Saturn chorus intensity variations

Result code in IS VaVaI

<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F13%3A10191477" target="_blank" >RIV/00216208:11320/13:10191477 - isvavai.cz</a>

Alternative codes found

RIV/68378289:_____/13:00423076

Result on the web

<a href="http://dx.doi.org/10.1002/jgra.50529" target="_blank" >http://dx.doi.org/10.1002/jgra.50529</a>

DOI - Digital Object Identifier

<a href="http://dx.doi.org/10.1002/jgra.50529" target="_blank" >10.1002/jgra.50529</a>

Result language

angličtina

Original language name

Saturn chorus intensity variations

Original language description

Whistler mode chorus plasma wave emissions have been observed at Saturn near the magnetic equator and the source region. During crossings of the magnetic equator along nearly constant L shells, the Cassini Radio and Plasma Wave Science Investigation often observes a local decrease in whistler mode intensity and bandwidth closest to the magnetic equator, where linear growth appears to dominate, with nonlinear structures appearing at higher latitudes and higher frequencies. We investigate linear growth rate using the Waves in a Homogeneous, Anisotropic, Multi-component Plasma dispersion solver and locally observed electron phase space density measurements from the Electron Spectrometer sensor of the Cassini Plasma Spectrometer Investigation to determinethe parameters responsible for the variation in chorus intensity and bandwidth. We find that a temperature anisotropy (T-perpendicular to/T-parallel to similar to 1.3) can account for linear spatiotemporal growth rate of whistler mode wav

Czech name

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Czech description

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Type

J_x - Unclassified - Peer-reviewed scientific article (Jimp, Jsc and Jost)

CEP classification

BL - Plasma physics and discharge through gases

OECD FORD branch

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Project

Result was created during the realization of more than one project. More information in the Projects tab.

Continuities

I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year

2013

Confidentiality

S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

Name of the periodical

JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS

ISSN

2169-9380

e-ISSN

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Volume of the periodical

118

Issue of the periodical within the volume

9

Country of publishing house

US - UNITED STATES

Number of pages

11

Pages from-to

5592-5602

UT code for WoS article

000325483800018

EID of the result in the Scopus database

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