C
C. C. Harvey
Researcher at Centre national de la recherche scientifique
Publications - 33
Citations - 2446
C. C. Harvey is an academic researcher from Centre national de la recherche scientifique. The author has contributed to research in topics: Magnetosheath & Solar wind. The author has an hindex of 18, co-authored 33 publications receiving 2370 citations.
Papers
More filters
Journal ArticleDOI
The Cassini Radio and Plasma Wave Investigation
Donald A. Gurnett,William S. Kurth,D. L. Kirchner,George Hospodarsky,T. F. Averkamp,P. Zarka,Alain Lecacheux,R. Manning,A. Roux,Patrick Canu,N. Cornilleau-Wehrlin,Patrick H. M. Galopeau,A. Meyer,Rolf Boström,Georg Gustafsson,Jan-Erik Wahlund,L. Åhlén,Helmut O. Rucker,H. P. Ladreiter,Wolfgang Macher,L. J. C. Woolliscroft,H. Alleyne,M. L. Kaiser,Michael D. Desch,William M. Farrell,C. C. Harvey,Philippe Louarn,Paul J. Kellogg,Keith Goetz,Arne Pedersen +29 more
TL;DR: The Cassini radio and plasma wave investigation is designed to study radio emissions, plasma waves, thermal plasma, and dust in the vicinity of Saturn as mentioned in this paper, which is the only spacecraft that can perform radio and plasmas measurements.
Journal ArticleDOI
Radio and plasma wave observations at Saturn from Cassini's approach and first orbit.
D. A. Gurnett,William S. Kurth,George Hospodarsky,A. M. Persoon,T. F. Averkamp,Baptiste Cecconi,Alain Lecacheux,P. Zarka,P. Canu,Nicole Cornilleau-Wehrlin,Patrick H. M. Galopeau,Aurélien Roux,C. C. Harvey,Philippe Louarn,Rolf Boström,Georg Gustafsson,Jan-Erik Wahlund,Michael D. Desch,William M. Farrell,M. L. Kaiser,Keith Goetz,Paul J. Kellogg,Georg Fischer,H. P. Ladreiter,Helmut O. Rucker,H. Alleyne,Arne Pedersen +26 more
TL;DR: Radio emissions from Saturn showed that the radio rotation period is now 10 hours 45 minutes 45 ± 36 seconds, about 6 minutes longer than measured by Voyager in 1980 to 1981, and many intense impulsive radio signals were detected from Saturn lightning during the approach and first orbit.
Journal ArticleDOI
Voyager 1 planetary radio astronomy observations near Jupiter
James W. Warwick,J. B. Pearce,A. C. Riddle,J. K. Alexander,Michael D. Desch,M. L. Kaiser,James R. Thieman,Thomas D. Carr,Samuel Gulkis,A. Boischot,C. C. Harvey,B. M. Pedersen +11 more
TL;DR: Results from the first low-frequency radio receiver to be transported into the Jupiter magnetosphere obtained dramatic new information, both because Voyager was near or in Jupiter's radio emission sources and also because it was outside the relatively dense solar wind plasma of the inner solar system.
Journal ArticleDOI
The Cluster Spatio-Temporal Analysis of Field Fluctuations (STAFF) Experiment
N. Cornilleau-Wehrlin,P. Chauveau,S. Louis,A. Meyer,J. M. Nappa,S. Perraut,Laurence Rezeau,P. Robert,A. Roux,C. de Villedary,Y. de Conchy,L. Friel,C. C. Harvey,D. Hubert,C. Lacombe,R. Manning,F. Wouters,François Lefeuvre,Michel Parrot,Jean-Louis Pinçon,B. Poirier,Wlodek Kofman,P. Louarn +22 more
TL;DR: The Spatio-Temporal Analysis of Field Fluctuations (STAFF) experiment is one of five experiments which together comprise the Wave Experiment Consortium (WEC). STAFF consists of a three-axis search coil magnetometer to measure magnetic fluctuations at frequencies up to 4 kHz, and a spectrum analyser to calculate in near-real time aboard the spacecraft, the complete auto- and cross-spectral matrices using the three magnetic and two electric components of the electromagnetic field as discussed by the authors.
Journal ArticleDOI
Early results from the Whisper instrument on Cluster: an overview
Pierrette Décréau,P. Fergeau,Vladimir Krasnoselskikh,E. Le Guirriec,M. Lévêque,Ph. Martin,Orélien Randriamboarison,Jean-Louis Rauch,F. X. Sené,H. C. Seran,Jean-Gabriel Trotignon,P. Canu,N. Cornilleau,H. de Feraudy,H. Alleyne,Keith H. Yearby,P. B. Mögensen,Georg Gustafsson,Mats André,D. Gurnett,Fabien Darrouzet,J. Lemaire,C. C. Harvey,Pavel M. Trávníček +23 more
TL;DR: In this article, the Whisper instrument yields two data sets: (i) the electron density determined via the relaxation sounder, and (ii) the spectrum of natural plasma emissions in the frequency band 2-80 kHz.