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Sökning: onr:"swepub:oai:DiVA.org:kth-16157" > Evidence of standin...

Evidence of standing waves during a Pi2 pulsation event observed on Cluster

Collier, Andrew (författare)
KTH,Rymd- och plasmafysik
Hughes, Arthur Robert W (författare)
University of KwaZulu-Natal, Durban, South Africa
Blomberg, Lars G. (författare)
KTH,Rymd- och plasmafysik
visa fler...
Sutcliffe, P. R. (författare)
visa färre...
 (creator_code:org_t)
2006-10-20
2006
Engelska.
Ingår i: Annales Geophysicae. - : Copernicus GmbH. - 0992-7689 .- 1432-0576. ; 24:10, s. 2719-2733
  • Tidskriftsartikel (refereegranskat)
Abstract Ämnesord
Stäng  
  • Observations of Pi2 pulsations at middle and low latitudes have been explained in terms of cavity mode resonances, whereas transients associated with field-aligned currents appear to be responsible for the high latitude Pi2 signature. Data from Cluster are used to study a Pi2 event observed at 18:09 UTC on 21 January 2003, when three of the satellites were within the plasmasphere (L=4.7,4.5 and 4.6) while the fourth was on the plasmapause or in the plasmatrough (L=6.6). Simultaneous pulsations at ground observatories and the injection of particles at geosynchronous orbit corroborate the occurrence of a substorm. Evidence of a cavity mode resonance is established by considering the phase relationship between the orthogonal electric and magnetic field components associated with radial and field-aligned standing waves. The relative phase between satellites located on either side of the geomagnetic equator indicates that the field-aligned oscillation is an odd harmonic. Finite azimuthal Poynting flux suggests that the cavity is effectively open ended and the azimuthal wave number is estimated as m similar to 13.5.

Ämnesord

NATURVETENSKAP  -- Fysik -- Fusion, plasma och rymdfysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Fusion, Plasma and Space Physics (hsv//eng)

Nyckelord

magnetospheric physics
MHD waves and instabilities
plasmasphere
storms and substorms
pi-2 pulsations
power spectra
magnetic pulsations
ulf pulsations
field-line
geomagnetic micropulsations
geosynchronous orbit
hydromagnetic-waves
inner magnetosphere
substorm onsets

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