کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
8142979 | 1523921 | 2015 | 14 صفحه PDF | دانلود رایگان |
عنوان انگلیسی مقاله ISI
Modeling the total dust production of Enceladus from stochastic charge equilibrium and simulations
ترجمه فارسی عنوان
مدل سازی کل تولید گرد و غبار انسلادوس از تعادل بار احتمالی و شبیه سازی
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کلمات کلیدی
موضوعات مرتبط
مهندسی و علوم پایه
علوم زمین و سیارات
فیزیک زمین (ژئو فیزیک)
چکیده انگلیسی
Negatively and positively charged nano-sized ice grains were detected in the Enceladus plume by the Cassini Plasma Spectrometer (CAPS). However, no data for uncharged grains, and thus for the total amount of dust, are available. In this paper we estimate this population of uncharged grains based on a model of stochastic charging in thermodynamic equilibrium and on the assumption of quasi-neutrality in the plasma-dust system. This estimation is improved upon by combining simulations of the dust component of the plume and simulations for the plasma environment into one self-consistent model. Calibration of this model with CAPS data provides a total dust production rate of about 12 kg sâ1, including larger dust grains up to a few microns in size. We find that the fraction of charged grains dominates over that of the uncharged grains. Moreover, our model reproduces densities of both negatively and positively charged nanograins measured by Cassini CAPS. In Enceladus׳ plume ion densities up to ~104cmâ3 are required by the self-consistent model, resulting in an electron depletion of about 50% in the plasma, because electrons are attached to the negatively charged nanograins. These ion densities correspond to effective ionization rates of about 10â7sâ1, which are about two orders of magnitude higher than expected.
ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Planetary and Space Science - Volume 119, 15 December 2015, Pages 208-221
Journal: Planetary and Space Science - Volume 119, 15 December 2015, Pages 208-221
نویسندگان
Patrick Meier, Uwe Motschmann, Jürgen Schmidt, Frank Spahn, Thomas W. Hill, Yaxue Dong, Geraint H. Jones, Hendrik Kriegel,