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Titel Low frequency instabilities based on electron and ion temperature anisotropies with generalized (r,q) distribution function
VerfasserIn Muhammad Nouman Sarwar Qureshi, Sundas Saeed, Roberto Bruno
Konferenz EGU General Assembly 2016
Medientyp Artikel
Sprache en
Digitales Dokument PDF
Erschienen In: GRA - Volume 18 (2016)
Datensatznummer 250124506
Publikation (Nr.) Volltext-Dokument vorhandenEGU/EGU2016-3952.pdf
 
Zusammenfassung
In this study we first observe Alfven waves in the solar wind using CLUSTER data and then analyze the ion distributions for the same time interval. We then fit the observed ion distributions using the generalized (r,q) distribution function which is the generalized form of kappa and Maxwellian distribution functions and apply this distribution to study the Alfven cyclotron instability using both the ion and electron temperature anisotropies for the first time, based on the observed parameters from the solar wind as well as from downstream region of bow shock. We studied the role of electron to ion temperature ratios and found that by increasing the anisotropy ratio T_(⊥e)/T_(∥i) growth rate of Alfven cyclotron instability decreases whereas by increasing the ratio T_(∥e)/T_(∥i) growth rate increases. We also found that left-hand circularly polarized wave becomes unstable not only when T_(⊥i)>T_(∥i) as reported in the literature but also for T_(⊥i)<T_(∥i). Theoretical values of frequency and growth rates are then compared with Maxwellian results as well as with the observations and found in good agreement with the data.