Disclaimer: The following material is being kept online for archival purposes.
Although accurate at the time of publication, it is no longer being updated. The page may contain broken links or outdated information, and parts may not function in current web browsers.
The Exploration of the Earth's Magnetosphere
Illustration by Steele Hill
An educational web site by David P. Stern and Mauricio Peredo
. Your comments and suggestions may be sent to Dr. David P. Stern at education("at" symbol)phy6.org. Unless overloaded, I will try to reply. If your question concerns any file here, please name it!
The Spanish version covers most files, but the French one is still underway (3/2003). Both home pages list translated files in bold face.
- Open here the home page of a Spanish translation "La Exploración de la Magnetosfera Terrestre", by J. Méndez of Algorta, Spain.
- Open here the home page of a French translation L'Exploration de la Magnétosphère Terrestre , by Kamil Fadel and Marielle Vergès of Paris, France. Only sections listed there in bold face have been translated.
We actively seek volunteer translators to other languages. Please contact the author Dr. David P. Stern at education("at" symbol)phy6.org.
This is the home page of an overview of space research on the Earth's environment in space. The description is non-mathematical but quite detailed, and here is what it contains:
INTRODUCTORY AND GENERAL:
Overview.... for those not sure how to use this site.
Introduction (former home page).... what to expect to find here.
SUMMARY FILES .... Capsule descriptions of the different sections:
"CONSTELLATION" MISSIONS AND FUTURE RESEARCH
Articles and thoughts
(primarily for active researchers)
"Recollections of Space Research"
Talk presented 13 September 2006, in Anahuac, Mexico
Original text of comment submitted to Eos (3 Nov 2007) on "A Turning
Point in Auroral Physics" by Duncan Bryant (26 September 2006).
TABLE OF CONTENTS .... The files themselves:
1. The Magnetosphere
1H. History: 1600--Gilbert's Terrella.
2. Magnetic Fields
2H. History: 1820: Oersted discovers electromagnetism.
3. The Polar Aurora
3H. History: Birkeland models the aurora in his laboratory
4H. History: 1896--J.J.Thomson discovers the electron
4a. Electricity as a Fluid
5. Magnetic Field Lines
5H. History: 1846--Faraday introduces the idea of fields.
5a-1. Electromagnetic Induction--1. New!!!
5a-2. Electromagnetic Induction--2.
6. Electromagnetic Waves
7a. The Fluorescent Lamp: a plasma you can use
7H. History : 1927--Irving Langmuir has a new use for the word "plasma".
8. Positive Ions
8H. History: 1884--Svante Arrhenius proposes a theory of "ions".
9. Trapped Radiation
9H. History: 1896--Henri Poincare shows magnetic field lines guide ions.
10. Motion of Trapped Radiation
10H. History: 1910--Einstein introduces "adiabatic invariants".
10a. Particle Drift in Space (optional)
11. Explorers 1 and 3
12. The Radiation Belts
12H. History: 1958--Inner radiation belt is explained.
13. Energetic Particles
14. Synchronous Orbit
16. The Sun
17. The Sun's Corona
16H. History: 1843--Heinrich Schwabe discovers the sunspot cycle.
18. The Solar Wind
18A. Drawing Interplanetary Magnetic Field Lines.
18H. History: 1959, 1961--First direct observations of the solar wind.
18B. The Heliosphere.
19. The Magnetopause
19H. History: 1930--the magnetic storm theory of Chapman and Ferraro.
20. Structure of the Earth's Magnetosphere
21. Lagrangian Points
22. The Wind Spacecraft
23. The Tail of the Magnetosphere
25. Electric Currents from Space
25H. History: 1903--Birkeland observes the electric currents of the polar aurora.
26. The Polar Caps
26H. History: 1895--Birkeland's terrella experiment.
27. Auroral Imaging
28. Auroral acceleration
29. Low Polar Orbit
30. Magnetic Storms
31. Space Weather
32. Magnetospheres other than Ours
33. Cosmic Rays
34 High Energy Particles in the Universe
35. Solar Energetic Particles
For a quick rundown of what these files cover, look up the Overview file. Or else, start wherever your interest lies!
Last updated 20 November 2003
Above is background material for archival reference only.