A5083777660- Solar and Space Plasma Dynamics
- Astro and Planetary Science
- Conducting polymers and applications
- Electrochemical sensors and biosensors
- Theoretical and Computational Physics
- Organic Electronics and Photovoltaics
- Gas Sensing Nanomaterials and Sensors
- Advanced Sensor and Energy Harvesting Materials
- Microfluidic and Capillary Electrophoresis Applications
- Hydrogen Storage and Materials
- Methane Hydrates and Related Phenomena
- Electronic Packaging and Soldering Technologies
- Electron and X-Ray Spectroscopy Techniques
- Copper Interconnects and Reliability
- Magnetic confinement fusion research
- Particle Accelerators and Free-Electron Lasers
- Surface and Thin Film Phenomena
- Advanced Thermodynamics and Statistical Mechanics
- Electrocatalysts for Energy Conversion
- Fuel Cells and Related Materials
- Astrophysics and Star Formation Studies
- Atomic and Subatomic Physics Research
- Statistical Mechanics and Entropy
- Analytical Chemistry and Sensors
- Ionosphere and magnetosphere dynamics
Dartmouth College
2024
Texas A&M University
1989
Abstract Interstellar neutral (ISN) hydrogen is the most abundant species in outer heliosheath and very local interstellar medium (VLISM). Charge-exchange collisions result filtration, reducing ISN density inside heliosphere. Additionally, these atoms are intensively ionized close to Sun, resulting a substantial reduction of their within few astronomical units from Sun. The products this ionization—pickup ions (PUIs)—are detected by charged particle detectors. Solar Wind Around Pluto...
Radiation pressure exerted by solar photon output is salient to the motion of primary neutral hydrogen atoms streaming into inner heliosphere directly from Local Interstellar Medium (LISM). The action a time-dependent radiation force, when coupled with usual gravitational changes characteristic velocities, and therefore energies, they reach regions in which explorer probes are present. A study presented that uses 2D code backtrace trajectories representative target points located 1 au Sun....
Abstract Radiation pressure exerted by solar photon output is salient to the motion of primary neutral hydrogen atoms streaming into inner heliosphere directly from local interstellar medium. The action a time-dependent radiation force, when coupled with usual gravitational changes characteristic velocities, and therefore energies, they reach regions in which explorer probes are present. A study presented that uses 2D code backtrace trajectories representative target points located 1 au Sun....