Studies of the magnetotail dynamics using VxO and web-base services.

Details Studies of the magnetotail dynamics using VxO and web-base services. Studies of the magnetotail dynamics using VxO and web-base services.

Dec 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011agufmsm13e..05j&link_type=abstract

American Geophysical Union, Fall Meeting 2011, abstract #SM13E-05

Physics

Plasma Physics

[7807] Space Plasma Physics / Charged Particle Motion And Acceleration, [7836] Space Plasma Physics / Mhd Waves And Instabilities, [7846] Space Plasma Physics / Plasma Energization

Scientific paper

It is well known that the magntetotail dynamics is very complex. The magnetotail is coupled to the interplanetary medium and the ionosphere which consist of highly varying limit conditions. Instabilities develop and propagate in the plasma sheet. Their effects result in numerous processes acting at various scales such as plamoids/TCR, BBF, plasma jets, energetic particle injections, electron beams, radio emission, ... The organisation of the sequence of the observed feature, i.e. their relation of causality require to analyse the data coming from all available observatories in space and on the ground. For identifying and characterising the process observed by each one, it is necessary to analyse in details the data obtained by several instruments. That means that generally a study of the magnetotail dynamics requires retrieving, accessing and analysing a large amount of data. Fortunatly, there are more and more web-based services making easier these tasks. In this presentation, we show results obtained by using web-based services for retrieving data (VSPO, HELIO, ...), accessing them (CAA, CDAWeb, CDPP, ...) and analyse them on line (TIPSOD, AMDA, CLWeb) in the context of magnetotail studies.

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