Introduction to Ionospheric Physics

Keyword(s):  
Eos ◽  
1973 ◽  
Vol 54 (10) ◽  
pp. 900 ◽  
Author(s):  
C. S. Gillmor ◽  
C. J. Terman

1971 ◽  
Vol 2 (2) ◽  
pp. 45
Author(s):  
S.H. Hall

If one seeks in any dictionary the meaning of geophysics, it is difficult, to my mind, to find an entirely satisfying one. One I found was the 'study of physical processes relating to the Earth'. A better one I feel would read 'the study of physical processes, state and properties relating to the Earth' ---. Most geophysicists not long ago insisted that this definition included the aesthenosphere, 1ithosphere, atmosphere, ionosphere, magnetosphere etc. -- if one judges by the contents of some geophysical journals, and thereby considered physical oceanography, meteorology, ionospheric physics, etc. as aspects of the all-embracing title-geophysics. In speaking on this topic as it relates to a department of geology, I should add that they have not had the temerity to include geology as a further aspect.


Nature ◽  
1985 ◽  
Vol 317 (6033) ◽  
pp. 114-115 ◽  
Author(s):  
M.J. Rycroft
Keyword(s):  

2010 ◽  
Vol 46 (1) ◽  
pp. 94
Author(s):  
T.W. Garner ◽  
T.L. Gaussiran ◽  
B.W. Tolman ◽  
R.B. Harris ◽  
R.S. Calfas ◽  
...  

Most of the matter in the Universe is in the plasma state. A plasma will be defined and the concepts of quasi-neutrality and Debye distance introduced. The subject has its historical roots in gas discharge, astrophysics and ionospheric physics. Key theoretical concepts were developed in the context of those subjects. However, only in the last two decades, under the pressures of the controlled thermonuclear and space exploration programmes, have these concepts been tested experimentally. The theory of collisions in plasma has special features owing to the Coulomb nature of the interaction. Magnetized plasma is a medium in which a rich variety of small signal waves can propagate. Charged particle—wave interactions lead to collisionless (Landau) damping and growth mechanisms. Finally, nonlinear phenomena in plasma can and do change its transport properties by orders of magnitude. Our lack of detailed understanding of these nonlinear phenomena applies equally to natural plasmas and to plasmas in both inertially and magnetically confined fusion systems. This feature provides the challenge and the fascination of high temperature plasma physics.


2018 ◽  
Vol 36 (1) ◽  
pp. 125-138 ◽  
Author(s):  
James A. D. Parker ◽  
S. Eleri Pryse ◽  
Natasha Jackson-Booth ◽  
Rachel A. Buckland

Abstract. The main ionospheric trough is a large-scale spatial depletion in the electron density distribution at the interface between the high- and mid-latitude ionosphere. In western Europe it appears in early evening, progresses equatorward during the night, and retreats rapidly poleward at dawn. It exhibits substantial day-to-day variability and under conditions of increased geomagnetic activity it moves progressively to lower latitudes. Steep gradients on the trough-walls on either side of the trough minimum, and their variability, can cause problems for radio applications. Numerous studies have sought to characterize and quantify the trough behaviour. The Electron Density Assimilative Model (EDAM) models the ionosphere on a global scale. It assimilates observations into a background ionosphere, the International Reference Ionosphere 2007 (IRI2007), to provide a full 3-D representation of the ionospheric plasma distribution at specified times and days. This current investigation studied the capability of EDAM to model the ionosphere in the region of the main trough. Total electron content (TEC) measurements from 46 GPS stations in western Europe from September to December 2002 were assimilated into EDAM to provide a model of the ionosphere in the trough region. Vertical electron content profiles through the model revealed the trough and the detail of its structure. Statistical results are presented of the latitude of the trough minimum, TEC at the minimum and of other defined parameters that characterize the trough structure. The results are compared with previous observations made with the Navy Ionospheric Monitoring System (NIMS), and reveal the potential of EDAM to model the large-scale structure of the ionosphere. Keywords. Ionosphere (midlatitude ionosphere; modelling and forecasting) – radio science (ionospheric physics)


2000 ◽  
Vol 18 (9) ◽  
pp. 1242-1247 ◽  
Author(s):  
T. Turunen ◽  
J. Markkanen ◽  
A. P. van Eyken

Abstract. Incoherent scatter radars measure ionosphere parameters using modified Thomson scatter from free electrons in the target (see e.g. Hagfors, 1997). The integrated cross section of the ionospheric scatterers is extremely small and the measurements can easily be disturbed by signals returned by unwanted targets. Ground clutter signals, entering via the antenna side lobes, can render measurements at the nearest target ranges totally impossible. The EISCAT Svalbard Radar (ESR), which started measurements in 1996, suffers from severe ground clutter and the ionosphere cannot be measured in any simple manner at ranges less than about 120–150 km, depending on the modulation employed. If the target and clutter signals have different, and clearly identifiable, properties then, in principle, there are always ways to eliminate the clutter. In incoherent scatter measurements, differences in the coherence times of the wanted and unwanted signals can be used for clutter cancellation. The clutter cancellation must be applied to all modulations, usually alternating codes in modern experiments, used for shorter ranges. Excellent results have been obtained at the ESR using a simple pulse-to-pulse clutter subtraction method, but there are also other possibilities.Key words: Radio science (ionospheric physics; signal processing; instruments and techniques)


Sign in / Sign up

Export Citation Format

Share Document