July 2020 Contract awarded from Lawrence Livermore National Laboratory. Artep will design, fabricate and align four new elliptically bent crystal packs for the existing NXS spectrometer.
January 2020 Contract awarded from Lawrence Livermore National Laboratory. Artep will design, and fabricated five crystal holders to be uses in the Imaging and Spectroscopy snout (ISS) spectrometer.
April 2019 Contract awarded from Lawrence Livermore National Laboratory Artep will provide a design of two reflection spectrometers that will incorporate toroid shaped GaAs diffraction crystals designed to record spectra in the hard x-ray range.
July 2018 Contract awarded from Lawrence Livermore National Laboratory Artep designed and fabricated five crystal holders to be uses in the Imaging and Spectroscopy snout (ISS) spectrometer.
December 2017 Contract awarded from Lawrence Livermore National Laboratory Artep designed, fabricated, and aligned a high energy x-ray spectrometer for spectroscopic analysis work to be performed at the AWE Orion Laser facility.
July, 2011 |
||
Artep awarded engineering support contract from ATK Space Systems Inc. The Artep engineering support involves development, test and implementation of hardware and software systems for real-time payload operations and control for ground support equipment for satellites and sounding rockets. The work also includes flight instrument testing and calibration, scientific data analysis and image processing. | ||
May, 2011 | ||
Artep awarded scientific support contract from NASA/Goddard Space Flight Center Artep will provide scientific support to the NASA investigation “The Dynamics of Neutral-Line Flows During CME’s & Flares” | ||
April, 2011 | ||
Artep awarded mechanical modification contract from SLAC National Accelerator Laboratory Artep will generate modification drawings and modify an existing stand to be compatible with LCLS. | ||
April, 2011 | ||
Artep awarded electronic development contract from Virginia Tech University Artep will design and fabricate a PCB suitable for a future flight of the Virginia Tech PolarNox sounding rocket. The new board will acquire data from the Star-1000 camera. The camera interface board will be designed for rapid sampling of large images. The camera interface board will have the ability to acquire full 1024 x 1024 pixel images from the Star-1000 and buffer them for transmission to the NASA Wallops WFF TM using the 10MBit link. | ||
February, 2011 | ||
Virginia Tech PolarNox sounding rocket successfully launched from Poker Flat Alaska Artep was responsible for the electronic controller, power system and distribution, camera interface, wire harnessing, flight software and Ground Support Equipment (GSE). | ||
November, 2010 | ||
Artep awarded instrument development contract from Lawrence Livermore National Laboratory/AWE This contract is for developing a pulsed x-ray source for testing streak cameras. The requirements are for an x-ray source that produces sufficient flux in the 10kev energy region for testing the operation and timing of LLNL X-ray streak cameras having picosecond time resolution. | ||
November, 2010 | ||
Artep awarded instrument development contract from Lawrence Livermore National Laboratory This contract is for the modification of the Artep built GCS. The spectrometer with IP holders will be modified to be compatible with an OMEGA-EP TIM. | ||
July, 2010 | ||
Artep awarded scientific support contract from NASA/Goddard Space Flight Center Artep will provide scientific and data analysis support to the Investigation of the Dynamics and Origin of neutral-line Shear Flows. | ||
June, 2010 | ||
Artep awarded scientific support contract from National Science Foundation (NSF). This research will address one of the fundamental themes of NSF’s Solar Terrestrial Program, namely the connection between magnetic structures at the solar surface and coronal mass ejections. The scientific goals of this research contract is to further the understanding of the structure, formation, and eruption of filaments. The specific studies that Artep intends to pursue are the following: 1. Filament Channel Formation 2. Barb formation 3. Filament Endpoint Brightenings. 4. Mixed Helicity in Erupting Filaments. | ||
May, 2010 | ||
Artep awarded instrument development contract from Lawrence Livermore National Laboratory Artep was given a contract to provide the absolute sensitivity calibration of the LLNS Crystal Spectrometer that was built by Artep for LLNL and delivered May 2009. Please contact us for detailed information regarding the sensitivity calibration. | ||
April, 2010 | ||
Artep awarded instrument development contract from Lawrence Livermore National Laboratory Artep was awarded a contract for the development of a Gamma Crystal Spectrometer (GCS) for detecting 511 keV Positron Annihilation Radiation. This instrument is built for the LLNL Titan laser facility. The design of this spectrometer is based on a transmission Crystal Spectrometer that was fabricated by Artep and successfully fielded in a TIM at the EP laser in August 2009. Please contact us for detailed information regarding this spectrometer. | ||
April, 2010 | ||
Artep awarded scientific support contract from University of Michigan at Ann Arbor. The Center for Radiative Shock Hydrodynamics (CRASH), at the Atmospheric, Oceanic and Space Sciences Department of University ofMichiganis involved in a large research effort to study radiative shocks for application to ICF and Astrophysics. Artep will provide support service for computation of radiative emissivities and opacities (REO) for various elements and compounds relevant to the CRASH project – for all temperatures and densities necessary. | ||
June, 2009 | ||
Artep awarded instrument development contract from Lawrence Livermore National Laboratory Artep will design and build a streak-camera compatible hard x-ray spectrometer that can be fielded at the LLNL Titan laser facility and at the NIF facility. Please contact us for detailed information regarding this spectrometer | ||
May, 2009 | ||
Artep awarded instrument development contract from Lawrence Livermore National Laboratory Artep will design and build a hard x-ray spectrometer that can be fielded at the LLNL Titan laser facility and at the NIF facility. The spectrometer will be similar in performance (covering 17-102 keV x-ray energies) and operation to the LULI Crystal Spectrometer (LCS) that was fielded at Titan and is currently being qualified at the Omega-EP facility. Please contact us for detailed information regarding this spectrometer. | ||
April, 2009 | ||
Artep awarded SBIR Phase-II contract from Air Force Artep will develop, test and deliver a space flight prototype Doppler Asymmetric Spatial Heterodyne (DASH) Spectrometer for measuring winds in the upper atmosphere. In addition Artep will develop an optical Doppler shift scene simulator and measure the Doppler shift from a simulated scene of the Earth’s limb. | ||
January 30, 2008 | ||
New Contract with USAF, Hanscom AFB | ||
Artep is awarded an SBIR Phase-I contract for the feasibility study of developing a Doppler Asymmetric Spatial Heterodyne Spectrometer (DASH) for measuring Winds in the Upper Atmosphere (90-300km). | ||
January 23, 2008 | ||
New contract award with Virginia Polytechnic Institute and State University | ||
Artep is awarded a contract to support the Virginia Tech delivery to NASA of an NO sounding rocket instrument that is to launch from Poker Flat Alaska. Artep will be responsible for the flight electronics, flight software, Ground Support Equipment (GSE), integration and launch support. | ||
September 18, 2006 | ||
New contract award from NASA Goddard Space Flight Center | ||
Artep is awarded a three year contract to study the Solar Wind Origin and Acceleration Over the Solar Cycle. | ||
June 14, 2006 | ||
New contract award with Virginia Polytechnic Institute and State University | ||
Artep is awarded a contract to refurbish and support an Avalanche Photodiode X-Ray Spectrometer (AXS) that is to be integrated and launched out ofWhiteSandsMissileRangeinNew Mexico. | ||
June 10, 2005 | ||
Artep Awarded multi year contract for continued support of NRL’s Plasma Physics Division. | ||
As a follow on to the previous research contract with Plasma Physics (Analysis of the interaction of radiation with non-LTE plasmas)the following was proposed.We will develop two advanced models for improving atomic physics for the hydrodynamic simulations of laser plasmas. These will be delivered as ancillary Fortran components for hydrodynamic codes.:1)- For the Equation of State (EOS) in laser produced ICF plasmas, we envisage an average atom model embedded in a constant external potential (due to a neutralizing background of free electrons and ions) and contained in a ion sphere. The novelty is the treatment of quasi-free electrons (a.k.a shape resonances). These will ensure smooth variations of the free energy, allowing numerical differentiation to obtain entropy and other relevant quantities. In addition, the pressure can be obtained directly from the virial theorem if relativistic wavefunctions are used. An extension to non LTE (non Local Thermodynamical equilibrium) is also proposed.2)-A detailed level accounting (DLA) model for the opacity of simple to medium spectra. In contradistinction to statistical models that are widely in use, this detailed model will be correct for systems at low density and high temperature, as in the corona where high Z elements are used. In particular, it will be able to handle metastable levels that can modify noticeably the charge distribution.We will also design, manage the construction, and modification of a time resolved, and absolutely calibrated instruments for Laser Plasma Interaction studies. | ||
March 8, 2005 | ||
New contract award from NRL’s Space Science Division | ||
Artep has been awarded a new five-year contract to continue science and engineering support for NRL’s Space Science Division. This work currently supports a number of key satellite and rocket programs, that include Solar-B, SECCHI, SHIMMER and VAULT. | ||
On going contract with NRL’s Plasma Physics Division | ||
Artep is in the midst of a five-year contract supporting theoretical and laboratory experimental science being conducted by NRL’s Plasma Physics Division.Title: Analysis of the interaction of radiation with non-LTE plasmasThe Naval Research Laboratory Laser Plasma Branch successfully built in recent years a kilojoule-class KrF laser called the Nike Facility. An important purpose of Nike is to investigate various methods of controlling hydrodynamic instabilities in laser accelerated targets. One of the primary methods considered uses controlled amounts of high Z-generated radiation that preheats the ablator, thus modifying the density profile of the target while leaving the fuel on low isentrope. The interaction of intense laser light with a target is known to have several features that are essentially non-LTE, due to the existence of temperature and density gradients, and optically thin regions. To take into account non-LTE effects with the same accuracy as the Super-Transition-Array (STA) model does for LTE, the NRL Laser Plasma Branch implemented the approach of Busquet, showing generally satisfactory agreements when compared with benchmark computations.In support of the Nike target design effort Artep scientists are carrying out the following studies:Using STA to generate opacities for materials and mixtures specified by the target development team.Validating target design by comparing the measured emitted X-ray spectra from the target with theoretical predictions.Improving the Busquet algorithmInvestigating ways of representing the target radiation field in a collisional radiative model such as the SCROLL and FAST that could be interfaced in a satisfactory manner. (FAST is radiation hydrodynamic code that uses LTE atomic physics to calculate opacities of various materials and SCROLL is a super configuration collisional radiative model). | ||
New contract award from NASA Goddard Space Flight Center | ||
Artep has been awarded a new three-year contract with NASA to study the transition region explosive events and their relation to the solar magnetic field.Magnetic field restructuring by reconnection is pervasive in astrophysics and in particular in solar physics. Magnetic reconnection can potentially provide the energy to heat and accelerate the plasma in the solar atmosphere, but it has proved elusive to direct observations.Explosive events are thought to be an observable manifestation of small-scale reconnection in the transition region of the solar atmosphere. Using simultaneous data recorded bySUMER, MDI and EIT all instruments on the Solar and Heliospheric Observatory (SOHO) and from the Transition Region and Coronal Explorer (TRACE) Artep scientists are engaged in the following studies:Pinpoint the spatial relationship between the photospheric magnetic field structures and explosive events in the quiet Sun, active regions and coronal holes.Characterize the dynamic and energy budget of explosive events in relation to the magnetic field.Find signatures of magnetic reconnection in the solar corona. |