Solar wind flow about the terrestrial planets 1. Modeling bow shock position and shape

General technique for modeling the position and shape of planetary bow waves are reviewed. A three-parameter method was selected to model the near portion (i.e.,x′ > −1 Rob) of the Venus, earth, and Mars bow shocks and the results compared with existing models using 1 to 6 free variables. By limiting consideration to the forward part of the bow wave, only the region of the shock surface that is most sensitive to obstacle shape and size was examined. In contrast, most other studies include portions of the more distant downstream shock, thus tending to reduce the planetary magnetosphere in question to a point source and constrain the resultant model surfaces to be paraboloid or hyperboloid in shape to avoid downstream closure. It was found by this investigation that the relative effective shapes of the near Martian, Cytherean, and terrestrial bow shocks are ellipsoidal, paraboloidal, and hyperboloidal, respectively, in response to the increasing bluntness of the obstacles that Mars, Venus, and earth present to the solar wind. The position of the terrestrial shock over the years 1965 to 1972 showed only a weak dependence on the phase of the solar cycle after the effects of solar wind dynamic pressure on magnetopause location were taken into account. However, the bow wave of Venus was considerably more distant around solar maximum in 1979 than at minimum in 1975–6 suggesting a solar cycle variation in its interaction with the solar wind. Finally, no significant deviations from axial symmetry were found when the near bow waves of the earth and Venus were mapped into the aberrated terminator plane. This finding is in agreement with the predictions of gas dynamic theory which neglects the effects of the IMF on the grounds of their smallness. Farther downstream where the bow wave position is being limited by the MHD fast mode Mach cone, an elliptical cross section is expected and noted in the results of other investigations.

[1]  C. Russell,et al.  The influence of the interplanetary magnetic field and thermal pressure on the position and shape of the magnetopause , 1981 .

[2]  C. Russell The magnetic field of Mars: Mars 5 evidence re‐examined , 1978 .

[3]  T. Breus Venus: Review of present understanding of solar wind interaction , 1979 .

[4]  J. Spreiter,et al.  ON THE EFFECT OF A WEAK INTERPLANETARY MAGNETIC FIELD ON THE INTERACTION BETWEEN THE SOLAR WIND AND THE GEOMAGNETIC FIELD , 1963 .

[5]  F. Michel Detectability of disturbances in the solar wind , 1965 .

[6]  G. Schubert,et al.  Observations of moon-plasma interactions by orbital and surface experiments , 1974 .

[7]  J. Binsack,et al.  Explorer 33 and 35 plasma observations of magnetosheath flow , 1972 .

[8]  W. Shen The earth's bow shock in an oblique interplanetary field. , 1972 .

[9]  O. Vaisberg,et al.  On the nature of the solar-wind-Mars interaction , 1976 .

[10]  A. Remizov,et al.  Magnetic field and plasma inside and outside of the Martian magnetosphere , 1976 .

[11]  H. Pérez-de-Tejada Evidence for a viscous boundary layer at the Venus ionopause from the preliminary Pioneer Venus results , 1980 .

[12]  S. Orsini,et al.  Backstreaming ions outside the Earth's bow shock and their interaction with the solar wind , 1980 .

[13]  E. F. Lyon,et al.  Experimental evidence for a detached lunar compression wave. , 1969 .

[14]  G. K. Walters Effect of oblique interplanetary magnetic field on shape and behavior of the magnetosphere , 1964 .

[15]  J. Gosling,et al.  Solar‐wind speed variations 1964–1967: An autocorrelation analysis , 1972 .

[16]  J. Wolfe The large-scale structure of the solar wind , 1971 .

[17]  V. Formisano,et al.  Solar wind interaction with the earth's magnetic field. II - Magnetohydrodynamic bow shock. , 1973 .

[18]  J. Spreiter,et al.  Solar wind flow past Venus: Theory and comparisons , 1980 .

[19]  R. Auer Magnetohydrodynamic aspects of the Earth's bow shock 2. Motions induced by directional discontinuities , 1974 .

[20]  J. Slavin,et al.  The effect of solar wind structure on magnetospheric energy supply during solar cycle 20 , 1981 .

[21]  M. Dryer,et al.  Magnetogasdynamic boundary condition for a self-consistent solution to the closed magnetopause. , 1965 .

[22]  K. Gringauz A comparison of the magnetospheres of Mars, Venus and the Earth , 1981 .

[23]  A. Rizzi,et al.  Aligned magnetohydrodynamic solution for solar wind flow past the earth's magnetosphere , 1974 .

[24]  C. Russell,et al.  Position and shape of the Venus bow shock: Pioneer Venus Orbiter observations , 1979 .

[25]  R. S. Wolff,et al.  A model of the variability of the Venus ionopause altitude , 1979 .

[26]  C. Russell On the relative locations of the bow shocks of the terrestrial planets , 1977 .

[27]  C. Russell The interaction of the solar wind with Mars, Venus and Mercury , 1979 .

[28]  C. Russell,et al.  A comparison of Pioneer Venus and Venera bow shock observations: Evidence for a solar cycle variation , 1979 .

[29]  K. W. Behannon,et al.  Bow Shock and magnetosheath waves at Mercury , 1975 .

[30]  E. Smith,et al.  Preliminary results from the Ogo 1 Search Coil Magnetometer: Boundary positions and magnetic noise spectra , 1966 .

[31]  C. Russell,et al.  Observation of the Venus mantle, the boundary region between solar wind and ionosphere , 1980 .

[32]  J. Olson,et al.  On the local time dependence of the bow shock wave structure , 1974 .

[33]  M. Dryer SOLAR WIND INTERACTIONS: HYPERSONIC ANALOGUE. , 1970 .

[34]  J. King Solar cycle variations in IMF intensity , 1979 .

[35]  J. King Interplanetary medium data book , 1977 .

[36]  M. D. Vandyke The supersonic blunt-body problem - Review and extension , 1972 .

[37]  J. R. Spreiter,et al.  Solar-wind flow past objects in the solar system , 1970 .

[38]  N. Ness,et al.  Multiple crossings of the Earth's bow shock at large geocentric distances , 1971 .

[39]  E. Smith Planetary magnetic field experiments. , 1968 .

[40]  C. Russell,et al.  The Venus ionosphere as an obstacle to the solar wind , 1981 .

[41]  M. V. Dyke,et al.  The Supersonic Blunt-Body Problem - Review and Extension , 1958 .

[42]  V. Formisano Orientation and Shape of the Earth's Bow Shock in Three Dimensions , 1979 .

[43]  N F Ness The Magnetic Fields of Mercury, Mars, and Moon , 1979 .

[44]  James A. Slavin,et al.  The effect of erosion on the solar wind stand-off distance at Mercury , 1979 .

[45]  C. Russell,et al.  Large-scale coherence and high velocities of the earth's bow shock on February 12, 1969. , 1972 .

[46]  J. Scudder,et al.  An empirical polytrope law for solar wind thermal electrons between 0.45 and 4.76 AU: Voyager 2 and Mariner 10 , 1980 .

[47]  S. Dolginov On The magnetic field of Mars: Mars 2 and 3 evidence , 1978 .

[48]  G. I. Volkov,et al.  Plasma near Venus from the Venera 9 and 10 wide-angle analyzer data , 1978 .

[49]  A. Summers,et al.  Hydromagnetic flow around the magnetosphere , 1966 .

[50]  N. Ness,et al.  The magnetic field of Mercury, 1 , 1975 .

[51]  A. Remizov,et al.  On electron and ion components of plasma in the antisolar part of near‐Martian space , 1976 .

[52]  V. Formisano,et al.  Solar wind and location of shock front and magnetopause at the 1969 solar maximum , 1970 .

[53]  C. Russell,et al.  The dynamic behavior of the Venus ionosphere in response to solar wind interactions , 1980 .

[54]  P. Cloutier Solar-wind interaction with planetary ionospheres , 1976 .

[55]  J. Chao,et al.  The ratio of specific heats for postshock plasmas of a detached bow shock - An MHD model. [in solar wind-earth interaction] , 1974 .

[56]  N. Ness,et al.  Observations and interpretation of the lunar mach cone , 1970 .

[57]  L. H. Brace,et al.  Empirical models of the electron temperature and density in the Venus ionosphere , 1980 .

[58]  E. Greenstadt,et al.  Initial ISEE magnetometer results: Shock observation , 1979 .

[59]  D. H. Fairfield,et al.  Average and unusual locations of the Earth's magnetopause and bow shock , 1971 .

[60]  O. Vaisberg,et al.  Structure and variations of solar wind-Mars interaction region , 1975 .

[61]  A. Hundhausen,et al.  Plasma flow pattern in the Earth's magnetosheath , 1969 .

[62]  J. Slavin,et al.  Magnetic flux transfer associated with expansions and contractions of the dayside magnetosphere , 1978 .

[63]  C. Russell,et al.  Study of waves in the earth's bow shock. , 1972 .

[64]  D. Intriligator,et al.  An empirical model of the Venusian outer environment 2. The shape and location of the bow shock , 1980 .

[65]  J. Spreiter,et al.  A new predictive model for determining solar wind-terrestrial planet interactions , 1980 .

[66]  M. Dryer,et al.  Application of the hypersonic analog to the standing shock of Mars , 1967 .

[67]  G. Siscoe,et al.  Observations at the planet Mercury by the plasma electron experiment, Mariner 10 , 1976 .

[68]  S. Dolginov On the magnetic field of Mars: Mars 5 Evidence , 1978 .

[69]  C. Russell,et al.  THE INTERACTION OF THE SOLAR WIND WITH VENUS , 1983, Venus.

[70]  R. T. Merrill Magnetic and Mineralogical Changes Associated with Low-Temperature Oxidation of Magnetite H. P. JoHso Geophysics Program, Unive'sity oWashington, Seattle 98195 , 1972 .

[71]  O. L. Vaisberg,et al.  Mars-Plasma Environment , 2013 .

[72]  D. Fairfield Global Aspects of the Earth's Magnetopause , 1979 .

[73]  K. Ogilvie,et al.  Long-term variations of the solar wind proton parameters , 1974 .

[74]  J. Gosling,et al.  Vela 2 measurements of the magnetopause and bow shock positions , 1967 .