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Magnetic reconnection
Magnetic reconnection

... (e-p collision) • Ionization non-equilibrium → strong heating or flare time scale for equilibrium is relatively long ...
Plasma-assisted combustion for gas turbine application
Plasma-assisted combustion for gas turbine application

Mike Zellner
Mike Zellner

Three-scale structure of diffusion region of magnetic reconnection in
Three-scale structure of diffusion region of magnetic reconnection in

Investigation of Atmospheric Pressure Plasma Source for CO  Dissociation
Investigation of Atmospheric Pressure Plasma Source for CO Dissociation

... about 4 eV/mol with 8 slm of CO2 flowing in the discharge. Yet this operating condition has the lowest conversion efficiency of about 25%. Likewise, the operating condition with highest conversion efficiency of about 100% at Ev = 27 eV/mol has the lowest energy efficiency of 10%. As the flow rate of ...
7510-13 NATIONAL AERONAUTICS AND SPACE
7510-13 NATIONAL AERONAUTICS AND SPACE

Time evolution of the particle distribution function in a high
Time evolution of the particle distribution function in a high

ARTEMIS writeup
ARTEMIS writeup

... Lunar Prospector had a precessing polar orbit about the Moon with an orbital period of about 118 minutes and an altitude about 100 km at the time of these measurements. In a Moon-centered (x,y,z) coordinate system with x along the Moon-Sun line, z along the rotation axis and y perpendicular to x an ...
slides
slides

Kinetic Studies of Nonrelativistic Young Supernova Remnant
Kinetic Studies of Nonrelativistic Young Supernova Remnant

... density of electrons and ions that lead to the formation of the double-shock structure. Thus, electron dynamics play an important role in the development of the system. Ionion or ion-electron streaming generally drives the turbulence, which is mainly magnetic. The exact type of an instability, howev ...
Collisionless interaction of an energetic laser produced plasma C. Constantin
Collisionless interaction of an energetic laser produced plasma C. Constantin

... vs ||B' within ± 45◦ ), the shock formation time is believed to be much longer, of the order of the growth-rate of the firehose instability (∼10Tci ) (Draine 1993). This means that the number of gyroperiods per shock transit time NT = (L/vs )/Tci must be larger than 1 in the quasi-perpendicular case ...
Diagnostic research of highly ionized plasma generated by an ECR
Diagnostic research of highly ionized plasma generated by an ECR

... can support the development of methods for production and investigation of plasmas from solid samples and powders (e.g. other metals and fullerenes). Very heavy low charged ions (e.g. C>) are very ...
Slide 1
Slide 1

The influence of negatively charged, heavier
The influence of negatively charged, heavier

... the crash of a comet on rocky surfaces was all that was needed for seeding planets (and their satellites) with amino acids – the basic building blocks so essential for the development of life. Very recently, it was demonstrated experimentally for the first time in a laboratory that amino acids are i ...
Final Presentation PPT
Final Presentation PPT

... Pressure peak formed also drives down-flowing ...
Fine structure of the interplanetary shocks observed by BMSW
Fine structure of the interplanetary shocks observed by BMSW

The Sun`s Magnetic Field Twisting Magnetic Fields PRS: Sunspots
The Sun`s Magnetic Field Twisting Magnetic Fields PRS: Sunspots

... 3. Nuclear reactions occur in them more slowly than in the surrounding gas. 4. Clouds in the cool corona block our view of the ...
The impact of black holes on the Universe
The impact of black holes on the Universe

Solar-B - to Nobeyama Radio Observatory
Solar-B - to Nobeyama Radio Observatory

... EIS (optics components), NASA polar station(s) ...
Plasma Seminar 4/23/07 "Negative Ion Plasmas"
Plasma Seminar 4/23/07 "Negative Ion Plasmas"

... neutral beam systems • magnetically confined fusion plasmas are heated by neutral beam injection (150 keV D+) • cannot accelerate neutral atoms • accelerate H+ then neutralize by charge exchange  inefficient at >100 keV • however, with H-, the neutralization efficiency remains high out to 500 keV. ...
Plasma physics, space research and the origin of the solar system
Plasma physics, space research and the origin of the solar system

Plasma Astrophysics
Plasma Astrophysics

ng - CAPCA
ng - CAPCA

... second field generation mechanism: – Displaces plasma electrons – Plasma ions try to restore neutrality: space charge oscillation ...
CIII 97.7 nm - Astronomy at Swarthmore College
CIII 97.7 nm - Astronomy at Swarthmore College

Written Transcript of this video lesson
Written Transcript of this video lesson

... works. These lamps are widely used; we find them in houses, offices, shops and many other places. Basically, fluorescent lamp consists of a glass tube. This tube is vacuumed, its two ends are connected to electrodes that are attached to a filament, the inner surface of the bulb is coated with phosph ...
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Variable Specific Impulse Magnetoplasma Rocket

The Variable Specific Impulse Magnetoplasma Rocket (VASIMR) is an electromagnetic thruster for spacecraft propulsion. It uses radio waves to ionize and heat a propellant, and magnetic fields to accelerate the resulting plasma to generate thrust. It is one of several types of spacecraft electric propulsion systems.The method of heating plasma used in VASIMR was originally developed as a result of research into nuclear fusion. VASIMR is intended to bridge the gap between high-thrust, low-specific impulse propulsion systems and low-thrust, high-specific impulse systems. VASIMR is capable of functioning in either mode. Costa Rican–born American scientist and former NASA astronaut Franklin Chang Díaz created the VASIMR concept and has been working on its development since 1977.VASIMRs units for development and test have been assembled by the Ad Astra Rocket Company, headquartered in the city of Houston, Texas, United States.
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