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The ionization of xenon atoms subjected to 42fs, 800nm pulses of radiation from a Ti:Sapphire laser was investigated. In our experiments a maximum laser intensity of $\sim2\times 10^{15} \textrm{W}/\textrm{cm}^2$ was used. Xenon ions were…

原子物理 · 物理学 2016-05-09 J. Strohaber , A. A. Kolomenskii , H. A. Schuessler

We have analyzed high-resolution X-ray spectra of a sample of 22 active stars observed with the High Energy Transmission Grating Spectrometer on {\em Chandra} in order to investigate their coronal plasma density. Densities where…

天体物理学 · 物理学 2009-11-10 Paola Testa , Jeremy J. Drake , Giovanni Peres

We investigate photoinization, energy deposition, plasma formation and the ultrafast optical breakdown in crystalline silicon irradiated by intense near-infrared laser pulses with pulse duration $\tau \le $ 100 fs. The occurrence of…

材料科学 · 物理学 2021-11-24 Tzveta Apostolova , Boyan Obreshkov

We present measurements of hard x-rays in the 50-300 keV range from copper plasmas produced by 100 fs, 806 nm laser pulses at a peak intensity ~ 1016 W cm-2. Surface roughness, even at the tens of nanometer level, is shown to influence the…

等离子体物理 · 物理学 2009-11-07 P. P. Rajeev , G. Ravindra Kumar

In this paper, we present an experiment that explores the plasma dynamics of a 7 micron diameter carbon wire after being irradiated with a near-relativistic-intensity short pulse laser. Using an X-ray Free Electron Laser pulse to measure…

The RESIK instrument on the CORONAS-F spacecraft obtained solar flare and active region X-ray spectra in four channels covering the wavelength range 3.8 -- 6.1 \AA in its operational period between 2001 and 2003. Several highly ionized…

太阳与恒星天体物理 · 物理学 2015-06-12 B. Sylwester , K. J. H. Phillips , J. Sylwester , A. Kepa

In simulations of a 10PW laser striking a solid we demonstrate the possibility of producing a pure electron-positron plasma by the same processes as those thought to operate in high-energy astrophysical environments. A maximum positron…

等离子体物理 · 物理学 2015-06-04 C. P. Ridgers , C. S. Brady , R. Duclous , J. G. Kirk , K. Bennett , T. D. Arber , A. P. L. Robinson , A. R. Bell

The intensity of the \oiv~2s$^{2}$ 2p $^{2}$P-2s2p$^{2}$ $^{4}$P and \siv~3 s$^{2}$ 3p $^{2}$P- 3s 3p$^{2}$ $^{4}$ P intercombination lines around 1400~\AA~observed with the \textit{Interface Region Imaging Spectrograph} (IRIS) provide a…

太阳与恒星天体物理 · 物理学 2016-10-19 V. Polito , G. Del Zanna , J. Dudík , H. E. Mason , A. Giunta , K. K. Reeves

We present a detailed analysis of the complex soft X-ray spectrum of NGC 4151 measured by the RGS instruments aboard XMM-Newton. The XMM-Newton RGS spectra demonstrate that the soft X-ray emission is extremely rich in X-ray emission lines…

天体物理学 · 物理学 2009-11-10 N. J. Schurch , R. S. Warwick , R. E. Griffiths , S. M. Kahn

We present a simple, yet powerful column density diagnostic for plasmas enabled by X-ray microcalorimeter observations. With the recent developments of the spectral simulation code Cloudy, inspired by the high spectral resolution of the…

高能天体物理现象 · 物理学 2025-02-19 Chamani M. Gunasekera , Peter A. M. van Hoof , Masahiro Tsujimoto , Gary J. Ferland

Pulses of extreme ultraviolet (XUV) light, with wavelengths between 10 and 100$\,$nm, can be used to image and excite ultra-fast phenomena such as the motion of atomic electrons. Here we show that the illumination of plasma with…

等离子体物理 · 物理学 2018-08-24 T. G. Blackburn , A. A. Gonoskov , M. Marklund

The Soft X-ray Spectrometer (SXS) on board \textit{Hitomi}, with the unprecedented resolving power of R$\sim$1250, allowed the detection of members of the Fe XXV \ka\ complex emission spectra from the center of the Perseus Cluster. In this…

高能天体物理现象 · 物理学 2020-09-30 P. Chakraborty , M. Chatzikos , F. Guzmán , Y. Su , G. J. Ferland

Experimental results for the reflection coefficient of shock-compressed dense Xenon plasmas at pressures of 1.6 - 17 GPa and temperatures around 30 000 K using a laser beam with \lambda = 1.06 10^-6 m are compared with calculations based on…

等离子体物理 · 物理学 2009-11-07 H. Reinholz , G. Roepke , A. Wierling , V. Mintsev , V. Gryaznov

The 1s2-1s2l lines are the most intense He-like ions lines. They are used as spectroscopic diagnostics for solar active regions as well as for different laboratory plasmas. Nowadays, it exits very high spectral resolution instruments and,…

天体物理学 · 物理学 2007-05-23 Jacques Dubau , Delphine Porquet

The Serendipitous Extragalactic X-ray Source Identification (SEXSI) Program is designed to extend greatly the sample of identified extragalactic hard X-ray 2-10 keV sources at intermediate fluxes ($\sim 10^{-13} - 10^{-15} erg/cm2/s$).…

天体物理学 · 物理学 2009-11-10 Fiona A. Harrison , Megan E. Eckart , Peter H. Mao , David J. Helfand , Daniel Stern

We have used an electron beam ion trap to measure electron-density-diagnostic line-intensity ratios for extreme ultraviolet lines from F XII, XIII, and XIV at wavelengths of 185-205 255-276 Angstroms. These ratios can be used as density…

In simulations of a 12.5PW laser (focused intensity I = 4x10^23W/cm^2) striking a solid aluminium target 10% of the laser energy is converted to gamma-rays. A dense electron-positron plasma is generated with a maximum density of 10^26/m^3;…

等离子体物理 · 物理学 2016-11-26 C. P. Ridgers , C. S. Brady , R. Duclous , J. G. Kirk , K. Bennett , T. D. Arber , A. R. Bell

A number of giant HII regions are associated with soft diffuse X-ray emission. Among these, the Carina nebula possesses the brightest soft diffuse emission. The required plasma temperature and thermal energy can be produced by collisions or…

天体物理学 · 物理学 2009-11-13 Kenji Hamaguchi , the Suzaku Eta Carinae team , the Carinae D-1 team

Using the Livermore X-ray Spectral Synthesizer, which calculates spectral models of highly charged ions based on HULLAC atomic data, we investigate the temperature, density, and photoexcitation dependence of the I(11.92 A)/I(11.77 A) line…

天体物理学 · 物理学 2007-05-23 Christopher W. Mauche , Duane A. Liedahl , Kevin B. Fournier