Search Publications
Systematic analysis of equatorial noise below the lower hybrid frequency
Santolík, O.; Cornilleau-Wehrlin, N.; Macúšová, E. +3 more
Available from http://www.copernicus.org/site/EGU/annales/22/7/2587.htm?FrameEngine=false;
Isolated electrostatic structures observed throughout the Cluster orbit: relationship to magnetic field strength
Balogh, A.; Santolík, O.; Chen, L. +4 more
Available from http://www.copernicus.org/site/EGU/annales/22/7/2515.htm?FrameEngine=false;
Cluster observations of continuous reconnection at the magnetopause under steady interplanetary magnetic field conditions
Balogh, A.; Klecker, B.; Rème, H. +9 more
Available from http://www.copernicus.org/site/EGU/annales/22/7/2355.htm?FrameEngine=false;
Evolutionary signatures in complex ejecta and their driven shocks
Farrugia, C.; Berdichevsky, D.
We examine interplanetary signatures of ejecta-ejecta interactions. To this end, two time intervals of inner-heliospheric (≤1AU) observations separated by 2 solar cycles are chosen where ejecta/magnetic clouds are in the process of interacting to form complex ejecta. At the Sun, both intervals are characterized by many coronal mass ejections (CMEs…
Multipoint investigation of the source region of storm-time chorus
Santolík, O.; Gurnett, D.; Pickett, J.
Available from http://www.copernicus.org/site/EGU/annales/22/7/2555.htm?FrameEngine=false;
Reconstruction of two-dimensional magnetopause structures from Cluster observations: verification of method
Balogh, A.; Dandouras, I.; Lavraud, B. +7 more
Available from http://www.copernicus.org/site/EGU/annales/22/4/1251.htm?FrameEngine=false;
Four-spacecraft determination of magnetopause orientation, motion and thickness: comparison with results from single-spacecraft methods
Balogh, A.; Klecker, B.; Vaivads, A. +9 more
Available from http://www.copernicus.org/site/EGU/annales/22/4/1347.htm?FrameEngine=false;
Predictions of the arrival time of Coronal Mass Ejections at 1AU: an analysis of the causes of errors
Cargill, P.; Owens, M.
. Three existing models of Interplanetary Coronal Mass Ejection (ICME) transit between the Sun and the Earth are compared to coronagraph and in situ observations: all three models are found to perform with a similar level of accuracy (i.e. an average error between observed and predicted 1AU transit times of approximately 11h). To improve long-term…
Magnetic turbulent spectra in the magnetosheath: new insights
Balogh, A.; Belmont, G.; Sahraoui, F. +4 more
Available from http://www.copernicus.org/site/EGU/annales/22/6/2283.htm?FrameEngine=false;
On the origin of field-aligned beams at the quasi-perpendicular bow shock: multi-spacecraft observations by Cluster
Balogh, A.; Kistler, L.; Kucharek, H. +6 more
Available from http://www.copernicus.org/site/EGU/annales/22/7/2301.htm?FrameEngine=false;