کد مقاله | کد نشریه | سال انتشار | مقاله انگلیسی | نسخه تمام متن |
---|---|---|---|---|
8134352 | 1523486 | 2018 | 7 صفحه PDF | دانلود رایگان |
عنوان انگلیسی مقاله ISI
Venus atmospheric structure and dynamics from the VEGA lander and balloons: New results and PDS archive
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کلمات کلیدی
موضوعات مرتبط
مهندسی و علوم پایه
علوم زمین و سیارات
علوم فضا و نجوم
پیش نمایش صفحه اول مقاله
![عکس صفحه اول مقاله: Venus atmospheric structure and dynamics from the VEGA lander and balloons: New results and PDS archive Venus atmospheric structure and dynamics from the VEGA lander and balloons: New results and PDS archive](/preview/png/8134352.png)
چکیده انگلیسی
The longest-lived in-situ measurement platforms at Venus have been the Soviet VEGA balloons in 1985 and the only high-quality pressure/temperature profile in the lowest 10â¯km of the atmosphere is that from the VEGA-2 lander. Here we review the mission and the resultant literature and report the archival of numerical data from these investigations on the NASA Planetary Data System Atmospheres Node to facilitate their access to the community. We additionally report some new results, including the striking absence of a signature of the planetary boundary layer in the near-surface potential temperature profile from the VEGA-2 lander, in contrast to the well-defined boundaries seen in a comparable profile at Titan.
ناشر
Database: Elsevier - ScienceDirect (ساینس دایرکت)
Journal: Icarus - Volume 305, 1 May 2018, Pages 277-283
Journal: Icarus - Volume 305, 1 May 2018, Pages 277-283
نویسندگان
Ralph D. Lorenz, David Crisp, Lyle Huber,