Published December 17, 2002 | Version v1
Journal article

Application of flyer acceleration by pulsed ion beam ablation to deep space thruster

  • 1. Department of Electrical Engineering, Nagaoka University of Technology, 1603-1 Kamitomioka, Nagaoka 940-2188 (Japan)
  • 2. Department of Electrical Engineering, Kagoshima National College of Technology, Hayato-cho, Kagoshima 899-5193 (Japan)
  • 3. Extreme Energy-Density Research Institute, Nagaoka University of Technology, 1603-1 Kamitomioka, Nagaoka 940-2188 (Japan)

Description

Flyer acceleration by ablation plasma pressure produced by irradiation of intense pulsed ion beam has been studied. Acceleration process including expansion of ablation plasma was simulated based on fluid model. In experiments, flyer velocities of 5.6 km/s and ablation plasma pressure of 15 GPa were demonstrated and these results agree well with numerical simulation. Finally, applicability of ablation propulsion was discussed. Specific impulse of 7000∼8000 seconds and time averaged thrust of up to 5000∼6000N can be expected

Additional details

Identifiers

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
650
Journal Issue
1
Journal Page Range
p. 441-444
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
14. international conference on high-power particle beams
Acronym
BEAMS 2002
Dates
23-28 Jun 2002
Place
Albuquerque, NM (United States)

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
36064937
Subject category
S75: CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY; S43: PARTICLE ACCELERATORS; S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
ABLATION; ACCELERATION; ION BEAMS; IRRADIATION; PLASMA; PLASMA EXPANSION; PLASMA HEATING; PLASMA PRESSURE; PLASMA SIMULATION; PRESSURE RANGE GIGA PA; PROPULSION; SPACE; THRUSTERS; USES
Descriptors DEC
BEAMS; EXPANSION; HEATING; PRESSURE RANGE; SIMULATION

Optional Information

Notes
(c) 2002 American Institute of Physics