Report
The structure of mass-loading shocks
العنوان: | The structure of mass-loading shocks |
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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 |
تدمد: | 01480227 |
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