scholarly journals X-RAY RADIATION MECHANISMS AND BEAMING EFFECT OF HOT SPOTS AND KNOTS IN ACTIVE GALACTIC NUCLEAR JETS

2010 ◽  
Vol 710 (2) ◽  
pp. 1017-1031 ◽  
Author(s):  
Jin Zhang ◽  
J. M. Bai ◽  
Liang Chen ◽  
Enwei Liang
Keyword(s):  
2011 ◽  
Vol 32 (1-2) ◽  
pp. 193-196
Author(s):  
Jin Zhang ◽  
Jin-Ming Bai ◽  
Liang Chen ◽  
Enwei Liang
Keyword(s):  

Author(s):  
Xia ◽  
Hu ◽  
Shao ◽  
Xu ◽  
Zhou ◽  
...  

To verify the feasibility of portable X-ray fluorescence (PXRF) for rapidly analyzing, assessing and improving soil heavy metals mapping, 351 samples were collected from Fuyang District, Hangzhou City, in eastern China. Ordinary kriging (OK) and co-ordinary kriging (COK) combined with PXRF measurements were used to explore spatial patterns of heavy metals content in the soil. The Getis-Ord index was calculated to discern hot spots of heavy metals. Finally, multi-variable indicator kriging was conducted to obtain a map of multi-heavy metals pollution. The results indicated Cd is the primary pollution element in Fuyang, followed by As and Pb. Application of PXRF measurements as covariates in COK improved model accuracy, especially for Pb and Cd. Heavy metals pollution hot spots were mainly detected in northern Fuyang and plains along the Fuchun River in southern Fuyang because of mining, industrial and traffic activities, and irrigation with polluted water. Area with high risk of multi-heavy metals pollution mainly distributed in plain along the Fuchun River and the eastern Fuyang. These findings certified the feasibility of using PXRF as an efficient and reliable method for soil heavy metals pollution assessment and mapping, which could contribute to reduce the cost of surveys and pollution remediation.


2021 ◽  
Vol 1020 ◽  
pp. 8-12
Author(s):  
Wu Hu ◽  
Ke Zhu ◽  
Meng Wang ◽  
Wei Dong Huang ◽  
Jian Min Zeng

Linear segregation of high strength aluminum alloy ZL205A castings were studied by X-ray Nondestructive testing, scanning electron microscope and energy dispersive spectrometer. It is found that the linear segregation occurs at the large wall thickness of the casting and/or at the place where the wall thickness is in transition. Segregation element is mainly Cu, which exists as compound θ (Al2Cu) phase. The formation of linear segregation is related to the flow of Cu-rich melt in the late solidification period, while the occurrence of thermal cracks promotes the formation of linear segregation. The formation of linear segregation of the casting can be effectively prevented by eliminating hot spots of the casting, refining crystal grains and increasing solidification speed of the casting.


1989 ◽  
Author(s):  
A. Krejc̆í ◽  
E. Kruouský ◽  
O. Renner
Keyword(s):  

2004 ◽  
Vol 612 (2) ◽  
pp. 729-748 ◽  
Author(s):  
M. J. Hardcastle ◽  
D. E. Harris ◽  
D. M. Worrall ◽  
M. Birkinshaw
Keyword(s):  

2000 ◽  
Vol 530 (2) ◽  
pp. L81-L84 ◽  
Author(s):  
D. E. Harris ◽  
P. E. J. Nulsen ◽  
T. J. Ponman ◽  
M. Bautz ◽  
R. A. Cameron ◽  
...  
Keyword(s):  

1960 ◽  
Vol 10 ◽  
pp. 706-708 ◽  
Author(s):  
Herbert Friedman

The X-ray spectrum of a quiet Sun can be approximated by a 500,000° K Planckian distribution. In the absence of coronal excitation, as evidenced by the intensity of the Fe xiv green line, the X-ray spectrum has a short wave-length limit near 20 A. Coronal activity is accompanied by weak emissions down to wave-lengths as short as 6 A, which appear to be associated with coronal hot spots at temperatures of 2 x 106° K or higher.


1987 ◽  
Vol 125 ◽  
pp. 249-249
Author(s):  
Tong Yi ◽  
Fang Geng ◽  
Mao Xinjie

Usually we think a X-ray source may be a compact(neutron) binary star on which the X-ray radiation might be generated by gravitational acceleration for the particles coming from the primary and going along magnetic field lines of the compact star to the poles. But, in the past, people don't consider well the problem of particle acceleration. It seems to be simplified for the situation only to consider the gravitation effect, because some electric-magnetic effect in a strong magnetic field could not be neglected. However, it is unreasonable to neglect the plasma turbulent waves in an electric-magnetic field, because strong enough turbulent waves such as Alfven waves, whistlers generated nearby the surface of neutron stars probably contribute energy to accelerate particles, which may be more important than gravitation sometimes. For a binary system with a neutron star if ion number density N > 1017 /cm3 in its surface atmosphere, the turbulent wavess will be stimulated that will accelerate the particles reaching a speed over 108cm/s. they strike the atmosphere of the compact star in the system, so that a shock wave is formed which turns part of kinetic energy to heat to form hot spots of about 108K to emit X-ray.


1990 ◽  
Vol 40 (11) ◽  
pp. 1244-1249 ◽  
Author(s):  
A. Krejčí ◽  
E. Krouský ◽  
O. Renner
Keyword(s):  

Sign in / Sign up

Export Citation Format

Share Document