SSD - TR - 67 - 95 TR - 100 l ( 2240 - 20 ) - 11 1 * 1 , 00 00 * o CO ^ ? Microwave Breakdown of the Reentry Boundary Layer

نویسندگان

  • BLANK PAGES
  • C. J. Lenander
چکیده

Measurements of the microwave power required for breakdown have been made in a simulated reentry boundary layer flow. By establishing a fully developed laminar pipe flow between cold walls, fed by a subsonic arc jet, we have simulated the appropriate boundary layer temperature, density, electron concentration, and chemical composition profiles over an altitude range from 80 to 180 kft. Correlation with existing theoretical models and comparison with recent hot-air breakdown measurements in shock tubes are made. The effects of chemical composition of hot air and of typical ablation products and quenchants upon breakdown are briefly explored. It is found that significant reduction in breakdown power occurs in hot air flows and that present theoretical models do not predict the high altitude breakdown power within a factor of three or more.

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Report on Course Popularity

AS TR 6 33 A st ro ph ys ic al T ec hn iq ue s 70 30 6 3. 00 00 1 AC TI VE 0 20 0 0 0 20 0% 0% TB A to T BA lo ca tio n IF A C 22 1 (M ax R m . c ap ac ity 3 0) (I ns tr: J H en ry ) L ec tu re /D ic us si on AS TR 6 99 D ire ct ed R es ea rc h 70 30 7 1. 00 00 1 AC TI VE 0 25 0 0 0 25 0% 0% TB A to T BA lo ca tio n TB A TB A (M ax R m . c ap ac ity 9 99 ) ( In st r: Jo sh ua B ar ne s) D ire c...

متن کامل

A Dynamic Atomistic-continuum Method for the Simulation of Crystalline Materials

X iv :c on dm at /0 11 21 73 v1 [ co nd -m at .m tr lsc i] 1 0 D ec 2 00 1 A Dynamic Atomistic-Continuum Method for the Simulation of Crystalline Materials 1 Weinan E∗† and Zhongyi Huang∗‡ ∗ Department of Mathematics and PACM, Princeton University, Princeton, NJ 08544 † School of Mathematics, Peking University, Beijing, 100866, China ‡ Department of Mathematical Sciences, Tsinghua University, B...

متن کامل

ar X iv : 0 81 1 . 21 76 v 2 [ as tr o - ph ] 6 D ec 2 00 9 Non - Gaussian Signatures from the Postinflationary Early Universe

We consider contributions to non-Gaussianity of the Cosmic Microwave Background (CMB) from remnants of phase transitions in the very early universe. Such signatures can optimistically be used to discover evidence of new particle physics through cosmological observations. More conservatively they may provide an obstacle to extracting information about the non-Gaussian nature of primordial densit...

متن کامل

ar X iv : 0 81 0 . 43 71 v 1 [ as tr o - ph ] 2 4 O ct 2 00 8 Welcome back , Polaris the Cepheid

For about 100 years the amplitude of the 4 d pulsation in Polaris has decreased. We present new results showing a significant increase in the amplitude based on 4.5 years of continuous monitoring from the ground and with two satellite missions.

متن کامل

RTES-04 Time & Space.indd

Ep h em er is T im e ET 1 19 67 : c o rr ec ti o n s to th e ET 0 m o d el Ep h em er is T im e ET 2 19 72 : c o rr ec ti o n s to th e ET 1 m o d el ‘1 s ec o n d ’ • 1 / 8 6, 40 0 o f a m ea n s o la r d ay . • 1 / 3 1, 56 6, 92 5. 97 47 o f t h e tr o p ic al y ea r fo r 19 00 (E p h em er is T im e as d efi n ed in 1 95 5) . • 9, 19 2, 63 1, 77 0 p er io d s o f t h e ra d ia ti o n c o rr ...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2012