Michael Börner

Dr. Michael Börner

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Research Focus & Metrics

Academic Career Length

15Years (2012-Present)

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

Representative Publications

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12 March 2013 in Physical Review Letters
Verified
Journal Article
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AFA. Frank
A. Frank
ABA. Blažević
A. Blažević
VBV. Bagnoud
V. Bagnoud
MBM. M. Basko
M. M. Basko
MBMichael Börner
Michael Börner
MRM. Roth
M. Roth
This Letter reports on the measurement of the energy loss and the projectile charge states of argon ions at an energy of 4  MeV/u penetrating a fully ionized carbon plasma. The plasma of ne≈1020  cm−3 and Te≈180  eV is created by two laser beams at λLas=532  nm incident from opposite sides on a thin carbon foil. The resulting plasma is spatially homogenous and allows us to record precise experimental data. The data show an increase of a factor of 2 in the stopping power which is in very good agreement with a specifically developed Monte Carlo code, that allows the calculation of the heavy ion beam’s charge state distribution and its energy loss in the plasma.

1 April 2012 in Review of Scientific Instruments
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Journal Article
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MBMichael Börner
Michael Börner
JFJ. Fils
J. Fils
AFA. Frank
A. Frank
ABA. Blažević
A. Blažević
THT. Hessling
T. Hessling
MRM. Roth
M. Roth
This article reports on the development and set-up of a Nomarski-type multi-frame interferometer as a time and space resolving diagnostics of the free electron density in laser-generated plasma. The interferometer allows the recording of a series of 4 images within 6 ns of a single laser-plasma interaction. For the setup presented here, the minimal accessible free electron density is 5 × 1018 cm−3, the maximal one is 2 × 1020 cm−3. Furthermore, it provides a resolution of the electron density in space of 50 μm and in time of 0.5 ns for one image with a customizable magnification in space for each of the 4 images. The electron density was evaluated from the interferograms using an Abel inversion algorithm. The functionality of the system was proven during first experiments and the experimental results are presented and discussed. A ray tracing procedure was realized to verify the interferometry pictures taken. In particular, the experimental results are compared to simulations and show excellent agreement, providing a conclusive picture of the evolution of the electron density distribution.

10 February 2018 in CEAS Space Journal
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Journal Article
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MBMichael Börner
Michael Börner
CMChiara Manfletti
Chiara Manfletti
JHJustin Hardi
Justin Hardi
DSDmitry Suslov
Dmitry Suslov
GKGerhard Kroupa
Gerhard Kroupa
MOMichael Oschwald
Michael Oschwald

19 June 2017 in CEAS Space Journal
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Journal Article
Closed access
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MBMichael Börner
Michael Börner
CMChiara Manfletti
Chiara Manfletti
GKGerhard Kroupa
Gerhard Kroupa
MOMichael Oschwald
Michael Oschwald

1 June 2018 in Acta Astronautica
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Journal Article
Closed access
Justin Steven HardiJustin Steven Hardi
Justin Steven Hardi
TTTobias Traudt
Tobias Traudt
CBCristiano Bombardieri
Cristiano Bombardieri
MBMichael Börner
Michael Börner
SBScott K. Beinke
Scott K. Beinke
MOMichael Oschwald
Michael Oschwald

8 January 2020 in CEAS Space Journal
Verified
Journal Article
Open access
PDF file
SKSebastian Klein
Sebastian Klein
MBMichael Börner
Michael Börner
JHJustin S. Hardi
Justin S. Hardi
DSDmitry Suslov
Dmitry Suslov
MOMichael Oschwald
Michael Oschwald
This paper reports the investigation of acoustic combustion instability experienced during repetitive ignition testing of a sub-scale LOX-methane rocket thrust chamber. The occurrence of resonant coupling between the LOX injectors and the combustion chamber acoustic modes was assessed from the experimental data recorded during the highly transient phase of operation from ignition up to around 2 s. A method was developed to model the evolution of acoustic properties in both the combustion chamber and the injectors during the transient period. For the LOX injectors, the Woods equation was used to estimate the speed of sound in the two-phase flow. The models were used to identify the corresponding mode frequencies in the unsteady pressure measurements, and show that the high-amplitude instability occurred when they intersected. Very close coupling of less than 3% frequency difference is required for high amplitudes to be observed. However, the condition was necessary but not sufficient for high amplitudes to be reached.