| Home > Publications database > Spatial characteristics of K alpha X-ray emission from relativistic femtosecond laser plasmas > print | 
| 001 | 31495 | ||
| 005 | 20230217124338.0 | ||
| 024 | 7 | _ | |2 DOI |a 10.1103/PhysRevE.68.056408  | 
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| 084 | _ | _ | |2 WoS |a Physics, Fluids & Plasmas  | 
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| 100 | 1 | _ | |a Reich, Ch. |b 0 |0 P:(DE-HGF)0  | 
| 245 | _ | _ | |a Spatial characteristics of K alpha X-ray emission from relativistic femtosecond laser plasmas | 
| 260 | _ | _ | |a College Park, Md. |b APS |c 2003  | 
| 264 | _ | 1 | |3 online |2 Crossref |b American Physical Society (APS) |c 2003-11-21  | 
| 264 | _ | 1 | |3 print |2 Crossref |b American Physical Society (APS) |c 2003-11-01  | 
| 300 | _ | _ | |a 056408 | 
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| 440 | _ | 0 | |a Physical Review E |x 1539-3755 |0 4924 |v 68  | 
| 500 | _ | _ | |a Record converted from VDB: 12.11.2012 | 
| 520 | _ | _ | |a The spatial structure of the Kalpha emission from Ti targets irradiated with a high intensity femtosecond laser has been studied using a two-dimensional monochromatic imaging technique. For laser intensities I<5x10(17) W/cm(2), the observed spatial structure of the Kalpha emission can be explained by the scattering of the hot electrons inside the solid with the help of a hybrid particle-in-cell/Monte Carlo model. By contrast, at the maximum laser intensity I=7x10(18) W/cm(2) the half-width of the Kalpha emission was 70 mum compared to a laser-focus half-width of 3 mum. Moreover, the main Kalpha peak was surrounded by a halo of weak Kalpha emission with a diameter of 400 mum and the Kalpha intensity at the source center did not increase with increasing laser intensity. These three features point to the existence of strong self-induced fields, which redirect the hot electrons over the target surface. | 
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| 700 | 1 | _ | |a Uschmann, I. |b 1 |0 P:(DE-HGF)0  | 
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| 700 | 1 | _ | |a Düsterer, S. |b 3 |0 P:(DE-HGF)0  | 
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| 700 | 1 | _ | |a Schwoerer, H. |b 5 |0 P:(DE-HGF)0  | 
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| 700 | 1 | _ | |a Gibbon, P. |b 8 |u FZJ |0 P:(DE-Juel1)132115  | 
| 773 | 1 | 8 | |a 10.1103/physreve.68.056408 |b American Physical Society (APS) |d 2003-11-21 |n 5 |p 056408 |3 journal-article |2 Crossref |t Physical Review E |v 68 |y 2003 |x 1063-651X  | 
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| 856 | 7 | _ | |u http://dx.doi.org/10.1103/PhysRevE.68.056408 | 
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