Hans Pecseli

Prof. Hans Pecseli

orcid

Research Focus & Metrics

Academic Career Length

54Years (1973-Present)

(Calculated once Scilit publication data is synced: current year − year of first publication + 1)

Representative Publications

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19 February 1979 in Physical Review Letters
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Journal Article
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KSK. Saeki
K. Saeki
PMP. Michelsen
P. Michelsen
HPHans Pecseli
Hans Pecseli
JRJens Juul Rasmussen
Jens Juul Rasmussen
Electron solitary holes were observed in a magnetized collisionless plasma. These holes were identified as Bernstein-Green-Kruskal equilibria, thus being purely kinetic phenomena. The electron hole does not damp even though its velocity is close to the electron thermal velocity. Two holes attract each other like particles of negative mass, and coalesce when their relative velocity is small.

1 September 1979 in Physica Scripta
Verified
Journal Article
Closed access
JLJ P Lynov
J P Lynov
PMP Michelsen
P Michelsen
HPHans Pecseli
Hans Pecseli
JRJens Juul Rasmussen
Jens Juul Rasmussen
KSK Saéki
K Saéki
VTV A Turikov
V A Turikov

1 July 1987 in The Physics of Fluids
Verified
Journal Article
Closed access
HJH. Johnsen
H. Johnsen
HPHans Pecseli
Hans Pecseli
JTJ. Trulsen
J. Trulsen
Low‐frequency electrostatic turbulence generated by the ion–ion beam instability was investigated experimentally in a double‐plasma device. Real time signals were recorded and examined by a conditional statistical analysis. Conditionally averaged potential distributions reveal the formation and propagation of structures with a relatively long lifetime. Various methods for making a conditional analysis are discussed and compared. The results are discussed with reference to ion phase space vortices and clump formation in collisionless plasmas.

24 June 2002 in Physical Review E
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Journal Article
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Eduard KontarEduard Kontar
Eduard Kontar
HPHans Pecseli
Hans Pecseli
The self-consistent description of Langmuir wave and ion-sound wave turbulence in the presence of an electron beam is presented for inhomogeneous nonisothermal plasmas. Full numerical solutions of the complete set of kinetic equations for electrons, Langmuir waves, and ion-sound waves are obtained for an inhomogeneous unmagnetized plasma. The results show that the presence of inhomogeneity significantly changes the overall evolution of the system. The inhomogeneity is effective in shifting the wave numbers of the Langmuir waves, and can thus switch between different processes governing the weakly turbulent state. The results can be applied to a variety of plasma conditions, where we choose solar coronal parameters as an illustration, when performing the numerical analysis.

1 January 1982 in Physica Scripta
Verified
Journal Article
Closed access
KDK B Dysthe
K B Dysthe
EME Mjølhus
E Mjølhus
HPHans Pecseli
Hans Pecseli
KRK Rypdal
K Rypdal

1 July 1991 in Physics of Fluids B: Plasma Physics
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Journal Article
Closed access
THThomas Huld
Thomas Huld
ANA. H. Nielsen
A. H. Nielsen
HPHans Pecseli
Hans Pecseli
JRJens Juul Rasmussen
Jens Juul Rasmussen