EXCITATION TEMPERATURE OF A RAPIDLY VARYING PLASMA

1979 ◽  
Vol 40 (C7) ◽  
pp. C7-49-C7-50
Author(s):  
M. Numano ◽  
H. Onishi
2021 ◽  
Vol 1825 (1) ◽  
pp. 012050
Author(s):  
J M Windajanti ◽  
D J D H Santjojo ◽  
M A Pamungkas ◽  
Abdurrouf

Author(s):  
Haruki Ejiri ◽  
Ryo Kikuchi ◽  
Akiko Kumada ◽  
Kunihiko Hidaka ◽  
Akihiro Suwa ◽  
...  

2021 ◽  
Vol 257 (2) ◽  
pp. 47
Author(s):  
Ningyu Tang ◽  
Di Li ◽  
Gan Luo ◽  
Carl Heiles ◽  
Sheng-Li Qin ◽  
...  

Abstract We present high-sensitivity CH 9 cm ON/OFF observations toward 18 extragalactic continuum sources that have been detected with OH 18 cm absorption in the Millennium survey with the Arecibo telescope. CH emission was detected toward 6 of the 18 sources. The excitation temperature of CH has been derived directly through analyzing all detected ON and OFF velocity components. The excitation temperature of CH 3335 MHz transition ranges from −54.5 to −0.4 K and roughly follows a log-normal distribution peaking within [−5, 0] K, which implies overestimation by 20% to more than 10 times during calculating CH column density by assuming the conventional value of −60 or −10 K. Furthermore, the column density of CH would be underestimated by a factor of 1.32 ± 0.03 when adopting local thermal equilibrium assumption instead of using the CH three hyperfine transitions. We found a correlation between the column density of CH and OH following log N(CH) = (1.80 ± 0.49) and log N(OH −11.59 ± 6.87. The linear correlation between the column density of CH and H2 is consistent with that derived from visible wavelengths studies, confirming that CH is one of the best tracers of H2 components in diffuse molecular gas.


2016 ◽  
Vol 37 (10) ◽  
pp. 1299-1304
Author(s):  
刘耀泽 LIU Yao-ze ◽  
袁承勋 YUAN Cheng-xun ◽  
高瑞林 GAO Rui-lin ◽  
贾洁姝 JIA Jie-shu ◽  
周忠祥 ZHOU Zhong-xiang

2008 ◽  
Vol 493 (2) ◽  
pp. 601-612 ◽  
Author(s):  
A. Hosford ◽  
S. G. Ryan ◽  
A. E. García Pérez ◽  
J. E. Norris ◽  
K. A. Olive

2017 ◽  
Vol 35 (1) ◽  
pp. 159-169 ◽  
Author(s):  
H. Iftikhar ◽  
S. Bashir ◽  
A. Dawood ◽  
M. Akram ◽  
A. Hayat ◽  
...  

AbstractThe effect of the transverse magnetic field on laser-induced breakdown spectroscopy and surface modifications of germanium (Ge) has been investigated at various fluences. Ge targets were exposed to Nd: YAG laser pulses (1064 nm, 10 ns, 1 Hz) at different fluences ranging from 3 to 25.6 J/cm2 to generate Ge plasma under argon environment at a pressure of 50 Torr. The magnetic field of strength 0.45 Tesla perpendicular to the direction of plasma expansion was employed by using two permanent magnets. The emission spectra of laser-induced Ge plasma was detected by the laser-induced breakdown spectroscopy system. The electron temperature and number density of Ge plasma are evaluated by using the Boltzmann plot and stark broadening methods, respectively. The variations in emission intensity, electron temperature (Te), and number density (ne) of Germanium plasma are explored at various fluences, with and without employment of the magnetic field. It is observed that the magnetic field is responsible for significant enhancement of both excitation temperature and number density at all fluences. It is revealed that an excitation temperature increases from Te,max,without B = 16,190 to Te,max,with B = 20,123 K. Similarly, the two times enhancement in the electron density is observed from ne,max,without B = 2 × 1018 to ne,max,with B = 4 × 1018 cm−3. The overall enhancement in Ge plasma parameters in the presence of the magnetic field is attributed to the Joule heating effect and adiabatic compression. With increasing fluence both plasma parameters increase and achieve their maxima at a fluence of 12.8 J/cm2 and then decrease. In order to correlate the plasma parameters with surface modification, scanning electron microscope analysis of irradiated Ge was performed. Droplets and cones are formed for both cases. However, the growth of ridges and distinctness of features is more pronounced in case of the absence of the magnetic field; whereas surface structures become more diffusive in the presence of the magnetic field.


2014 ◽  
Vol 781 (2) ◽  
pp. L41 ◽  
Author(s):  
Claire E. Murray ◽  
Robert R. Lindner ◽  
Snežana Stanimirović ◽  
W. M. Goss ◽  
Carl Heiles ◽  
...  

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