Solar and astrophysical magnetohydrodynamic flows:
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| Format: | Book |
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| Language: | English |
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Dordrecht [u.a.]
Kluwer
1996
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| Series: | NATO: [Nato ASI series / C]
481 |
| Subjects: | |
| Online Access: | Inhaltsverzeichnis |
| Physical Description: | XL, 742 S. Ill., graph. Darst. |
| ISBN: | 079234054X |
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| 245 | 1 | 0 | |a Solar and astrophysical magnetohydrodynamic flows |c ed. by Kanaris C. Tsinganos |
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| 650 | 4 | |a Théorie de la dynamo | |
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SOLAR AND ASTROPHYSICAL MAGNETOHYDRODYNAMIC FLOWS EDITED BY KANARIS C.
TSINGANOS DEPARTMENT OF PHYSICS, UNIVERSITY OF CRETE, HERAKLION, GREECE
KLUWER ACADEMIC PUBLISHERS DORDRECHT / BOSTON / LONDON PUBLISHED IN
COOPERATION WITH NATO SCIENTIFIC AFFAIRS DIVISION TABLE OF CONTENTS
PREFACE XXIII PARTICIPANTS XXIX PART I: SOLAR MAGNETOHYDRODYNAMIC FLOWS
1. QUESTIONS AND CONJECTURES ON THE ORIGIN OF STELLAR AND GALACTIC
MAGNETIC FIELDS EUGENE PARKER 1 1 INTRODUCTION 1 2 THE DIFFICULTY 5 3
THE SUN 6 4 THE GALAXY 8 5 REFERENCES 13 2. MAGNETIC FLUX TUBES AND THE
SOLAR DYNAMO MANFRED SCHIISSLER 17 1 THE DYNAMO PROBLEM 18 2 STORAGE OF
MAGNETIC FLUX 18 2.1 THE BUOYANCY DILEMMA 18 2.2 FLUX TUBES IN
MECHANICAL EQUILIBRIUM 20 3 INSTABILITY AND ERUPTION 23 3.1 UNDULATORY
INSTABILITY 23 3.2 NONLINEAR EVOLUTION OF THE INSTABILITY 25 4
GENERATION OF SUPER-EQUIPARTITION FIELDS 30 4.1 STRETCHING BY
DIFFERENTIAL ROTATION 30 4.2 'EXPLOSION' OF MAGNETIC FLUX TUBES 32 5
STRONG FIELDS AND DYNAMO THEORY 35 6 CONCLUSIONS 36 VI 7 REFERENCES 37
3. SIPHON FLOWS IN SOLAR MAGNETIC FLUX TUBES AND SUNSPOTS JOHN H. THOMAS
39 1 INTRODUCTION 39 2 STEADY SIPHON FLOWS IN ISOLATED MAGNETIC FLUX
TUBES 40 2.1 BASIC EQUATIONS 40 2.2 ISOTHERMAL SIPHON FLOWS 42 2.3 MORE
REALISTIC SIPHON FLOWS 45 3 TUBE SHOCKS IN SUPERCRITICAL SIPHON FLOWS 48
4 SIPHON FLOWS IN INTENSE PHOTOSPHERIC FLUX TUBES 53 5 SIPHON FLOWS AND
THE EVERSHED EFFECT IN SUNSPOTS 53 6 REFERENCES 59 4. MHD WAVES IN
MAGNETIC FLUX TUBES MARCEL GOOSSENS AND MICHAEL RUDERMAN 61 1
INTRODUCTION 61 2 ASYMPTOTIC STATE OF RESONANT ALFVEN WAVES 65 3
RESONANT ALFVEN WAVES IN LINEAR IDEAL MHD 68 4 RESISTIVE MHD EQUATIONS
FOR RESONANT ALFVEN WAVES 71 5 RESISTIVE MHD SOLUTIONS FOR RESONANT
ALFVEN WAVES CLOSE TO THE IDEAL RESONANCE POSITION 73 6 CONCLUSIONS 80 7
REFERENCES 81 5. THE DYNAMIC SOLAR CORONA IN X-RAYS WITH YOHKOH SAKU
TSUNETA 85 1 INTRODUCTION 85 2 THE X-RAY CORONA 87 2.1 THE OVERALL X-RAY
CORONA 87 2.2 THE ACTIVE REGION CORONA 89 3 TRANSIENT AND STEADY LOOPS
IN THE SOLAR CORONA .90 3.1 TRANSIENT LOOPS IN THE SOLAR CORONA 90 3.2
CAN TRANSIENT BRIGHTENINGS EXPLAIN CORONAL HEATING ? 91 4 TEMPERATURE
STRUCTURE OF ACTIVE REGIONS 94 VU 4.1 CUSP RECONNECTION AND LOOP-LOOP
RECONNECTION 95 4.2 TEMPERATURE STRUCTURE AND TIME VARIABILITY 95 5 THE
SCALING LAWS 97 5.1 SCALING LAW OBTAINED WITH YOHKOH 99 5.2 TEMPERATURE
DISTRIBUTION ALONG LOOPS 100 5.3 THE ENERGY SCALING LAW 101 6 SOLAR
FLARES AND MAGNETIC RECONNECTION 102 6.1 PHYSICAL PARAMETERS OF THE
RECONNECTION SITE 102 6.2 HOW IS THE NEUTRAL SHEET STRUCTURE CREATED ?
103 7 MAGNETIC RECONNECTION AND TRANSIENT PHENOMENA 104 7.1 TIME SCALE
OF RECONNECTION 104 7.2 WHY DOES RECONNECTION OCCUR IN THE SOLAR CORONA
? 106 8 FROM YOHKOH TO SOLAR-B 106 9 REFERENCES 107 6. THE SPONTANEOUS
FORMATION OF CURRENT-SHEETS IN ASTROPHYSICAL MAGNETIC FIELDS BOON CHYE
LOW 109 1 INTRODUCTION 109 2 THE PARKER PROBLEM 110 3 CURRENT-SHEET
FORMATION BY FLUX EXPULSION 115 3.1 A TWO-STEP EVOLUTIONARY PROCESS 116
3.2 CURRENT-SHEETS AT MAGNETIC NULL POINTS 117 3.3 CURRENT-SHEET
FORMATION WITHOUT A NULL POINT 121 3.4 CURRENT-SHEET FORMATION IN A
SHEARED MAGNETIC FIELD 123 3.5 INFLUENCE OF PRESSURE AND GRAVITY 128 4
DISCUSSION AND CONCLUSION 129 5 REFERENCES 131 7. MAGNETOHYDRODYNAMIC
PROCESSES IN THE SOLAR CORONA : FLARES, CORONAL MASS EJECTIONS AND
MAGNETIC HELICITY BOON CHYE LOW 133 1 INTRODUCTION 133 2 THE SOLAR
CORONA 134 3 HELMET-STREAMERS, MASS EJECTIONS AND THE SOLAR WIND 136 3.1
LARGE-SCALE EQUILIBRIUM 136 VLLL 3.2 INTERNAL STRUCTURES OF THE CORONAL
HELMET 138 3.3 DISRUPTIONS INTO CORONAL MASS EJECTIONS 140 4 MAGNETIC
FLUX ROPES AND MAGNETIC HELICITY 143 5 SUMMARY AND CONCLUSION 146 6
REFERENCES 148 8. RECONNECTION OF MAGNETIC LINES OF FORCE ERIC R. PRIEST
151 1 INTRODUCTION 151 2 SWEET-PARKER RECONNECTION 153 3 ALMOST-UNIFORM
POTENTIAL RECONNECTION 158 4 ALMOST-UNIFORM NON-POTENTIAL RECONNECTION
164 5 NON-UNIFORM RECONNECTION 165 5.1 POTENTIAL RECONNECTION 165 5.2
NON-POTENTIAL RECONNECTION 166 6 CONCLUSIONS 168 7 REFERENCES 169 9. NEW
DEVELOPMENTS IN MAGNETIC RECONNECTION THEORY ERIC R. PRIEST 171 1
INTRODUCTION 172 2 TWO-DIMENSIONAL MAGNETIC RECONNECTION THEORY 174 2.1
LINEAR RECONNECTION 174 2.2 X-POINT COLLAPSE 177 3 THREE-DIMENSIONAL
RECONNECTION 179 3.1 RECONNECTION AT NULL POINTS 180 4 RECONNECTION
WITHOUT NULL POINTS 184 5 RECONNECTION IN SOLAR CORONAL HEATING 190 5.1
CONVERGING FLUX MODEL 192 5.2 APPLICATION TO SPECIFIC BRIGHT POINTS 192
6 CONCLUSIONS 193 7 REFERENCES 193 IX 10. HYDRODYNAMIC AND
MAGNETOHYDRODYNAMIC TURBULENCE ANNICK POUQUET 195 1 INTRODUCTION 195 2
THE ONE-DIMENSIONAL CASE 196 2.1 A FLUID MODEL 196 2.2 A NUMERICAL MODEL
199 2.3 THE HADA EQUATION AND THE ASYMMETRIC STABILITY OF PROTO-STELLAR
JETS 201 3 DIAGNOSTICS 202 3.1 STRUCTURE FUNCTIONS 202 3.2 THE
SHE-LEVEQUE MODEL 203 4 THE TWO-DIMENSIONAL CASE 205 4.1 ARE NONLINEAR
INTERACTIONS SELF-DEFEATING IN MHD ? 205 4.2 DOES RECONNECTION OCCUR AT
A FINITE RATE FOR R * * OO ? 206 4.3 A PLAUSIBLE MODEL FOR HEATING THE
SOLAR CORONA 207 5 THE THREE-DIMENSIONAL CASE 208 5.1 THE BETCHOV
RELATION 208 5.2 THE STRUCTURING OF VORTICITY INTO FILAMENTS 208 5.3
TRANSPORT COEFFICIENTS AND THE EXCESS OF MAGNETIC ENERGY IN THE SMALL
SCALES 209 5.4 TRANSPORT COEFFICIENTS AND THE DYNAMO PROBLEM 209 5.5 THE
DYNAMICAL DEVELOPMENT OF SINGULARITIES 210 6 TURBULENCE IN THE
INTERSTELLAR MEDIUM 211 6.1 EVIDENCE OF TURBULENCE THROUGH LINE WIDTHS
211 6.2 A MODEL OF THE ISM AT THE KILOPARSEC SCALE 211 6.3 AN EFFECTIVE
THERMODYNAMICAL LAW 212 6.4 THE MHD CASE 213 7 CONCLUSION 213 8
REFERENCES 214 11. NUMERICAL SIMULATIONS OF SOLAR AND ASTROPHYSICAL MHD
FLOWS KAZUNARI SHIBATA 217 1 INTRODUCTION 217 2 DIFFICULTIES IN
SIMULATING MHD PHENOMENA IN THE SOLAR ATMOSPHERE AND ASTROPHYSICAL GAS
LAYERS 219 X 3 JETS - PLASMA ACCELERATION DUE TO NONLINEAR MHD WAVES AND
CENTRIFUGAL FORCE 221 3.1 SOLAR JETS: SPICULES AND SURGES 221 3.1.1 SLOW
SHOCK ACCELERATION 221 3.1.2 NONLINEAR ALFVEN WAVE (OR MAGNETIC TWIST)
ACCELERATION . 224 3.2 ASTROPHYSICAL JETS EJECTED FROM ACCRETION
DISKS 225 3.2.1 NONSTEADY MHD JETS FROM THIN DISKS - THE SWEEPING
MAGNETIC TWIST MECHANISM 225 3.2.2 RELATION TO THE MAGNETO-ROTATIONAL
(BALBUS-HAWLEY) INSTABILITY " 227 3.2.3 NONSTEADY MHD JETS FROM THICK
DISKS 228 3.2.4 RELATION BETWEEN NONSTEADY AND STEADY JETS 229 3.2.5
THREE DIMENSIONAL PROPAGATION OF MHD JETS 231 4 LOOPS - NONLINEAR
EVOLUTION OF THE PARKER INSTABILITY 232 4.1 MAGNETIC LOOPS IN GALACTIC
AND ACCRETION DISKS 232 4.1.1 TYPICAL NONLINEAR EVOLUTION OF THE PARKER
INSTABILITY: THE MOST UNSTABLE MODE 232 4.1.2 CONDITION OF SHOCK WAVE
FORMATION AND NONLINEAR OSCILLATION 234 4.1.3 EFFECT OF CORONA (HALO)
235 4.1.4 EFFECT OF ROTATION AND SHEARING MOTION 236 4.2 EMERGING SOLAR
MAGNETIC LOOPS 238 4.2.1 SELF-SIMILAR EXPANSION OF MAGNETIC LOOPS 238
4.2.2 THREE DIMENSIONAL EFFECT: COUPLING WITH THE INTERCHANGE MODES 241
4.2.3 EMERGENCE OF TWISTED FLUX TUBE 242 5 FLARES - MAGNETIC
RECONNECTION 242 5.1 SOLAR COMPACT FLARES AND X-RAY JETS 242 5.2
PROTOSTELLAR MAGNETOSPHERE 244 6 FUTURE DIRECTIONS 244 7 REFERENCES 245
12. FURTHER THOUGHTS ON THE SOLAR CORONA AS A MINIMUM ENERGY SYSTEM PAUL
CHARBONNEAU AND ART J. HUNDHANSEN 249 1 INTRODUCTION 249 2 AN
ILLUSTRATIVE MODEL 253 XI 2.1 OVERVIEW OF MODEL CONSTRUCTION 253 2.2 THE
TOTAL ENERGY 254 2.3 SAMPLE RESULTS 256 3 IMPLICATIONS 259 3.1 CORONAL
MASS EJECTIONS 259 3.2 NUMERICAL SIMULATIONS 260 4 APPLICATIONS 261 5
REFERENCES 263 13. ULYSSES OBSERVATIONS OF THE SOLAR WIND OUT OF THE
ECLIPTIC PLANE W.C. FELDMAN, J.L. PHILLIPS, B.L. BARRACLOUGH AND CM.
HAMMOND 265 1 INTRODUCTION 265 2 OBSERVATIONS 267 2.1 OVERVIEW OF SOLAR
WIND FLOW STRUCTURE 267 2.2 COROTATING INTERACTION REGIONS (CIR S) 269
2.3 CORONAL MASS EJECTIONS (CME S) 271 2.4 FLOW STRUCTURE AT HIGH
LATITUDES 274 2.5 HELIUM ABUNDANCE 281 2.6 INTERNAL STATE OF THE
HIGH-LATITUDE WIND; PROTONS 285 2.7 INTERNAL STATE OF THE HIGH-LATITUDE
WIND; ELECTRONS 288 3 SUMMARY AND DISCUSSION 290 4 REFERENCES 297 14.
STELLAR WINDS KEITH B. MACGREGOR 301 1 INTRODUCTION 301 2 THE WINDS FROM
THE SUN AND SOLAR-TYPE STARS 303 2.1 THE SOLAR WIND: SOME PRELIMINARY
PHYSICAL CONSIDERATIONS 303 2.2 WINDS FROM SOLAR-TYPE STARS:
OBSERVATIONAL EVIDENCE 304 3 MAGNETIC MODIFICATIONS TO THERMALLY DRIVEN
FLOW 311 3.1 MAGNETIC DEFINITION OF FLOW GEOMETRY 311 3.2
MAGNETIC/CENTRIFUGAL ACCELERATION 315 3.3 ALFVEN WAVE-DRIVEN WINDS 322 4
DISCUSSION: EXTENSION TO WINDS FROM NON-SOLAR-TYPE STARS 327 4.1 WINDS
FROM EARLY-TYPE STARS 327 XLL 4.2 THE FORCE OF RADIATION IN SPECTRAL
LINES 328 4.3 MAGNETIC MODIFICATIONS TO RADIATIVELY DRIVEN FLOW 329 5
REFERENCES 334 15. SOME IMPLICATIONS OF SOLAR AND STELLAR ACTIVITY
EUGENE PARKER 337 1 SUPRATHEMAL ACTIVITY AND VARIABILITY 337 2 ENERGY
SUPPLY 341 3 THE X-RAY CORONA 342 4 DISSIPATION OF MAGNETIC ENERGY 344 5
ENERGY INPUT AND RECONNECTION RATES 346 6 OBSERVATIONAL TESTS 349 7
REFERENCES 351 XLLL PART II: ASTROPHYSICAL MAGNETOHYDRODYNAMIC FLOWS 16.
HUBBLE SPACE TELESCOPE OBSERVATIONS OF GALACTIC AND EXTRAGALACTIC JETS
JOHN A. BIRETTA 357 1 INTRODUCTION 357 2 GALACTIC JETS 358 2.1 JETS FROM
YOUNG STELLAR OBJECTS 358 2.2 JETS FROM OLDER, SYMBIOTIC STARS 363 3
EXTRAGALACTIC JETS 365 3.1 THE JET IN M87 367 3.2 THE JET IN 3C273 373
3.3 OPTICAL SYNCHROTRON JETS DISCOVERED BY HST 375 3.4 SUMMARY OF HST
OBSERVATIONS OF EXTRAGALACTIC JETS 376 4 PROBLEMS POSED BY OBSERVATIONS
OF EXTRAGALACTIC JETS 377 5 FUTURE PROSPECTS 379 6 REFERENCES 380 17.
EXACT MHD SOLUTIONS FOR SELF-SIMILAR OUTFLOWS EDOARDO TRUSSONI,
CHRISTOPHE SAUTY AND KANARIS TSINGANOS 38 3 1 INTRODUCTION 384 2 MHD
EQUATIONS FOR AXISYMMETRIC CONFIGURATIONS 386 2.1 POLOIDAL COMPONENTS
387 2.2 TOROIDAL COMPONENTS 387 2.3 ALFVEN SINGULARITY 388 3 SCALING
LAWS FOR SELF-SIMILAR SOLUTIONS 388 4 EQUATIONS OF THE WIND 391 5
SOLUTIONS WITH PRESCRIBED PRESSURE DISTRIBUTION 392 5.1 ENERGETICS OF
THE OUTFLOW 393 5.2 ASYMPTOTIC STRUCTURE OF THE OUTFLOW 393 5.3
OSCILLATIONS IN THE WIDTH OF COLLIMATED OUTFLOWS 395 5.4 ALFVEN AND
X-TYPE SINGULARITY 396 5.5 NUMERICAL RESULTS 398 6 SOLUTIONS WITH
PRESCRIBED STREAMLINES 400 6.1 PRESCRIPTION OF THE STREAMLINES 402 XIV
6.2 ASYMPTOTIC STRUCTURE OF THE OUTFLOW 402 6.3 NUMERICAL SOLUTIONS 404
7 CONCLUDING REMARKS 408 8 REFERENCES 410 18. NUMERICAL SIMULATION OF
PLASMA FLOW IN THE MAGNETOSPHERE OF AN AXISYMMETRIC ROTATOR SERGEI V.
BOGOVALOV 411 1 INTRODUCTION 411 2 EQUATIONS OF STATIONARY MHD FLOW 412
3 BOUNDARY CONDITIONS AND CRITICAL SURFACES FOR MIXED-TYPE EQUATIONS .
.413 4 TIME DEPENDENT MODEL 418 5 STRUCTURE OF THE STATIONARY SOLUTIONS
419 6 CENTRIFUGAL ACCELERATION OF PLASMA 421 7 REFERENCES 423 19.
CRITICAL POINTS AND SEPARATRIX CHARACTERISTICS IN SOLAR AND
ASTROPHYSICAL MHD FLOWS KANANS TSINGANOS, CHRISTOPHE SAUTY, GEORGE
SURLANTZIS, EDOARDO TRUSSONI AND JOHN CONTOPOULOS 427 1 INTRODUCTION 428
2 CRITICAL POINTS IN SYMMETRIC MHD FLOWS 430 2.1 BERNOULLI K TRANSFIELD
EQUATIONS IN SYMMETRIC POLYTROPIC FLOWS . .430 2.2 CHARACTERISTICS OF
SYMMETRIC MHD FLOWS 432 2.3 SEPARATRIX CHARACTERISTICS OF BERNOULLI AND
TRANSFIELD EQUATIONS IN POLYTROPIC FLOWS 432 2.4 CRITICAL POINTS IN
SELF-SIMILAR FLOWS 440 3 EXAMPLES OF CRITICAL POINTS AND SEPARATRIX
CHARACTERISTICS IN SYMMETRIC AND SELF-SIMILAR POLYTROPIC MHD FLOWS 443
3.1 VERTICALLY SELF-SIMILAR FLOWS IN LOOPS EMBEDDED IN A PLANAR
ATMOSPHERE 443 3.2 RADIALLY SELF-SIMILAR POLYTROPIC DISC WINDS AND JETS
445 4 EXAMPLES OF CRITICAL POINTS AND SEPARATRIX CHARACTERISTICS IN
AXISYMMETRIC AND MERIDIONALLY-SELF-SIMILAR NONPOLYTROPIC MHD FLOWS 450 5
SUMMARY 456 6 REFERENCES 458 XV 20. COLLIMATION OF MHD OUTFLOWS JEAN
HEYVAERTS AND COLIN A. NORMAN 459 1 INTRODUCTION 459 2 BASICS OF
AXISYMMETRIC STATIONARY MHD FLOWS 460 2.1 THE FOCUSING HOOP STRESS 460
2.2 THE AXISYMMETRIC STATIONARY WIND MODEL 460 2.3 SURFACE FUNCTIONS 461
2.4 ALFVEN RADIUS AND DENSITY 463 3 FIELD-ALIGNED FLOWS 464 3.1 THE
BERNOULLI INTEGRAL 464 3.2 CRITICAL POINTS AND CRITICALITY RELATIONS 465
4 THE TRANSFIELD EQUATION 466 4.1 FORCE BALANCE PERPENDICULAR TO FIELD
LINES 466 4.2 ALFVEN REGULARITY CONDITION 467 5 GENERAL RESULTS ON THE
ASYMPTOTIC BEHAVIOUR OF POLYTROPIC ROTATING MHD WINDS 469 5.1 ROTATING
POLYTROPIC MHD WINDS DO NOT ASYMPTOTICALLY BEND TOWARDS THE EQUATOR 469
5.2 WINDS WHICH CARRY NO POYNTING FLUX AT INFINITY ALSO CARRY NO
POLOIDAL CURRENT AND FOCUS PARABOLICALLY 470 5.3 MAGNETIC SURFACES WHICH
DIVERGE OFF AXIS ENCLOSE NO POLOIDAL CURRENT BETWEEN THEM AT INFINITY
471 5.4 WINDS WHICH CARRY NON VANISHING POYNTING FLUX AT INFINITY
CONTAIN A CYLINDRICALLY COLLIMATED CORE 473 6 REFERENCES 473 21. THE
PARKER INSTABILITY IN THE INTERSTELLAR MEDIUM TELEMACHOS CH. MOUSCHOVIAS
475 1 INTRODUCTION 475 2 BASIC EQUATIONS AND PHYSICS OF THE INSTABILITY
476 2.1 COSMIC RAYS AS A FLUID 478 2.2 MAGNETIC RAYLEIGH-TAYLOR (OR
PARKER) INSTABILITY 479 2.2.1 THE ZEROTH-ORDER STATE 480 2.2.2
TWO-DIMENSIONAL STABILITY ANALYSIS 480 2.2.3 INSTABILITY IN THREE
DIMENSIONS 484 3 FINAL EQUILIBRIUM STATES 485 3.1 WHY FINAL STATES EXIST
486 XVI 3.2 SELF-CONSISTENT FORMULATION OF THE PROBLEM 486 3.3
DETERMINATION OF EQUILIBRIUM STATES 489 4 ENERGY INTEGRAL FOR ISOTHERMAL
PLASMA 490 5 NONLINEAR EVOLUTION 492 5.1 SUMMARY OF PAST WORK 492 5.2
NEW NUMERICAL SIMULATIONS 494 5.2.1 NONLINEAR EVOLUTION OF THE ODD
LINEAR MODES 494 5.2.2 NONLINEAR EVOLUTION OF THE EVEN LINEAR MODES 495
5.2.3 EFFECT OF COSMIC RAYS ON THE INSTABILITY AND VICE VERSA 501 6
SUMMARY 502 7 REFERENCES 503 22. MULTIFLUID MAGNETOHYDRODYNAMICS AND
STAR FORMATION TELEMACHOS CH. MOUSCHOVIAS 505 1 INTRODUCTION - A MODERN
THEORY OF STAR FORMATION 505 2 FIVE-FLUID MHD DESCRIPTION OF PROTOSTAR
FORMATION 508 2.1 PHYSICAL ORIGIN OF THE FIVE-FLUID EQUATIONS 508 2.2
REDUCTION OF THE FIVE-FLUID EQUATIONS: FLUX-FREEZING IN THE PLASMA 513
2.3 GRAIN MOTION AND ATTACHMENT TO THE MAGNETIC FIELD 514 3 TWO-FLUID
DESCRIPTION OF PROTOSTAR FORMATION 515 3.1 BASIC EQUATIONS 515 3.2
AMBIPOLAR DIFFUSION: GENERAL CONSIDERATIONS AND TIMESCALES 516 3.3
MAGNETIC BRAKING 518 4 RESULTS OF TWO-FLUID DESCRIPTION OF PROTOSTAR
FORMATION 519 4.1 AMBIPOLAR DIFFUSION IN NONROTATING MODELS 520 4.2
ROTATING MODELS: AMBIPOLAR DIFFUSION AND MAGNETIC BRAKING 523 5
PROTOSTAR FORMATION IN THE FOUR-FLUID APPROXIMATION 527 5.1 MAIN EFFECTS
OF GRAINS 527 5.2 COMPARISON WITH OBSERVATIONS: THE BARNARD I CLOUD 531
5.3 EFFECT OF ULTRAVIOLET RADIATION 531 6 HYDROMAGNETIC WAVES,
LINEWIDTHS, AMBIPOLAR DIFFUSION, AND STAR FORMATION 532 7 CONCLUSION 534
8 APPENDIX 536 9 REFERENCES 536 XV11 23. JETS ASSOCIATED WITH YOUNG
STARS TOM P. RAY .'. 539 1 HISTORICAL INTRODUCTION 539 1.1 HERBIG-HARO
OBJECTS 539 1.2 THE DISCOVERY OF JETS FROM YOUNG STARS 540 2 JET
PROPERTIES 542 2.1 SPECTROSCOPY 542 2.2 MORPHOLOGY 544 2.3 PHYSICAL
PARAMETERS 544 2.4 SOURCES OF YSO JETS 547 3 THE PROPAGATION OF YSO JETS
549 3.1 WHAT IS THE ORIGIN OF THE KNOTS ? 549 3.2 BOW SHOCKS 550 4 THE
VIEW FROM SPACE AND AT NON-OPTICAL WAVELENGTHS 552 4.1 HST IMAGING 552
4.2 OBSERVING YSO JETS AT NON-OPTICAL WAVELENGTHS 555 5 THE WIDER
PERSPECTIVE 558 5.1 THE CONNECTION BETWEEN YSO JETS AND MOLECULAR
OUTFLOWS 558 5.2 THE DISC-JET CONNECTION: A CASE STUDY 561 6 REFERENCES
563 24. MOLECULAR OUTFLOWS FROM PROTOSTARS R.N. HENRIKSEN 567 1
INTRODUCTION 567 2 PERTINENT THEORETICAL QUESTIONS 567 2.1 WHAT IS THE
ENERGY AND MOMENTUM SOURCE FOR THE OUTFLOW ? 567 2.2 HOW ARE THESE FLOWS
COLLIMATED AND WHERE ? 568 2.3 HOW MANY 'INDEPENDENT' PARTS OF THE
MACHINE ARE THERE ? 568 2.4 WHAT KINDS OF TIME DEPENDENCE ARE THERE ?
569 2.5 WHAT DETERMINES THE CHARACTERISTIC SCALES OF THE OUTFLOWS ? 569
2.6 DOES THE PHENOMENON OCCUR ALSO IN A PRE-PROTOSTAR PHASE ? 570 2.7
HOW CONTINGENT OR UNIVERSAL IS THE PHENOMENON ? 570 2.8 WHAT ARE THE
'NEIGHBOURHOOD' MAGNETIC AND VELOCITY FIELDS ? 571 2.9 ARE THERE
DIFFERENCES BETWEEN THE MAGNETIC AND ROTATION AXES ? 571 3 GENERAL
CONSIDERATIONS 571 4 MODELS; CLASSIFICATION AND CRITIQUE 576 XV111 4.1
WIND DRIVEN MODELS 576 4.2 ENTRAINED OUTFLOW 577 4.3 OUTFLOW DRIVEN BY
WANDERING AND/OR INTERMITTENT JETS 577 4.4 MAGNETIZED DISC DRIVEN
OUTFLOW 578 4.5 BOUNDARY LAYER MODELS 580 4.6 HEATED QUADRUPOLAR
ADVECTION MODELS 581 5 REFERENCES 582 25. JETS AND MHD FLOWS ASSOCIATED
WITH SYMBIOTIC STARS MENAS KAFATOS 585 1 INTRODUCTION 586 2 SYMBIOTIC
STAR SYSTEM COMPONENTS 588 3 OVERALL PROPERTIES OF SYMBIOTICS .' 590 4 R
AQUARII 594 5 CH CYGNI 599 6 MHD FLOWS IN R AQUARII 600 7 REFERENCES 603
26. PHENOMENOLOGY AND MODELLING OF LARGE-SCALE JETS ATTILIO FERRARI,
SILVANO MASSAGLIA, GIANLUIGI BODO AND PAOLA ROSSI 607 1 HISTORICAL
INTRODUCTION 607 2 OBSERVATIONS OF COLLIMATED OUTFLOWS 610 2.1 RADIO
DATA 610 2.2 OPTICAL AND X-RAY DATA 611 2.3 PHYSICAL PARAMETERS 612 2.4
LUMINOSITY - LINEAR SIZE DIAGRAM 614 2.5 UNIFIED MODELS 614 3 PHYSICS OF
COLLIMATED OUTFLOWS 615 3.1 RELATIVISTIC PLASMAS AND MAGNETIC FIELDS 616
3.2 AGE, EXPANSION SPEED AND SPECTRAL BREAK 617 3.3 THE MINIMUM ENERGY
HYPOTHESIS 617 4 PARSEC-SCALE JETS 618 4.1 ACCRETION DISKS 618 4.2
DYNAMICS OF EQUILIBRIUM JETS 619 4.3 RELATIVISTIC JETS 620 4.4
COLLIMATION 621 XIX 4.5 MINI-JETS AS CHOCKED JETS 621 4.6 FREE JETS 621
4.7 MAGNETOHYDRODYNAMICAL AND CENTRIFUGAL MODELS 621 4.8 DIFFICULTIES
AND IMPROVEMENTS 622 5 LARGE-SCALE JETS, MORPHOLOGIES, RADIATION 622 5.1
FLUID INSTABILITIES: LINEAR ANALYSIS 622 5.1.1 KELVIN-HELMHOLTZ
INSTABILITY 623 5.1.2 FILAMENTATION INSTABILITY 624 5.1.3 RESISTIVE
INSTABILITIES, ETC 624 5.2 NONLINEAR EVOLUTION OF HYDRODYNAMIC
INSTABILITIES 624 5.3 SHOCKS 626 5.4 NONLINEAR MHD INSTABILITIES 628 5.5
INSTABILITIES AND RADIATION 628 6 JET TERMINATION ' 629 6.1 HOT SPOTS
632 6.2 COCOONS 632 6.3 FILAMENTS 634 6.4 NUMERICAL SIMULATIONS OF JET'S
HEAD EVOLUTION 635 6.4.1 DYNAMICS OF THE JET'S HEAD 636 6.4.2 DYNAMICS
OF THE COCOON 638 7 REFERENCES 640 27. MHD ACCRETION-EJECTION FLOWS IN
ACTIVE GALACTIC NUCLEI GUY PELLETIER, J. FERREIRA, G. HENRI AND A.
MARCOWITH 643 1 INTRODUCTION 643 2 THE MHD ENGINE 643 2.1 ANGULAR
MOMENTUM TRANSFER 645 2.2 DIFFUSION 645 2.3 CURRENT PROFILE 646 2.4
CROSSING THE SLOW MAGNETOSONIC SURFACE 647 3 MOTION AND CONFINEMENT
COUPLED 648 3.1 CROSSING THE ALFVEN SURFACE 649 3.2 GLOBAL ENERGY BUDGET
649 3.3 TURBULENT HEATING 650 4 THE ISSUE OF THE TURBULENT TRANSPORT 651
5 A MAGNETIC CAULDRON FOR AGNS AND MICROQUASARS 651 XX 5.1 WHY AN
ELECTRON POSITRON COMPONENT ? 652 5.2 HEATING AND BOOSTING THE PAIR
PLASMA 653 5.3 THE PROTON BACKSTREAM INSTABILITY 654 5.4 TURBULENT
CASCADE IN THE RELATIVISTIC PLASMA 655 6 SYNTHESIS 656 7 REFERENCES 657
28. INTERACTION OF TURBULENT ACCRETION DISKS WITH EMBEDDED MAGNETIC
FIELDS JEAN F. HEYVAERTS, ANN BARDOU AND ERIC R. PRIEST 659 1 TURBULENCE
AND ACCRETION 659 2 WHAT DETERMINES THE LEVEL OF TURBULENCE ? 660 2.1
SELF-CONSISTENT TURBULENCE IN GENERAL ' 661 2.2 SELF-CONSISTENT
KOLMOGOROFF TURBULENCE 661 3 TURBULENCE FROM THE MAGNETIC SHEARING
INSTABILITY 664 3.1 FULLY DEVELOPED MAGNETIC SHEARING INSTABILITY 664
3.2 ACCOUNTING FOR TURBULENCE ANISOTROPY 664 3.3 INHIBITION OF THE
MAGNETIC SHEARING INSTABILITY AND CONSEQUENCES . 666 4 MAGNETIC FIELD
DRAGGING BY TURBULENT ACCRETION DISKS 666 5 INTERACTION BETWEEN A THIN
TURBULENT ACCRETION DISK AND THE MAGNETIC FIELD OF THE ACCRETING STAR
668 5.1 FIELD REJECTION BY THE DISK: PHYSICAL MECHANISM 668 5.2 FIELD
INFLATION: A MORE FORMAL DERIVATION 669 6 REFERENCES 671 29. MAGNETIC
RECONNECTION IN ACCRETION DISC CORONAE HARALD LESCH 673 1 INTRODUCTION
673 2 MAGNETIC RECONNECTION AND PARTICLE ACCELERATION 675 3
OBSERVATIONAL CONSEQUENCES OF UNSTABLE RELATIVISTIC ELECTRON BEAMS 678 4
COHERENT EMISSION OF RELATIVISTIC ELECTRON BEAMS 679 5 DISCUSSION 680 6
REFERENCES 681 XXI 30. RELATIVISTIC OUTFLOWS IN THE GALAXY /. FELIX
MIRABEL AND L.F. RODRIGUEZ 683 1 INTRODUCTION 683 2 GRS 1915+105 683 2.1
SUPERLUMINAL MOTIONS IN GRS 1915+105 684 2.2 TIME VARIABILITY IN THE
RADIO AND X-RAYS 688 2.3 EVIDENCE FOR A CIRCUMSTELLAR COCOON 690 2.4
ENERGY AND POWER CONSIDERATIONS 691 2.5 SEARCH FOR EXTENDED LOBES IN GRS
1915+105 691 3 THE TWO SUPERLUMINAL SOURCES AND SS 433 693 4 SEARCH FOR
"MOVING" EMISSION LINES 695 5 OTHER SOURCES OF RELATIVISTIC JETS IN THE
GALAXY 696 6 REFERENCES : 697 31. STATIONARY RELATIVISTIC MHD FLOWS MAX
CAMENZIND 699 1 INTRODUCTION 700 2 THE DISK-JET CONNECTION IN AGN AND
YOUNG STELLAR OBJECTS 701 3 MHD OF RAPIDLY ROTATING OBJECTS 703 3.1 THE
GRAVITATIONAL FIELD OF COMPACT OBJECTS 703 3.1.1 ROTATING NEUTRON STARS
705 3.1.2 ROTATING BLACK HOLES 705 3.2 ROTATIONAL ENERGY OF COMPACT
OBJECTS 707 3.3 STATIONARY MHD FLOWS 709 3.4 POLYTROPIC WIND EQUATION
714 3.5 AXISYMMETRIC MAGNETOSPHERES 718 3.6 PROSPECTS FOR TIME-DEPENDENT
MHD 719 4 RELATIVISTIC JETS AS SELF-COLLIMATED PLASMA FLOWS DRIVEN BY
RAPID ROTATION 719 4.1 THE JET-PLASMA CONFINEMENT 719 4.2
SELF-COLLIMATED SOLUTIONS OF THE GSS EQUATION 721 4.3 PLASMA DIAGNOSTICS
FOR PARSEC-SCALE JETS 722 5 CONCLUSIONS 723 6 REFERENCES 724 INDEX 727 |
| any_adam_object | 1 |
| building | Verbundindex |
| bvnumber | BV010900913 |
| callnumber-first | Q - Science |
| callnumber-label | QB521 |
| callnumber-raw | QB521 |
| callnumber-search | QB521 |
| callnumber-sort | QB 3521 |
| callnumber-subject | QB - Astronomy |
| classification_rvk | US 6300 |
| ctrlnum | (OCoLC)34548532 (DE-599)BVBBV010900913 |
| dewey-full | 523.7/2 |
| dewey-hundreds | 500 - Natural sciences and mathematics |
| dewey-ones | 523 - Specific celestial bodies and phenomena |
| dewey-raw | 523.7/2 |
| dewey-search | 523.7/2 |
| dewey-sort | 3523.7 12 |
| dewey-tens | 520 - Astronomy and allied sciences |
| discipline | Physik |
| format | Book |
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| genre | (DE-588)1071861417 Konferenzschrift 1995 Iraklion gnd-content |
| genre_facet | Konferenzschrift 1995 Iraklion |
| geographic | Sun Sonnensystem (DE-588)1236963989 gnd |
| geographic_facet | Sun Sonnensystem |
| id | DE-604.BV010900913 |
| illustrated | Illustrated |
| indexdate | 2024-09-12T00:02:21Z |
| institution | BVB |
| isbn | 079234054X |
| language | English |
| oai_aleph_id | oai:aleph.bib-bvb.de:BVB01-007290643 |
| oclc_num | 34548532 |
| open_access_boolean | |
| owner | DE-12 DE-355 DE-BY-UBR DE-20 DE-19 DE-BY-UBM DE-83 |
| owner_facet | DE-12 DE-355 DE-BY-UBR DE-20 DE-19 DE-BY-UBM DE-83 |
| physical | XL, 742 S. Ill., graph. Darst. |
| publishDate | 1996 |
| publishDateSearch | 1996 |
| publishDateSort | 1996 |
| publisher | Kluwer |
| record_format | marc |
| series2 | NATO: [Nato ASI series / C] |
| spelling | Solar and astrophysical magnetohydrodynamic flows ed. by Kanaris C. Tsinganos Dordrecht [u.a.] Kluwer 1996 XL, 742 S. Ill., graph. Darst. txt rdacontent n rdamedia nc rdacarrier NATO: [Nato ASI series / C] 481 Champ magnétique Magnétohydrodynamique Soleil Soleil - Champ magnétique ram Théorie de la dynamo Astrophysics Magnetohydrodynamics Magnetohydrodynamik (DE-588)4130803-7 gnd rswk-swf Sun Sonnensystem (DE-588)1236963989 gnd rswk-swf (DE-588)1071861417 Konferenzschrift 1995 Iraklion gnd-content Sonnensystem (DE-588)1236963989 g Magnetohydrodynamik (DE-588)4130803-7 s DE-604 Tsinganos, Kanaris C. Sonstige oth C] NATO: [Nato ASI series 481 (DE-604)BV000902768 481 GBV Datenaustausch application/pdf http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=007290643&sequence=000001&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA Inhaltsverzeichnis |
| spellingShingle | Solar and astrophysical magnetohydrodynamic flows Champ magnétique Magnétohydrodynamique Soleil Soleil - Champ magnétique ram Théorie de la dynamo Astrophysics Magnetohydrodynamics Magnetohydrodynamik (DE-588)4130803-7 gnd |
| subject_GND | (DE-588)4130803-7 (DE-588)1236963989 (DE-588)1071861417 |
| title | Solar and astrophysical magnetohydrodynamic flows |
| title_auth | Solar and astrophysical magnetohydrodynamic flows |
| title_exact_search | Solar and astrophysical magnetohydrodynamic flows |
| title_full | Solar and astrophysical magnetohydrodynamic flows ed. by Kanaris C. Tsinganos |
| title_fullStr | Solar and astrophysical magnetohydrodynamic flows ed. by Kanaris C. Tsinganos |
| title_full_unstemmed | Solar and astrophysical magnetohydrodynamic flows ed. by Kanaris C. Tsinganos |
| title_short | Solar and astrophysical magnetohydrodynamic flows |
| title_sort | solar and astrophysical magnetohydrodynamic flows |
| topic | Champ magnétique Magnétohydrodynamique Soleil Soleil - Champ magnétique ram Théorie de la dynamo Astrophysics Magnetohydrodynamics Magnetohydrodynamik (DE-588)4130803-7 gnd |
| topic_facet | Champ magnétique Magnétohydrodynamique Soleil Soleil - Champ magnétique Théorie de la dynamo Astrophysics Magnetohydrodynamics Magnetohydrodynamik Sun Sonnensystem Konferenzschrift 1995 Iraklion |
| url | http://bvbr.bib-bvb.de:8991/F?func=service&doc_library=BVB01&local_base=BVB01&doc_number=007290643&sequence=000001&line_number=0001&func_code=DB_RECORDS&service_type=MEDIA |
| volume_link | (DE-604)BV000902768 |
| work_keys_str_mv | AT tsinganoskanarisc solarandastrophysicalmagnetohydrodynamicflows |