Search Publications

Automated Multi-Dataset Analysis (AMDA): An on-line database and analysis tool for heliospheric and planetary plasma data
DOI: 10.1016/j.pss.2021.105214 Bibcode: 2021P&SS..20105214G

André, N.; Fedorov, A.; Budnik, E. +27 more

Accessing, visualizing and analyzing heterogeneous plasma datasets has always been a tedious task that hindered students and senior researchers as well. Offering user friendly and versatile tools to perform basic research tasks is therefore pivotal for data centres including the Centre de Données de la Physique des Plasmas (CDPP http://www.cdpp.eu…

2021 Planetary and Space Science
Cluster 29
Science data visualization in planetary and heliospheric contexts with 3DView
DOI: 10.1016/j.pss.2017.07.007 Bibcode: 2018P&SS..150..111G

André, N.; Budnik, E.; Pitout, F. +21 more

We present a 3D orbit viewer application capable of displaying science data. 3DView, a web tool designed by the French Plasma Physics Data Center (CDPP) for the planetology and heliophysics community, has extended functionalities to render space physics data (observations and models alike) in their original 3D context. Time series, vectors, dynami…

2018 Planetary and Space Science
Cluster Ulysses 20
On the estimation of the current density in space plasmas: Multi- versus single-point techniques
DOI: 10.1016/j.pss.2017.03.008 Bibcode: 2017P&SS..140....6P

Sorriso-Valvo, Luca; Perri, Silvia; Malara, Francesco +2 more

Thanks to multi-spacecraft mission, it has recently been possible to directly estimate the current density in space plasmas, by using magnetic field time series from four satellites flying in a quasi perfect tetrahedron configuration. The technique developed, commonly called ;curlometer; permits a good estimation of the current density when the ma…

2017 Planetary and Space Science
Cluster 10
Isolated magnetic field structures in Mercury's magnetosheath as possible analogues for terrestrial magnetosheath plasmoids and jets
DOI: 10.1016/j.pss.2016.06.002 Bibcode: 2016P&SS..129...61K

Karlsson, Tomas; Raines, Jim M.; Liljeblad, Elisabet +3 more

We have investigated MESSENGER magnetic field data from the Mercury magnetosheath and near solar wind, to identify isolated magnetic field structures (defined as clear, isolated changes in the field magnitude). Their properties are studied in order to determine if they may be considered as analogues to plasmoids and jets known to exist in Earth's …

2016 Planetary and Space Science
Cluster 27
Origin of the backstreaming ions in a young Hot Flow Anomaly
DOI: 10.1016/j.pss.2016.08.003 Bibcode: 2016P&SS..131..102V

Vaisberg, O. L.; Shuvalov, S. D.; Shestakov, A. Yu. +1 more

We analyze an event in front of the bow shock observed by Cluster spacecraft on 22.02.2006. This event has many attributes of Hot Flow Anomaly at early stage of development including strong upstream beam and disturbed magnetic profile with increased magnetic field at one or two sides as observed by 4 Cluster spacecraft. The angle between the magne…

2016 Planetary and Space Science
Cluster 4
On the shape and motion of the Earth's bow shock
DOI: 10.1016/j.pss.2014.01.006 Bibcode: 2014P&SS...93....1M

Meziane, K.; Hamza, A. M.; Alrefay, T. Y.

Multipoint-measurements by the magnetic field Cluster-FGM (Flux Gate Magnetometer) are used to determine the local shock normal, and in turn allow the study of shock location shape and the velocity of the Earth's bow shock. The shock crossings cover orbits in which the spacecraft separation is of the order of ~600 km or less. A data selection of 1…

2014 Planetary and Space Science
Cluster 18
The occurrence of upstream waves in relation with the solar wind parameters: A statistical approach to estimate the size of the foreshock region
DOI: 10.1016/j.pss.2013.10.012 Bibcode: 2014P&SS...90..100R

Regi, M.; De Lauretis, M.; Francia, P.

We studied the occurrence of upstream waves in the foreshock region and their relationship with the solar wind and interplanetary magnetic field parameters. To this purpose, we developed a method for a careful identification of the upstream wave events. The results of the statistical analyses based on Cluster data (2003-2010 years) confirm that th…

2014 Planetary and Space Science
Cluster 12
Radial distribution of magnetic field in earth magnetotail current sheet
DOI: 10.1016/j.pss.2014.07.014 Bibcode: 2014P&SS..103..273R

Petrukovich, A. A.; Dunlop, M. W.; Baumjohann, W. +4 more

Knowing the magnetic field distribution in the magnetotail current sheet (CS) is essential for exploring magnetotail dynamics. In this study, using a joint dataset of Cluster/TC-1, the radial profile of the magnetic field in the magnetotail CS with radial distances covering 8<r<20RE under different geomagnetic activity states (i.e…

2014 Planetary and Space Science
Cluster 10
Turbulent dynamics inside the cavity of hot flow anomaly
DOI: 10.1016/j.pss.2014.01.001 Bibcode: 2014P&SS...92...24K

Dandouras, I.; Facskó, G.; Kovács, P.

In this paper the turbulent dynamics of a hot flow anomaly (HFA) event is investigated. The HFAs are transient plasma disturbances generated by the interaction of the bow shock (BS) and a tangential discontinuity (TD) embedded in the solar wind. The typical changes of the plasma parameters inside HFAs (increased plasma temperature, low bulk veloci…

2014 Planetary and Space Science
Cluster 10
The far magnetotail response to an interplanetary shock arrival
DOI: 10.1016/j.pss.2014.07.016 Bibcode: 2014P&SS..103..228G

Němeček, Z.; Šafránková, J.; Přech, L. +2 more

We present a study of the impact of the December 7, 2003 fast forward interplanetary (IP) shock on the distant tail of the Earth's magnetosphere. Using the data from the several spacecraft located in the solar wind/magnetosheath upstream to the Earth, we monitor a propagation of the IP shock from the L1 point to the magnetosphere. A behavior of th…

2014 Planetary and Space Science
Cluster 9