2009 Workshop:Meteors and the Upper Atmosphere

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Meteors and the Upper Atmosphere

Zia, 1300-1500, 30 June 2009

Conveners

Lars Dyrud
Diego Janches

Workshop Categories

Altitudes: MLT - Latitudes: global - Inst/Model: radar - Other: and modeling and optical

Agenda of the Workshop

Panel and Short Presentations

PANEL

 Panel members will be given a few minutes prior to panel discussion
 to introduce their results and the topic relating to Radar Observations of Non-uniform/non-smooth
 Signal to Noise Ratio (SNR) Meteor Head Echoes, and what these observations can teach us about meteoroids and the deposition
 of metals in the upper atmosphere.
 
 Panel Members:
 John Plane
 John Mathews
 Koki Chau: Jicamarca examples of meteor ablation and fragmentation
 Meers Oppenheim
 

SHORT PRESENTATIONS

 Speakers:
 
 Diego Janches Observation of Differential ablation
 Jonathan Fentzke* Meteoric Smoke Particles Observed with Arecibo
 Jonathon Sparks* Temporal and Geographical variability of the meteor altitude distribution
 Elizabeth Bass*
 Julio Urbina  The Nittany Meteor Radar: Current Status
 Laura Vertatschitsch* Polarization Properties of Meteor Head Echoes
 Jason Hinrichs* Global modeling of the variability of non-specular meteor trails
 Eli Hibit* Modeling and radar observations of mid-latitude non-specular meteors
 Lars Dyrud  Differential Ablation and non-specular meteor trails
 Siming Zhao*  On the role of geomagnetic field in meteor detection
 Akshay Malhotra*
 Meers Oppenheim   The 3D evolution of meteor plasma: Fully kinetic simulation results
 Joe Grebowsky GOME measurements of Neutral and ionized Mg and Fe
 Ingemar Hagsstroem  Eiscat Meteor Observations
 * indicates student speaker

Estimated attendance

50-80

Special technology requests

none

Description

Every year approximately 100,000 tons of meteoric material impacts Earth's atmosphere near 100 km altitude. However, many questions remain on this meteor mass and energy flux and the impact of this flux on upper atmospheric chemistry and ionization. For example, global yearly mass flux estimates are not constrained to within an order of magnitude. Of particular importance to the CEDAR community is that meteors account for all of the dust, metal neutral and ionized particles in the upper atmosphere (since there is no convection or diffusion of atoms or particles of this size from the ground all the way to 100 km). Further, meteoric dust is also thought to provide the condensation nuclei for polar mesospheric clouds PMC (high altitude clouds near 80 km), which is the focuses of a current NASA mission (AIM). Yet it remains unclear whether variability in meteor flux generates variability in PMC occurrence. Additionally, CEDAR researchers have used radar reflections from meteor trails to remotely sense winds and temperatures near the mesopause (a very difficult place to take meausurements, too high for lidar to low for fabry-perot measurements). With some success for winds but little success for temperatures. To address these issues, we invite presentations on the physics of meteors and their interaction with the atmosphere and ionosphere. Specific discussion is encouraged on the observation of meteors with NSF and CEDAR supported facilities, or the theoretical interpretation of such observations.


We encourage contributions of research attempting to better understand meteors or general aeronomy via meteor observations, including upper atmospheric chemistry and metal layers. We also invite presentations of radar, Lidar and optical observations. Theoretical studies or simulations of the meteors and meteor trail interactions with the atmosphere/ionosphere are also invited.

This year we will also hold a panel discussion on the following topic. "Differential ablation or fragmentation: how do we make sense of non-smooth radar “light curves”?"

This topic has been the result of a number of recent papers, and disagreement between different researchers. We look forward to a very interesting discussion amongst panel members and would also encourage all those that are interested to attend, and those that have data or ideas on the subject are welcome and encouraged to participate in the discussion.

Workshop Summary

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