did-you-know? rent-now

Amazon no longer offers textbook rentals. We do!

did-you-know? rent-now

Amazon no longer offers textbook rentals. We do!

We're the #1 textbook rental company. Let us show you why.

9781402006852

Exploring the Secrets of the Aurora

by
  • ISBN13:

    9781402006852

  • ISBN10:

    1402006853

  • Format: Hardcover
  • Copyright: 2002-10-01
  • Publisher: Kluwer Academic Pub
  • Purchase Benefits
  • Free Shipping Icon Free Shipping On Orders Over $35!
    Your order must be $35 or more to qualify for free economy shipping. Bulk sales, PO's, Marketplace items, eBooks and apparel do not qualify for this offer.
  • eCampus.com Logo Get Rewarded for Ordering Your Textbooks! Enroll Now
List Price: $120.00 Save up to $101.44
  • Digital
    $40.22
    Add to Cart

    DURATION
    PRICE

Supplemental Materials

What is included with this book?

Summary

Prominent progress in science is inevitably associated with controversies. Thus, young researchers, in particular, have to learn how to persevere during the period of controversy and struggle for acceptance. Unfortunately, the skills needed are not taught in textbooks or monographs, which mostly describe the consensus of contemporary experts. This book, which is based on my own experiences as a scientist, describes the history of the progress made in auroral science and magnetospheric physics by providing examples of ideas, controversies, struggles, acceptance, and success in some instances. Although no general methodology (if any exists) is mentioned, I hope that the reader will learn about the history of progress in auroral science and examples (right or wrong) of dealing with the controversies.

Table of Contents

Source of Figures vii
Preface xvi
Prologue xix
Search For The Unknown Quantity In The Solar Wind
1(40)
Solar Corpuscular Streams
1(5)
The Chapman-Ferraro Theory
6(5)
The Solar Wind
11(1)
Interplanetary Shock Waves
12(1)
The Modern Interpretation of the Chapman-Ferraro Theory
13(1)
The Main Phase of Geomagnetic Storms and the Ring Current
13(4)
Variety of the Development of Geomagnetic Storms
17(4)
Unknown Quantity
21(3)
The ε Parameter
24(11)
The Directly Driven and Unloading Components
35(1)
The Open Magnetosphere
36(5)
Confronting Paradigms: Aurora Research During The Early Space Age
41(48)
My Earliest Association with the Aurora
41(1)
The Auroral Zone to the Auroral Oval
42(9)
Significance of the Auroral Oval
51(3)
Auroral Substorms: Fixed Pattern to Substorm Pattern
54(14)
Auroral Storms
68(2)
Auroral Rays
70(1)
Thickness of an Auroral Curtain
70(3)
Auroral Kilometric Radiation
73(1)
Auroral Observation at the South Pole
74(1)
Auroral Spectra as Tools for Detecting Extraterrestrial Life
74(2)
Emperor Showa and the Aurora
76(1)
An Exciting New Development
77(12)
Realizing The Dream Of Our Pioneers: Polar Magnetic Substorms And The Associated Current System
89(44)
The Three-Dimensional Current System
90(7)
The Uniqueness Problem
90(1)
Chapman's Equivalent Current System
90(4)
Birkeland-Alfven Model
94(3)
Alaska Meridian Chain of Magnetic Observatories
97(2)
The IMS Meridian Chains of Observatories
99(1)
Bostrom's Current Loops
100(9)
Nikolsky's Spiral
109(3)
Substorm Onset
112(3)
Changes of Magnetic Energy in the Magnetotail
115(4)
Storm-Substorm Relationship
119(1)
Geomagnetic Indices
120(1)
Publication of Solar-Terrestrial Physics from Oxford University Press
121(3)
Summary of Chapters 1, 2, and 3
124(9)
Is The Earth's Dipole Really Off-Centered And Inclined?: Planetary Magnetic Fields
133(16)
Introduction
133(1)
Rotation of the Solar Magnetic Dipolar Field on the Source Surface
134(5)
Large Inclination and Eccentricity of the Dipole-like Field of Uranus and Neptune
139(3)
Is the Earth's Dipole Actually Inclined with Respect to the Rotation Axis?
142(1)
Does the Main Dipole of the Geomagnetic Field Rotate during the Reversals?
143(2)
Heliospheric Current Sheet
145(4)
Myth Of The Emerging Flux Tubes: Sunspots And Solar Flares
149(16)
Introduction
149(1)
Emerging Magnetic Flux Tubes
150(3)
Energy Source
153(3)
Sunspots
156(2)
Force-free Fields and Solar Flares
158(4)
Magnetic Reconnection
162(3)
Synthesis Of The Four Major Disciplines: Predicting Geomagnetic Storms As A Space Weather Project
165(32)
Introduction
165(1)
Modeling the Background Solar Wind Flow
166(4)
Parameterizing Solar Events
170(1)
Modeling the Propagation of Shock Waves
171(2)
Detecting Shock Waves by IPS
173(4)
Estimating the Velocity, Density, and IMF at the Earth
177(1)
Characterizing Geomagnetic Storms
177(2)
Predicting Ionospheric Effects
179(1)
Effects on Power Transmission Lines and Oil/Gas Pipelines
180(1)
Missing Links
181(4)
High-speed Streams from Coronal Holes
185(1)
A New Example
186(6)
Summary
192(5)
Beyond The Inner Heliosphere: The Magnetic Field Structure Of The Outer Heliosphere: A Three-Dimensional Model
197(7)
Epilogue 204(9)
Further Readings: Mostly Historical 213(4)
Name Index 217(6)
Index 223(4)
A Scenario on Substorm Onset (Note added on March 1, 2002) 227

Supplemental Materials

What is included with this book?

The New copy of this book will include any supplemental materials advertised. Please check the title of the book to determine if it should include any access cards, study guides, lab manuals, CDs, etc.

The Used, Rental and eBook copies of this book are not guaranteed to include any supplemental materials. Typically, only the book itself is included. This is true even if the title states it includes any access cards, study guides, lab manuals, CDs, etc.

Rewards Program