Linear analysis of bump on tail instability with non-Maxwellian distribution function
The growth rate of bump on tail instability propagating in unmagnetized plasma has been derived. The dispersion relation has been characterized for (r, q) distribution function with spectral indices r and q which ultimately contributes towards tails and shoulder of distribution function. The growt...
Saved in:
Main Authors: | Noreen, N, Shiekh, A, Habumugisha, I, Zaheer, S, AShah, H |
---|---|
Format: | Article |
Language: | en_US |
Published: |
IOP Publishing
2020
|
Subjects: | |
Online Access: | http://hdl.handle.net/20.500.12493/420 |
Tags: |
Add Tag
No Tags, Be the first to tag this record!
|
Similar Items
-
Differentiating the Acceleration Mechanisms in the Slow and Alfvénic Slow Solar Wind
by: Yeimy J. Rivera, et al.
Published: (2025-01-01) -
Baroclinic instability from an experimental perspective
by: Harlander, Uwe, et al.
Published: (2024-09-01) -
Clinical outcomes and long-term efficacy of high tibial osteotomy in treating knee instability: An updated systematic review
by: Mustamsir Edi, et al.
Published: (2025-01-01) -
Exploring the Complex Heliotail Boundary by an Extended Level Set Approach
by: C. Onubogu, et al.
Published: (2025-01-01) -
Propagation of Interplanetary Shocks in the Inner Heliosphere
by: Munkhjargal Lkhagvadorj, et al.
Published: (2025-01-01)