liu ◽  
Ming-Chih Lai ◽  
Chang-Chou Hwang ◽  
Chun-Hung Tu ◽  
Li-Yang Liu ◽  
...  

Nature ◽  
2009 ◽  
Vol 457 (7226) ◽  
pp. 167-169 ◽  
Author(s):  
Ulrich R. Christensen ◽  
Volkmar Holzwarth ◽  
Ansgar Reiners

2019 ◽  
Vol 33 (01n03) ◽  
pp. 1940017 ◽  
Author(s):  
D. L. Ma ◽  
Y. T. Li ◽  
Q. Y. Deng ◽  
B. Huang ◽  
Y. X. Leng ◽  
...  

Titanium (Ti) thin films with (002) or (100) texture are favored for many applications. In this paper, Ti thin films were prepared by high-power pulsed magnetron sputtering, and the texture of Ti thin films was successfully tailored by adjusting the pulse width, substrate bias and magnetic field strength. It is found that the peak power and average power of the Ti target are increased by increasing sputtering pulse width and decreasing magnetic field strength, which raise the Ti plasma flux and ion/atom ratio of Ti ions in front of the substrate simultaneously. Ti thin films with a highly (002) out-of-plane texture can be obtained with higher pulse width and lower magnetic field strength. The Ti thin films with highly (100) out-of-plane texture can be achieved with shorter pulse width, lower magnetic field strength and substrate bias.


1976 ◽  
Vol 32 ◽  
pp. 613-622
Author(s):  
I.A. Aslanov ◽  
Yu.S. Rustamov

SummaryMeasurements of the radial velocities and magnetic field strength of β CrB were carried out. It is shown that there is a variability with the rotation period different for various elements. The curve of the magnetic field variation measured from lines of 5 different elements: FeI, CrI, CrII, TiII, ScII and CaI has a complex shape specific for each element. This may be due to the presence of magnetic spots on the stellar surface. A comparison with the radial velocity curves suggests the presence of a least 4 spots of Ti and Cr coinciding with magnetic spots. A change of the magnetic field with optical depth is shown. The curve of the Heffvariation with the rotation period is given. A possibility of secular variations of the magnetic field is shown.


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