MOONLANDER HHG
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The Moonlander HHG is an efficient coherent EUV source for time-resolved spectroscopy such as ARPES. Driven by our high-power White Dwarf HE OPCPA, the Moonlander HHG-50 provides high photon flux at high repetition rates in a robust, reliable design.
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Applications
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Specifications
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Performance
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Downloads
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Contact
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Ultrafast material science
2D Infrared spectroscopy (2DIR) / Multi-color pump-probe, Mid-IR and THz spectroscopy / Magneto-optical Kerr-effect (MOKE) microscopy / Raman spectroscopy (CARS, GAMERS)
• Strong-field physics
• Relativistic plasma physics |
• Cluster and gasphase dynamics
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• Carrier dynamics of
solid materials • Photosynthesis |
• Strong-field physics
• Relativistic plasma physics |
Time-resolved ARPES
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OPCPA is a versatile tool which provides ultra-short pulses from the UV to the mid-infrared.
Combined with our high flux, high repetition rate Moonlander HHG source, this makes OPCPA the ideal technology platform for time-resolved photoelectron spectroscopy. |
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EUV and soft X-Ray science
Coherent diffractive imaging (CDI) / Time-resolved reaction microscopy (ARPES) / Coherent control / Attosecond streaking
• Bioparticle imaging
• Nanoparticles and clusters |
• Inspection in EUV
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• Attosecond dynamics
in solids and gases |
The Moonlander HHG-50 is a high flux coherent EUV source for time-resolved spectroscopy such as ARPES. Our White Dwarf HE OPCPA serves as an ultrashort driver at 400 nm or 800 nm with excellent temporal contrast and clean pulse profile to drive stable and efficiently higher harmonics. Hence, the Moonlander HHG-50 provides high photon flux at high repetition rates with long-term stable operation based on a robust, reliable design.
A second, synchronized optical output from UV to mid-IR can be provided with our White Dwarf HE OPCPA, hence offering a full pump-probe suite to take the next step in time-resolved photoelectron spectroscopy.
A second, synchronized optical output from UV to mid-IR can be provided with our White Dwarf HE OPCPA, hence offering a full pump-probe suite to take the next step in time-resolved photoelectron spectroscopy.
Moonlander HHG-50 |
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Driver inclusive |
White Dwarf HE OPCPA at 400 nm or 800 nm |
Photon energy |
21...50 eV |
Wavelength |
24...59 nm |
Spectral bandwidth (FWHM) |
ca 100 meV depending on driver |
Photon flux at source |
> 5x10^12 ph/sec @ 38 eV |
Photon flux filtered (single-harmonic) |
> 1x10^12 ph/sec @ 38 eV |
Repetition rate |
100 kHz, higher on request |
Focusing and steering |
on request |
Full pump-probe suite |
optionally based on White Dwarf HE OPCPA |
User interface |
motor control for target position and target camera, remote gas pressure control, diode for EUV flux measurement |
Normalized spectral intensity: Moonlander HHG-50 driven by White Dwarf HE OPCPA at 800 nm at 100 kHz.
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