2 edition of External aerodynamics of the magnetosphere found in the catalog.
External aerodynamics of the magnetosphere
John R. Spreiter
Published
1968
by National Aeronautics and Space Administration; for sale by the Clearinghouse for Federal Scientific and Technical Information, Springfield, Va. in [Washington]
.
Written in English
Edition Notes
| Statement | by John R. Spreiter, Alberta Y. Alksne, and Audrey L. Summers. |
| Series | NASA TN D-4482, NASA technical note ;, D-4482. |
| Contributions | Alksne, Alberta Y., joint author., Summers, Audrey L., joint author. |
| Classifications | |
|---|---|
| LC Classifications | TL521 .A3525 no. 4482 |
| The Physical Object | |
| Pagination | 70 p. |
| Number of Pages | 70 |
| ID Numbers | |
| Open Library | OL5638938M |
| LC Control Number | 68067339 |
The field of aerodynamics has had an increasingly significant effect on performance enhancement over the past 50 years. Competition Car Aerodynamics 3rd Edition continues the practical, hands-on approach of its popular predecessors to cover all aspects of motorsport aerodynamics, with more CFD and wind tunnel project material and case studies. Author Simon McBeath tackles aerodynamic /5(6). An Introduction to Ionosphere and Magnetosphere. Preview this book -distribution height-variation horizontal increase ionization ionosonde ions ions and electrons lines of force magnetic field magnetosphere magnitude mass Maxwell distribution measured molecules motion move movements neutral observed oxygen peak perpendicular.
This book is intended as a text for undergraduate and graduate courses in aerodynamics, typically offered to students of aerospace and mechanical engineering programs. It covers all aspects of aerodynamics. The book begins with a description of the standard atmosphere and basic concepts, then moves on to cover the equations and mathematical. Vehicle aerodynamics includes three interacting flow fields: • flow past vehicle body • flow past vehicle components (wheels, heat exchanger, brakes, windshield), • flow in passenger compartment. Approaches in vehicle aerodynamics 1 Adaptation of shapes from other fields Airship.
this activity, students will visit a website and learn the main features of the magnetosphere and the functioning of the Sun-Earth system. Students should start a lab book in which to keep notes about Earth’s magnetosphere, space weather, and magnetometer data. Goals 1) Students will learn about the basic elements of the Sun-Earth Size: KB. Physics of the Jovian Magnetosphere – The Book came out of this conference. Hosted by Alex Dessler (Rice University) Lindau, Federal Republic of Germany. Workshop on the Structure and Dynamics of the Jovian Magnetosphere. Hosted by Vytenis Vasyliunas (Max Planck – Institut fur Aeronomie) View full size View full size with name tags.
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External aerodynamics of the magnetosphere. [Washington] National Aeronautics and Space Administration; for sale by the Clearinghouse for Federal Scientific and Technical Information, Springfield, Va.
[] (OCoLC) Document Type: Book: All Authors / Contributors: John R Spreiter; Alberta Y Alksne; Audrey L Summers. EXTERNAL AERODYNAMICS OF THE MAGNETOSPHERE* By John R. Spreiter, Alberta Y. Alksne, and Audrey L. Summers Ames Research Center SUMMARY A comprehensive survey is given of the continuum fluid theory of the solar wind and its interaction with the Earth's magnetic field, and the rela.
The flow of the solar wind past the earth and its magnetosphere constitutes a problem similar in many ways to the familiar, but complex problem of the external aerodynamics of round-nosed bodies in a supersonic by: External aerodynamics of the magnetosphere. By A. Alksne, A. Summers and J. Spreiter.
(external link) Suggested articles. To submit an update or takedown request for this paper, please submit an Update/Correction/Removal Request. Abstract. Solar wind flow past earth and magnetosphere correspondence to external aerodynamics of round nosed bodies in supersonic strea.
adshelp[at] The ADS is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative Agreement NNX16AC86ACited by: Part of the Astrophysics and Space Science Library book series (ASSL, volume 10) Log in to check access. Buy eBook. USD External Aerodynamics of the Magnetosphere. John R.
Spreiter, Alberta Y. Alksne, Audrey L. Summers. Physics of the Magnetosphere, held on the Boston College campus, luneThis monograph is based upon the proceedings of the Summer Institute, Physics of the Magnetosphere, held on the Boston College campus, luneThe pro gram consisted of invited speakers selected by the Editors.
An attempt was made to provide comprehensive treatment of all topics ofBrand: Springer Netherlands. Earth's Magnetosphere Formed by the Low-Latitude Boundary Layer. Book • Authors: Walter J. Heikkila In hydrodynamics and aerodynamics, almost all practical problems can be accurately treated with fluid equations of motion and the thermodynamic state.
the dayside plasma sheet, and the magnetosheath. This external boundary is. (d) Direction of magnetic-field and velocity vectors. Solution for solar wind flow past the earth's magnetosphere Fig.
Various flow properties for aligned magnetohydrodynamic flow past the earth's magnetosphere for MAx = 5, M. = 10, y = | represented by constant-property contours for: (a) Density ratio by: Magnetohydrodynamics (MHD; also magneto-fluid dynamics or hydromagnetics) is the study of the magnetic properties and behaviour of electrically conducting fluids.
Examples of such magnetofluids include plasmas, liquid metals, salt water, and electrolytes. External Aerodynamics of the Magnetosphere. Magnetic merging in the magnetospheric tail. Hydromagnetic flow around the magnetosphere. Planetary and Space Science, Vol. 14, No. Plasma in the geomagnetic tail.
Aerodynamic aspects of the magnetospheric by: Magnetospheres. A magnetosphere is the region around a planet dominated by the planet's magnetic field. Other planets in our solar system have magnetospheres, but Earth has the strongest one of all the rocky planets: Earth's magnetosphere is a vast, comet-shaped bubble, which has played a crucial role in our planet's habitability.
The flow of the solar wind past the earth and its magnetosphere constitutes a problem similar in many ways to the familiar, but complex problem of the external aerodynamics. The bu eting of the magnetosphere by the solar wind and the interactions between magnetospheric and near-Earth solar wind plasma is the cause of many phenomena in the magnetosphere and the ionosphere, and a ects the way in which we observe many other features.
For many years, scientists have tried to understand the physical phenomena in-File Size: 3MB. Get this from a library. Physics of the Magnetosphere: Based upon the Proceedings of the Conference Held at Boston College June[Robert L Carovillano; John F McClay; Henry R Radoski] -- This monograph is based upon the proceedings of the Summer Institute, Physics of the Magnetosphere, held on the Boston College campus, lune Experimental Aerodynamics Drag of slender bodies •!There are no simple but accurate methods for estimating the aerodynamic forces acting on slender bodies.
•!Slender bodies are usually designed for operation at minimum drag and zero lift. •!The main consideration then, is the estimation of the drag of such Size: 1MB. A magnetosphere is a region of space surrounding an astronomical object in which charged particles are affected by that object's magnetic field.
It is created by a star or planet with an active interior dynamo. In the space environment close to a planetary body, the magnetic field resembles a magnetic dipole.
Farther out, field lines can be significantly distorted by the flow. Page A1. THE MAGNETOSPHERE, IONOSPHERE, AND ATMOSPHERE. Appendix A1 was largely developed by the following workshop group: James Slavin (Group Leader), R. Clauer, M. Engebretson, D.
Herzog, R. McPherron, J. Olson, V. Papitashvili, V. Patel, F. Rich, A. Richmond, M. Teague, R. Walker, L. Zanetti.A complete and accurate knowledge of the geomagnetic field. Magnetosphere, region in the atmosphere where magnetic phenomena and the high atmospheric conductivity caused by ionization are important in determining the behaviour of charged particles.
The Earth, in contrast to Mars and Venus, has a significant surface. Planetary encounters by numerous spacecraft launched by the USA and USSR have furnished information concerning the solar-wind interaction with the planets Mercury, Venus, Mars, and Jupiter.
While direct measurements have indicated a wide range of atmospheric densities and intrinsic magnetic field strengths.
The flow field around the planet may therefore be described to an excellent approximation by the aerodynamic models of Spreiter et al.
(,) with an impenetrable boundary surface between the solar wind and the ionosphere. A qualitative model of the flow region is shown in figure 1. U.S. Department of Transportation Federal Aviation Administration Independence Avenue, SW Washington, DC () tell-FAA (() )Missing: magnetosphere.
