1996
DOI: 10.1029/95ja03479
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Interplanetary discontinuities and Alfvén waves at high heliographic latitudes: Ulysses

Abstract: This paper presents the results of the first statistical study of interplanetary directional discontinuities at both low and high heliographic latitudes measured by the Ulysses magnetometer. There is a gradual decrease in the rate of occurrence of interplanetary discontinuities (ROIDs) with increasing radial distance. From 1 to 5 AU, an e−(r−1)/5 dependence is derived. Much of this decrease is believed to be an artifact due to the discontinuity thickening with decreasing |B|, falling outside the detection crit… Show more

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Cited by 57 publications
(64 citation statements)
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“…The angular distribution of wave vector k is assumed to be a forward hemisphere centering in the direction of V || . The observation of the propagation directions of solar wind rotational discontinuities reported by Tsurutani et al (1996) (see also Tsurutani and Ho, 1999) has shaped our choice for the above assumption, In addition, this assumption also appears to agree with some recent work on the predominance of quasi-perpendicular turbulence versus quasi-parallel turbulence (Bieber et al, 1996).…”
Section: Scattering Mean Free Paths Determined By Particle Measurementssupporting
confidence: 64%
“…The angular distribution of wave vector k is assumed to be a forward hemisphere centering in the direction of V || . The observation of the propagation directions of solar wind rotational discontinuities reported by Tsurutani et al (1996) (see also Tsurutani and Ho, 1999) has shaped our choice for the above assumption, In addition, this assumption also appears to agree with some recent work on the predominance of quasi-perpendicular turbulence versus quasi-parallel turbulence (Bieber et al, 1996).…”
Section: Scattering Mean Free Paths Determined By Particle Measurementssupporting
confidence: 64%
“…Kinetic directional discontinuities Tsurutani et al (1996) have demonstrated that DDs were more prevalent in solar wind high speed streams than in slow speed streams. The overabundance of DDs was a factor of 5 to 10 whereas enhanced solar wind convection (higher speeds) could only explain a factor of $2 difference.…”
Section: Directional Discontinuities (Dds): Rds Tds or Intermediate mentioning
confidence: 99%
“…It has been shown that the main parameter for the generation of geomagnetic storms is the Interplanetary magnetic field Bz (e.g. Tsurutani et al, 1990Tsurutani et al, , 1996Kamide, 1992;Gonzalez et al, 1994;Adebesin and Chukwuma, 2008), as the input of energy into the magnetosphere depends on the orientation and magnitude of the IMF Bz (Shweta et al, 2010). The intensity of a geomagnetic storm can be defined by the minimum Dst value (Gonzalez et al, 1994;Kamide et al, 1998a,b).…”
Section: Introductionmentioning
confidence: 99%