X-Ray Imaging Spectrometer for Recording Calibrated Time-Resolved K-Shell Spectra from Magnetically Confined Fusion Plasmas

2008 ◽  
Author(s):  
John F. Seely ◽  
Uri Feldman ◽  
Szymon Suckewer ◽  
Lawrence T. Hudson ◽  
Giuseppe Gorini ◽  
...  
2011 ◽  
Author(s):  
N. A. Pablant ◽  
M. Bitter ◽  
L. F. Delgado-Aparicio ◽  
K. W. Hill ◽  
M. Sanchez del Rio

2019 ◽  
Vol 489 (3) ◽  
pp. 4300-4310 ◽  
Author(s):  
A Sezer ◽  
T Ergin ◽  
R Yamazaki ◽  
H Sano ◽  
Y Fukui

ABSTRACT We present the results from the Suzaku X-ray Imaging Spectrometer observation of the mixed-morphology supernova remnant (SNR) HB9 (G160.9+2.6). We discovered recombining plasma (RP) in the western Suzaku observation region and the spectra here are well described by a model having collisional ionization equilibrium (CIE) and RP components. On the other hand, the X-ray spectra from the eastern Suzaku observation region are best reproduced by the CIE and non-equilibrium ionization model. We discuss possible scenarios to explain the origin of the RP emission based on the observational properties and concluded that the rarefaction scenario is a possible explanation for the existence of RP. In addition, the gamma-ray emission morphology and spectrum within the energy range of 0.2–300 GeV are investigated using 10 yr of data from the Fermi Large Area Telescope (LAT). The gamma-ray morphology of HB9 is best described by the spatial template of radio continuum emission. The spectrum is well fit to a log-parabola function and its detection significance was found to be 25σ. Moreover, a new gamma-ray point source located just outside the south-east region of the SNR’s shell was detected with a significance of 6σ. We also investigated the archival H i and CO data and detected an expanding shell structure in the velocity range of $-10.5$ and $+1.8$ km s−1 that is coinciding with a region of gamma-ray enhancement at the southern rim of the HB9 shell.


2000 ◽  
Vol 61 (3) ◽  
pp. 3042-3052 ◽  
Author(s):  
M. May ◽  
K. Fournier ◽  
D. Pacella ◽  
H. Kroegler ◽  
J. Rice ◽  
...  

1998 ◽  
Author(s):  
James L. Matteson ◽  
Duane E. Gruber ◽  
William A. Heindl ◽  
Michael R. Pelling ◽  
Laurence E. Peterson ◽  
...  

2002 ◽  
Vol 33 (4) ◽  
pp. 613-623 ◽  
Author(s):  
Ragnvald H. Mathiesen ◽  
Lars Arnberg ◽  
Kjell Ramsøskar ◽  
Timm Weitkamp ◽  
Christoph Rau ◽  
...  

2016 ◽  
Vol 18 (4) ◽  
pp. 043017 ◽  
Author(s):  
L Flückiger ◽  
D Rupp ◽  
M Adolph ◽  
T Gorkhover ◽  
M Krikunova ◽  
...  
Keyword(s):  
X Ray ◽  

2009 ◽  
Vol 58 (9) ◽  
pp. 6397
Author(s):  
Hu Xin ◽  
Zhang Ji-Yan ◽  
Yang Guo-Hong ◽  
Liu Shen-Ye ◽  
Ding Yong-Kun

2019 ◽  
Vol 49 (1) ◽  
pp. 389-415 ◽  
Author(s):  
Haidan Wen ◽  
Mathew J. Cherukara ◽  
Martin V. Holt

X-ray microscopy has been an indispensable tool to image nanoscale properties for materials research. One of its recent advances is extending microscopic studies to the time domain to visualize the dynamics of nanoscale phenomena. Large-scale X-ray facilities have been the powerhouse of time-resolved X-ray microscopy. Their upgrades, including a significant reduction of the X-ray emittance at storage rings (SRs) and fully coherent ultrashort X-ray pulses at free-electron lasers (FELs), will lead to new developments in instrumentation and will open new scientific opportunities for X-ray imaging of nanoscale dynamics with the simultaneous attainment of unprecedentedly high spatial and temporal resolutions. This review presents recent progress in and the outlook for time-resolved X-ray microscopy in the context of ultrafast nanoscale imaging and its applications to condensed matter physics and materials science.


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