Remote sensing space weather events: the AARDDVARK network

Abstract. The Antarctic-Arctic Radiation-belt (Dynamic) Deposition- VLF Atmospheric Research Konsortium (AARDDVARK) provides a network of continuous long-range observations of the lower-ionosphere in the polar regions. Our ultimate aim is to develop the network of sensors to detect changes in ioniza...

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Bibliographic Details
Main Authors: Mark A. Clilverd, Craig J. Rodger, Neil R Thomson, James B. Brundell, Pekka T. Verronen, Esa Turunen
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Subjects:
Antarctic
Arctic
New Zealand
The Antarctic
Antarc*
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.490.8182
http://www.physics.otago.ac.nz/space/2008SW000412-pip.pdf
Description
Summary:Abstract. The Antarctic-Arctic Radiation-belt (Dynamic) Deposition- VLF Atmospheric Research Konsortium (AARDDVARK) provides a network of continuous long-range observations of the lower-ionosphere in the polar regions. Our ultimate aim is to develop the network of sensors to detect changes in ionization levels from ~30-90 km altitude, globally, continuously, and with high time resolution, with the goal of increasing the understanding of energy coupling between the Earth's atmosphere, the Sun, and space. This science area impacts our knowledge of space weather processes, global atmospheric change, communications, and navigation. The joint New Zealand-United Kingdom AARDDVARK is a new extension of a well-established experimental technique, allowing long-range probing of ionization changes at comparatively low altitudes. Most other instruments which can probe the same altitudes are limited to essentially overhead measurements. At this stage AARDDVARK is essentially unique, as similar systems are only deployed at a regional level. The AARDDVARK network has contributed to the scientific understanding of a growing list of space weather science topics including solar proton events, the descent of NOx into the middle atmosphere, substorms, precipitation of energetic electrons by plasmaspheric hiss and EMIC waves, the impact of coronal mass ejections upon the radiation belts, and relativistic electron microbursts. Future additions to the receiver network will increase the science potential and provide global coverage of space weather event signatures.

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