Spacecraft Propulsion Using Solar Energy Spacecraft with Magnetic Field Light from the Sun Solar Wind Thrust Mirror Solar Sail Thrust production by li

Similar documents
75 unit: mm Fig. Structure of model three-phase stacked transformer cores (a) Alternate-lap joint (b) Step-lap joint 3 4)

PowerPoint Presentation

プラズマ核融合学会誌11月【81‐11】/小特集5

Optical Lenses CCD Camera Laser Sheet Wind Turbine with med Diffuser Pitot Tube PC Fig.1 Experimental facility. Transparent Diffuser Double Pulsed Nd:

Developement of Plastic Collocation Method Extension of Plastic Node Method by Yukio Ueda, Member Masahiko Fujikubo, Member Masahiro Miura, Member Sum

Fig, 1. Waveform of the short-circuit current peculiar to a metal. Fig. 2. Waveform of arc short-circuit current. 398 T. IEE Japan, Vol. 113-B, No. 4,

スペースプラズマ研究会-赤星.ppt

untitled

Study on Application of the cos a Method to Neutron Stress Measurement Toshihiko SASAKI*3 and Yukio HIROSE Department of Materials Science and Enginee

Motivation and Purpose There is no definition about whether seatbelt anchorage should be fixed or not. We tested the same test conditions except for t

4/15 No.

第62巻 第1号 平成24年4月/石こうを用いた木材ペレット

日立金属技報 Vol.34

untitled

空力騒音シミュレータの開発

JFE(和文)No.4-12_下版Gのコピー

The Evaluation on Impact Strength of Structural Elements by Means of Drop Weight Test Elastic Response and Elastic Limit by Hiroshi Maenaka, Member Sh

1..FEM FEM 3. 4.

Table 1. Assumed performance of a water electrol ysis plant. Fig. 1. Structure of a proposed power generation system utilizing waste heat from factori

Study on Throw Accuracy for Baseball Pitching Machine with Roller (Study of Seam of Ball and Roller) Shinobu SAKAI*5, Juhachi ODA, Kengo KAWATA and Yu


Fig. 1 Schematic construction of a PWS vehicle Fig. 2 Main power circuit of an inverter system for two motors drive

mm mm PC PC Epson Endeavor NT mm288 mm 30 mm 3 I II4 1FQR 5 mm II Tab. 1 Characteristics of participants. 2 Fig. 2 Adj

早稲田大学現代政治経済研究所 ダブルトラック オークションの実験研究 宇都伸之早稲田大学上條良夫高知工科大学船木由喜彦早稲田大学 No.J1401 Working Paper Series Institute for Research in Contemporary Political and Ec

: u i = (2) x i Smagorinsky τ ij τ [3] ij u i u j u i u j = 2ν SGS S ij, (3) ν SGS = (C s ) 2 S (4) x i a u i ρ p P T u ν τ ij S c ν SGS S csgs

/ Motor Specifications Direct Motor Drive Ball Screws / Precision Ball Screw type MB / MB MB Precision Ball Screw type MB / MoBo C3 5 5 Features A 5-p

[2] OCR [3], [4] [5] [6] [4], [7] [8], [9] 1 [10] Fig. 1 Current arrangement and size of ruby. 2 Fig. 2 Typography combined with printing

NUMERICAL CALCULATION OF TURBULENT OPEN-CHANNEL FLOWS BY USING A MODIFIED /g-e TURBULENCE MODEL By Iehisa NEZU and Hiroji NAKAGA WA Numerical calculat

258 5) GPS 1 GPS 6) GPS DP 7) 8) 10) GPS GPS ) GPS Global Positioning System

Development of Induction and Exhaust Systems for Third-Era Honda Formula One Engines Induction and exhaust systems determine the amount of air intake

Journal of Geography 116 (6) Configuration of Rapid Digital Mapping System Using Tablet PC and its Application to Obtaining Ground Truth

Microsoft PowerPoint - hoshino_part1.pptx

(1) 2

On the Wireless Beam of Short Electric Waves. (VII) (A New Electric Wave Projector.) By S. UDA, Member (Tohoku Imperial University.) Abstract. A new e

技術研究所 研究所報 No.80

スライド 1

2 ( ) i

Time Variation of Earthquake Volume and Energy-Density with Special Reference to Tohnankai and Mikawa Earthquake Akira IKAMi and Kumizi IIDA Departmen

Fig. 1. Horizontal displacement of the second and third order triangulation points accompanied with the Tottori Earthquake of (after SATO, 1973)

mm mm , ,000 Fig. 1 Locality map of the investigation area NE SW Fi

Development and Field Test of a Portable Camera System for Long Term Observation of Natural Dam Ken AKIYAMA (Tohoku Univ.), Genki YAMAUCHI (Tohoku Uni

K02LE indd

: , , % ,299 9, , % ,

Mott散乱によるParity対称性の破れを検証

1 a b cc b * 1 Helioseismology * * r/r r/r a 1.3 FTD 9 11 Ω B ϕ α B p FTD 2 b Ω * 1 r, θ, ϕ ϕ * 2 *

kut-paper-template.dvi

perature was about 2.5 Ž higher than that of the control irrespective of wind speed. With increasing wind speeds of more than 1m/s, the leaf temperatu

IHIMU Energy-Saving Principle of the IHIMU Semicircular Duct and Its Application to the Flow Field Around Full Scale Ships IHI GHG IHIMU CFD PIV IHI M

* * 2

Corrections of the Results of Airborne Monitoring Surveys by MEXT and Ibaraki Prefecture

untitled

JOURNAL OF THE JAPANESE ASSOCIATION FOR PETROLEUM TECHNOLOGY VOL. 66, NO. 6 (Nov., 2001) (Received August 10, 2001; accepted November 9, 2001) Alterna

Visual Evaluation of Polka-dot Patterns Yoojin LEE and Nobuko NARUSE * Granduate School of Bunka Women's University, and * Faculty of Fashion Science,

07_Shiota.pptx

28 Horizontal angle correction using straight line detection in an equirectangular image

Transcription:

2004.3.28 物理学会シンポジウム 磁気プラズマセイル の可能性と 深宇宙探査への挑戦 宇宙航空研究開発機構 船木一幸

Spacecraft Propulsion Using Solar Energy Spacecraft with Magnetic Field Light from the Sun Solar Wind Thrust Mirror Solar Sail Thrust production by light pressure Magnetic Sail Thrust production by the solar wind dynamic pressure

1.??

1. (MPS) 2. MPS Inflation 3. JAXA/MPS

Original Idea of Magsail Top View Superconducting Coil Solar Wind Streamlines Side View 128km Solar Wind Vehicle System and Payload Support Magnetic Field Lines Proposal by Zubrin (JBIS, 1993) Solar Wind Dynamic Pressure ~ Magnetic Field of nt B-field by superconducting coil of 5mm diameter Current Density 10 10 A/m 2 ( difficult to construct/deploy)

Magsail with Plasma Jet (Magneto Plasma Sail, MPS) Mini-Magnetospheric Plasma Propulsion (M2P2) Proposed by R.M. Winglee, JGR, 2000 Bow Shock Magnetosheath Solar Wind Thrust Solar Wind Plasma Jet Thrust B-Field Lines Original Small B-field Inflated B-field by Plasma Jet Large interaction area -> Large thrust

(MPS) MPS MPS MPS

Comparison of MPS with EP Target of MPS both large T/P and Isp

MPS( ) Winglee MPS Inflation MPS

2. MPS( ) 2.1

~ ~ 2D

~ ~ Shock Front -30Re 30Re Magnetopause -30Re 30Re

D D C = D 2 ( ρu 2 )S ~ ~ C D ~0.95

2. MPS 2.2

2D-MHD Simulation of Magnetic Field Inflation 0.500 using resistive MHD model Axysymmetry θ Background Plasma ρ 0, p 0 :fixed u 0 =0 at r=r out r (polar direction), m Outflow Condition 0.375 0.250 0.125 0.000 Magnetic Flux Density (Dipole Field) 0.000 0.125 0.250 0.375 0.500 r, m at r=r in ρ in, u in, p in, B in : fixed Plasma Injection B-Field Lines r Symmetry r (polar direction), m 0.500 0.375 0.250 0.125 0.000 = 2.434e-03 Initial Plasma Distribution 10 18 /m 3, 3eV 0.000 0.125 0.250 0.375 0.500 r, m T r-θ Calculation Region 0.25 0.50 0.75 1.00 1.25 Pressure, Pa Initial Conditions

5.00 Numerical Result: Plasma Flowfield obtained by resistive MHD code (NIRVANA) t=0.22ms, B in =0.02T (200Gauss) p in =1.3Pa,T in =3eV, sonic inlet shock waves (large T) 5.00 Rm=σµ 0 ur-> (B-field frozen-in) r (polar direction), m 3.75 2.50 1.25 Background Plasma 10-4 Pa 3eV r (polar direction), m 3.75 2.50 1.25 5m 0.00 Acceleration r, m Deceleration 0.00 0.00 1.25 2.50 3.75 5.00 r, m 2500 5000 7500 100001250015000 Velocity, m/s Velocity Distribution 500 1000 1500 2000 25 Rm Magnetic Reynold s Number Distribution

Numerical Result: Magnetic Field Inflation by Plasma Injection B in =0.02T (200Gauss), p in =1.3Pa,T in =3eV, sonic inlet 5.00 5.00 r (polar direction), m 3.75 2.50 1.25 r (polar direction), m 3.75 2.50 1.25 0.00 0.00 1.25 2.50 3.75 5.00 r, m 0.00 0.00 1.25 2.50 3.75 5.00 r, m -5-4 -3-2 B-field, T -5-4 -3 B-field, T Magnetic Flux Density (without Plasma Injection, t=0) Magnetic Flux Density (with Plasma Injection, t=2.2e-04 s)

Summary of Numerical Result : Inflated Magnetic Field point of plasma injection Rm-> B-field frozen-in Magnetic Flux Tube MPS with plasma injection t=0.22ms t=0 without plasma Magnetic Dipole Magnetic Flux Density Model of Magnetic Field Inflation B-field inflation is also confirmed in the case of resistive MHD model. However, currently, only transient results are obtained.

3.

Research Topics remains

H16 H17 MPS H18