Overview

"In summary, we can conclude that the contributions of the different ionization processes to the total ionization rate for the most abundant interstellar species are basically known. The ionization of the noble gases He and Ne is almost completely dominated by photoionization, whereas for H charge-exchange with the solar wind is most important. For other species, such as 0 and Ar, both processes contribute significantly. Electron impact ionization can typically contribute by '"" 10% to the total rate in the inner Solar System. Because direct measurements of the solar EUV flux are not yet continuously available, the variation of the ionization rate over the solar cycle still contains a relatively large uncertainty. The recent measurements of pickup ion distributions and of the neutral helium gas provide an independent tool to determine the total ionization rate that can be used to cross calibrate with the results obtained for the individual ionization processes. Acknowledgements The authors are grateful to M. Allen for supplying us with new data on photoioniza­ tion cross-sections compiled by him. We thank also M. Gruntman for drawing our attention to and support in collecting the most recent data on charge-exchange cross-sections. D. R. was supported by grant No. 2 P03C. 004. 09 from the Com­ mittee for Scientific Research (Poland). This work was also supported in part through NASA contract NAS7-918, NSF Grant INT-911637, NASA Grant NAGW- 2579."

Full Product Details

Author:   Rudolf von Steiger ,  R. Lallement ,  M.A. Lee
Publisher:   Springer
Imprint:   Springer
Edition:   Softcover reprint of the original 1st ed. 1996
Volume:   1
Dimensions:   Width: 16.00cm , Height: 2.20cm , Length: 24.00cm
Weight:   0.662kg
ISBN:  

9789401072960

ISBN 10:   9401072965
Pages:   399
Publication Date:   20 September 2011
Audience:   Professional and scholarly ,  Professional & Vocational
Format:   Paperback
Publisher's Status:   Active
Availability:   Manufactured on demand  
We will order this item for you from a manufactured on demand supplier.

Table of Contents

Science as an Adventure.- The Heliosphere.- The Heliosphere.- The Heliospheric Magnetic Field.- The Solar Wind: A Turbulent Magnetohydrodynamic Medium.- Voyager Observations of the Magnetic Field, Interstellar Pickup Ions and Solar Wind in the Distant Heliosphere.- Origin of C+ Ions in the Heliosphere.- Radio Emissions from the Outer Heliosphere.- A Summary of Solar Wind Observations at High Latitudes: Ulysses.- Ionization Processes in the Heliosphere — Rates and Methods of Their Determination.- 3-D Magnetic Field and Current System in the Heliosphere.- Modelling the Heliosphere.- The Termination Shock.- The Termination Shock of the Solar Wind.- Composition of Anomalous Cosmic Rays and Implications for the Heliosphere.- Implications of a Weak Termination Shock.- The Acceleration of Pickup Ions.- The Isotopic Composition of Anomalous Cosmic Rays from SAMPEX.- The Local Interstellar Medium.- GHRS Observations of the LISM.- In Situ Measurements of Interstellar Dust with the Ulysses and Galileo Spaceprobes.- The Local Bubble, Current State of Observations and Models.- The Local Bubble, Origin and Evolution.- The Interstellar Gas Flow Through the Heliospheric Interface Region.- LISM Structure — Fragmented Superbubble Shell?.- Relative Ionizations in the Nearest Interstellar Gas.- Properties of the Interstellar Gas Inside the Heliosphere.- Local Clouds: Distribution, Density and Kinematics Through Ground-Based and HST Spectroscopy.- Possible Shock Wave in the Local Interstellar Plasma, Very Close to the Heliosphere.- Interstellar Grains in the Solar System: Requirements for an Analysis.- Modelling of the Interstellar Hydrogen Distribution in the Heliosphere.- Observations of the Local Interstellar Medium with the Extreme Ultraviolet Explorer.- Recent Results on theParameters of the Interstellar Helium from the Ulysses/GAS Experiment.- Interaction Between HS And Lism.- Physical and Chemical Characteristics of the ISM Inside and Outside the Heliosphere.- Axisymmetric Self-Consistent Model of the Solar Wind Interaction with the LISM: Basic Results and Possible Ways of Development.- UV Studies and the Solar Wind.- Quasilinear Relaxation of Interstellar Pickup Ions.- The Abundance of Atomic 1H, 4He, and 3He in the Local Interstellar Cloud from Pickup Ion Observations with SWICS on Ulysses.- Physics of Interplanetary and Interstellar Dust.- Relations Between ISM Inside and Outside the Heliosphere.- The Local Interstellar Medium Viewed Through Pickup Ions, Recent Results and Future Perspectives.- Moment Equation Description of Interstellar Hydrogen.- Pickup Protons in the Heliosphere.- Author index.

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