[HTML][HTML] Polarization dependency of transverse scattering and collisional coupling to the ambient atmosphere from meteor trails—Theory and observations
G Stober, R Weryk, D Janches, ECM Dawkins… - Planetary and Space …, 2023 - Elsevier
Quantitative analyses of transverse scatter meteors to derive physically consistent solutions
of the ambipolar diffusion coefficient, electron line density, and initial trail radius have been …
of the ambipolar diffusion coefficient, electron line density, and initial trail radius have been …
Modelling the entry of meteoroids
O Popova, J Borovicka… - Meteoroids. Sources of …, 2019 - cambridge.org
Meteoroids represent the material remaining from the formation of the solar system and carry
unique information on the earliest forming solids. They enable the study of the structure and …
unique information on the earliest forming solids. They enable the study of the structure and …
The Local Time and Altitude Dependences of Long‐Lived Nonspecular Meteor Echoes With Weak Magnetic Aspect Sensitivity at Low Latitudes
Long‐lived nonspecular meteor echoes backscattered from meteor trail nonfield‐aligned
irregularities (NFAIs) were observed sporadically at high latitudes. In this study, we employ …
irregularities (NFAIs) were observed sporadically at high latitudes. In this study, we employ …
Formation of plasma around a small meteoroid: 1. Kinetic theory
YS Dimant, MM Oppenheim - Journal of Geophysical Research …, 2017 - Wiley Online Library
Every second, millions of submilligram meteoroids enter the Earth's atmosphere producing
dense plasmas. Radars easily detect these plasmas, and researchers use this data to …
dense plasmas. Radars easily detect these plasmas, and researchers use this data to …
First 3‐D simulations of meteor plasma dynamics and turbulence
MM Oppenheim, YS Dimant - Geophysical Research Letters, 2015 - Wiley Online Library
Millions of small but detectable meteors hit the Earth's atmosphere every second, creating
trails of hot plasma that turbulently diffuse into the background atmosphere. For over 60 …
trails of hot plasma that turbulently diffuse into the background atmosphere. For over 60 …
Nonspecular meteor trail altitude distributions and durations observed by a 50 MHz high‐power radar
G Sugar, MM Oppenheim, E Bass… - Journal of Geophysical …, 2010 - Wiley Online Library
High‐power large‐aperture (HPLA) radars frequently observe nonspecular meteor trail
echoes that result from plasma turbulence driven by the intense pressure gradients on the …
echoes that result from plasma turbulence driven by the intense pressure gradients on the …
A radio science perspective on long‐duration meteor trails
A Malhotra, JD Mathews… - Journal of Geophysical …, 2007 - Wiley Online Library
Nonclassical radar meteor echoes or range spread trail echoes (RSTEs), lasting from tens of
seconds to over 15 min, have been a subject of considerable interest and speculation in the …
seconds to over 15 min, have been a subject of considerable interest and speculation in the …
On the validity of the ambipolar diffusion assumption in the polar mesopause region
AP Ballinger, PB Chilson, RD Palmer… - Annales …, 2008 - angeo.copernicus.org
The decay of underdense meteor trails in the polar mesopause region is thought to be
predominantly due to ambipolar diffusion, a process governed by the ambient temperature …
predominantly due to ambipolar diffusion, a process governed by the ambient temperature …
Day to night variation in meteor trail measurements: Evidence for a new theory of plasma trail evolution
MM Oppenheim, G Sugar, E Bass… - Geophysical …, 2008 - Wiley Online Library
A recent theory of meteor trail plasma diffusion made the prediction that meteors will
generate more and longer lasting non‐specular echoes at night than during the day. This …
generate more and longer lasting non‐specular echoes at night than during the day. This …
Ionospheric irregularities: frontiers
There are several thermosphere ionosphere models with bottom boundaries somewhere in
the middle atmosphere. Achieving a true whole atmosphere modeling capability requires the …
the middle atmosphere. Achieving a true whole atmosphere modeling capability requires the …