GRIMM Aerosol Technik GmbH & Co. KG
GRIMM - Model 11-D - Dust Decoder - Portable aerosol spectrometer SECURE YOUR DISCOUNT TODAY! The most powerful dust monitor. The model 11-D, in its compact and rugged design,
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GRIMM - Model 11-D - Dust Decoder - Portable aerosol spectrometer SECURE YOUR DISCOUNT TODAY! The most powerful dust monitor. The model 11-D, in its compact and rugged design,
Dominik Waldburger''s 56 research works with 759 citations and 3,032 reads, including: Calibration of high-accuracy spectrometers using stabilized 11-GHz femtosecond semiconductor laser
The spacecraft will be equipped with the DESTINY + Dust Analyzer (DDA) which will be a time-of-flight impact ionization mass spectrometer. In addition to the composition of impacting dust
This configuration places the 11-D in the leading po-sition of the portable aerosol spectrometers for moni- toring inhalable, thoracic and respirable dust, PM val-ues, and particle number concentration.
Cassini Cosmic Dust Detector, CDA The Cosmic Dust Analyzer (CDA) was a large-area (0.1 m 2 total sensitive area) multi-sensor dust instrument included on the Cassini spacecraft, which was launched
Dominik Charczun: 3 Followers, 1 Following, 4 Research papers. Research interests: Surfactant Science & Technology, Fluid structure interaction, and Fluids.
We report on the design and testing of a compact impact-ionization time-of-flight mass spectrometer for analysis of cosmic dust, suitable for use on deep space missions.
Dr. Friedhelm Schneider, Product Manager at GRIMM, on the launch of the new product, "The latest generation of our aerosol spectrometer sets
Precise and compact aerosol spectrometer for the determination of dust mass fractions and particle number size distribution. Optimal solution for reliable and flexible real-time measurements for aerosol
Optool computes dust opacities and scattering matrices, for specific grain sizes or averaged over size distributions. It is derived from OpacityTool (ascl:2104.009) and implements the Distribution of Hollow
To study cosmic dust analogs, we installed dust samples, embedded in low-density polyethylene (LDPE) pellets, in a sample-exchanger and cooled it down within a cryostat to 3.0 Kelvin.
Dominic Hinz I started my doctoral studies in February 2019 at the KATRIN experiment. My further research focuses on background studies in the KATRIN spectrometers due to intrinsic radioactivity,
Command-line driven tool to create dust opacities. Contribute to cdominik/optool development by creating an account on GitHub.
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Spectroscopy is an essential tool to investigate the composition and structure of cosmic matter. To interpret astronomical observations, laboratory astrophysics experiments are built and dedicated to
Nitrogen-vacancy (NV) quantum defects in diamond are sensitive detectors of magnetic fields. Owing to their atomic size and optical readout capability, they have been used for magnetic resonance
Size-dependence of physicochemical processes on cosmic dust surfaces is a fundamental aspect for understanding the formation of complex organic molecules in space and improving the
Dominik A. Hecker - Dust | Epic Heroic Fantasy Orchestral Music Premium Music HQ 545K subscribers Subscribed
Nitrogen-vacancy (NV) quantum defects in diamond are sensitive detectors of magnetic fields. Owing to their atomic size and optical readout capability, they have been used for magnetic resonance
Ia supernovae produce the majority of interstellar iron but do ot appear to produce dust. Therefore, iron dust must form rapidly in the ISM (Dwek, 2016). Olivine is a prime candidate material for interstellar
Abstract We performed an experiment under long-term microgravity conditions aboard the International Space Station (ISS) to obtain information on the energetics and experimental constraints required for
We present new James Webb Space Telescope (JWST) NIRSpec and MIRI integral-field spectroscopy of the remarkable system SN~2010da / NGC~300 ULX-1, the only known ultraluminous
Interstellar Dust Experiment | Purpose: IDEX provides the elemental composition, speed and mass distributions of interstellar dust particles.
Sometime in the last 20 million years, one or more stars in the solar neighborhood went supernova, producing clouds of gas and dust enriched with radioisotopes. As the Solar System
We developed a compact time-of-flight mass spectrometer (TOF-MS) for the sensitive investigation of gas samples in planetary missions. The advantage of a TOF-MS for space research is its fairly...
Dominic Berger Affiliation Institute of Signal Processing and Wireless Communications, Zurich University of Applied Sciences, Winterthur, Switzerland Publication Topics
We have presented new NIRSpec and MIRI IFU spectroscopy of SN 2010da / NGC 300 ULX–1, revealing that the system remains luminous but is now heavily obscured by warm, optically
The dust composition was analyzed by infrared spectroscopy and the molecular composition by laser mass spectrometry. The experimental methodology was complemented by density functional theory
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