The structure of mass-loading shocks

التفاصيل البيبلوغرافية
العنوان: The structure of mass-loading shocks
المؤلفون: Zank, G. P, Khabibrakhmanov, I. KH, Story, T
المصدر: Journal of Geophysical Research. 98(A4)
بيانات النشر: United States: NASA Center for Aerospace Information (CASI), 1993.
سنة النشر: 1993
مصطلحات موضوعية: Astrophysics
الوصف: A new two-fluid model which describes mass loading in the solar wind (e.g., the interaction of the solar wind with a cometary coma or the local interstellar medium) is presented. The self-consistent back-reaction of the mass-loaded ions is included through their effective scattering in low-frequency MHD turbulence and the invocation of a diffusive approximation. Such an approximation has the advantage of introducing self-consistent dissipation coefficients into the governing equations, thereby facilitating the investigation of the internal structure of shocks in mass-loading environments. To illustrate the utility of the new model, we consider the structure of cometary shocks in the hypersonic one-dimensional limit, finding that the incoming solar wind is slowed by both mass loading and the development of a large cometary ion pressure gradient. The shock is broadened and smoothed by the cometary ions with a thickness of the order of the cometary ion diffusion scale.
نوع الوثيقة: Report
اللغة: English
تدمد: 0148-0227
URL الوصول: https://ntrs.nasa.gov/citations/19930049288
ملاحظات: NAGW-2076

NAGW-3116

NGT-40023

JPL-959167
رقم الانضمام: edsnas.19930049288
قاعدة البيانات: NASA Technical Reports