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r I RADIO SCIENCE Journal of Re search NBS /USNC-URSI Vol. 69D, No.2, February 1965 Prefa ce to "Wave s in Plasma ll Paper s The first thirteen papers of this i ss ue deal with the propagation of el ectromagnetic waves in ionized media . Th e importance of this subj ect has increased significantly in recent years. 'With the advent of manned space vehicles and the need for communications during "reentry" , the class ical plasma sheath has ceased to be a laboratory curi osity. The all eviati on of the "black-out" effects associated with the shock induced layer of ionized gas which surrounds a reentry yehicle is currently a pr ess in g problem. Some of the papers in this issue deal dire ctly with this topic. Th e first paper , by Dr. Bachynski of the R OA Research Laboratories in : Montreal, ser ves as ttl1 excellen t introd llction to this topi c. Th e radiation characteristics of satellite-borne antennas which are immersed in ionized media (or plas ma ) such as the i onsphere are a related subj ect which l'ecently has received a gl'eat deal of attent ion . In the paper by Professor Fel sen, it is shown that a greftt deal of insigh t into this probl em is obtained by st udying the refractive index diagrams which rel ate the propagation vector for the homogeneolls ph,sma with the orein tation of earth' s magnetic field. III most reali stic s ituation s, the plasma medium is not unbounded and homo geneoLi s. Some very interesting effects are a res ult of the surface waves which m ay exist at the interrace be Lwee n th e metallic surface of the yehicle and the plas ma . A pr oblem of this type is treated in the paper by Drs. Adachi and :'1ushiake of Tohoku Ulli\Tersity in J apan. By using a Fourier transform method , they find that surface wftves will be excited by a magnetic line source on a plasma-coated co ndu cting plane. Furthermor e, it is shown that the char acter istics of this wave may be controlled by the stren gt h of a supe rimpo sed d-c magnetic field. An important physical cll aracteris Lic of a pl asma layer is the profile of thE' el ectron density var iation in the trans\'e]'se direction. Recently, techni ques have been developed to dedu ce this profile from dat a on the refraction of a microwave beam . In a short but import ant paper , Professor Oullen of Sheffi eld Universit y dis cu ss ed the validi ty of ray theory for this appli cati on. When an antenna is immersed in the plasma, an imp ortant property is the driving point imp ed ance. Even for antennas located in free space, t hi s can be a diffi cult problem to treat theoretically. Many additional co mplications occur when dealing with inhomogeneous plasma as m ay be seen in the paper by Dr. Galejs of Syl vania Eledric Products. Despite the complexi ty of the problem, he obtains specific results for the self and mutual admittance of waveguide-backed slots which rad iate into a s tratified pl asma layer.

Preface to 'Waves in Plasma' papers...r I RADIO SCIENCE Journal of Research NBS/USNC-URSI Vol. 69D, No.2, February 1965 Preface to "Wave s in Plasmall Papers The first thirteen papers

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Page 1: Preface to 'Waves in Plasma' papers...r I RADIO SCIENCE Journal of Research NBS/USNC-URSI Vol. 69D, No.2, February 1965 Preface to "Wave s in Plasmall Papers The first thirteen papers

r I

RADIO SCIENCE Journal of Research NBS/USNC-URSI Vol. 69D, No.2, February 1965

Preface to "Waves in Plasmall Papers

The first thirteen papers of this issue deal with the propagation of electromagnetic waves in ionized media. The importance of this subj ect has in creased significantly in recent years. 'With the advent of manned space vehicles and the need for communications during "reentry", the classical plasma sheath has ceased to be a laboratory curiosity. The alleviation of the "black-out" effects associated with the shock induced layer of ionized gas which surrounds a reentry yehicle is currently a pressin g problem. Some of the papers in this issue deal directly with this topic. The first paper, by Dr. Bachynski of the R OA Research Laboratories in :Montreal, ser ves as ttl1 excellen t introd llction to this topic.

The radiatio n ch aracteristics of satellite-borne antennas which are immersed in ionized media (or plasma) such as the ionsphere are a related subj ect which l'ecently has received a gl'eat deal of attention . In the paper by Professor Felsen, it is shown that a greftt deal of insigh t into th is problem is obtained by studying the refractive index diagrams which relate the propagation vector for the homogeneoll s ph,sma with the orein tation of earth's magnetic field.

III most realistic situations, the plasma medium is not unbounded and homogeneoLi s. Some very interesting effects are a result of the surface waves which may exist at the interrace beLween the metallic surface of the yehicle and the plasma. A problem of this type is treated in the paper by Drs. Adachi and :'1ushiake of Tohoku Ulli\Tersity in J apan. By using a F ourier transform method, they find that surface wftves will be excited by a magnetic line source on a plasma-coated conducting plane. Furthermore, it is shown that the char acteristics of this wave may be controlled by the stren gth of a superimposed d-c magnetic field.

An important physical cll aracteris Lic of a plasma layer is the profile of thE' electron density variation in the tran s\'e]'se direction. Recently, techniques have been developed to deduce this profile from data on the refraction of a microwave beam . In a short but important paper, Professor Oullen of Sheffield University discussed the validity of ray theory for this application.

When an antenna is immersed in the plasma, an important property is the driving point imped ance. Even for antennas located in free space, this can be a difficult problem to treat theoretically. Many additional co mplications occur when dealing with inhomogeneous plasma as may be seen in the paper by Dr. Galej s of Sylvania Eledric Products. Despite the complexity of the problem, he ob tains specific results for the self and mutual admittance of waveguide-backed slots which radiate in to a stratified plasma layer.

Page 2: Preface to 'Waves in Plasma' papers...r I RADIO SCIENCE Journal of Research NBS/USNC-URSI Vol. 69D, No.2, February 1965 Preface to "Wave s in Plasmall Papers The first thirteen papers

In the classical theory of treating wave propagation in a simple plasma, it is assumed that collisions may be accounted for by assuming that the electron experiences a retarding force proportional to its velocity. This leads to the Appleton-Hartree formula for the two refractive indices of the ionized medium where the collision frequency is a constant. How­ever, there is a growing body of experimen tal evidence which indicates that the collision fre­quency is approximately proportional to the square of the electron velocity. In a most enlightening paper, Dr. Budden of Cambridge University discusses the modifications required in order to generalize the theory. In the following paper, Dr. Mentzoni of Sylvania Electric Products uses microwave methods to determine the electron collision frequency in an oxygen­type plasma. His results were consistent with the dependence according to the square of the electron velocity.

N ow that radio signals are received on the ground from satellites, it is realized that the ionospheric plasma has numerous irregularities and perturbations. In a useful summary paper, Dr. Heisler of the University of Sydney in Australia gives an accoun t of various experi­mental procedures for observing perturbations in ionospheric plasma. As he points out, a significant feature is the discrepancy between speeds and directions of perturbations measured by different observational techniques.

Some information about bounded plasma bodies (or idealized perturbations) can be ob­tained by measuring the radar cross section as a fun ction of the scattering angle. Fundamental to a study is the influence of the parameters of the plasma on the strength of the scattered wave. By using a modified form of geometrical op tics, Drs. Lee, Peters, and Walter of Ohio State U niversity show how to calculate the radar cross section of an infinitely long cylinder of plasma which has a superimposed d-c magnetic field. They demonstrate the validity of their method by comparing their results with those calculated by using the known exact solu­tion for the problem. In the following paper, Dr. Peters uses a similar approximate method to calculate the cross section of a spherical plasma body.

In most of the li terature on "waves in plasma," including the above ten papers, the plasma is regarded as "cold." When a finite temperature plasma is considered , it is really necessary to consider the effect of finite compressibility. This means, in effect, that a source placed in a warm plasma will excite both electroacoustic- and electromagnetic-type waves. Then , in the limiting case of zero temperature, the electroacoustic wave ceases to propagate and the plasma becomes "cold ." This subject, which has received considerable attention in the past year, is discussed in an interesting paper by Dr. Chen of Michigan State University. In a companion paper, he also considers the effect of finite compressibili ty on the radar return from orbiting bodies immersed in the ionospheric plasma. Dr. Chen suggests that the large out­bursts of the observed reflected HF signals from satellites may be attributed to the hitherto neglected electroacoustic wave. It is clearly evident that this subj ect warrants further study.

The final paper in the issue, contributed by the editor, also deals with electroacoustic and electromagnetic waves in a compressible plasma. It is shown that a cylindrical inhomogeneity in a warm plasma will serve as a mechanism for conversion of electromagnetic modes to electro­acoustic modes and vice versa.

It is planned that the following issue of Radio Science will contain additional papers on "waves in plasma" in addition to the regular contributions.

JAMES R. WAIT, Editor.