Results 21 to 30 of about 28,867 (162)

Methods of Orbit Clustering of Serviced Spacecraft

open access: yesSystem technologies, 2019
When planning orbital service operations, it is important to rationally divide a set of orbits serviced by a spacecraft into subsets (clusters) of orbits. This article proposes a technique for clustering the orbits of serviced spacecraft in the event of their servicing by a reusable service spacecraft with an electric rocket low thrust engine.
Anatolii Petrovych Alpatov   +1 more
openaire   +2 more sources

The Cluster spacecraft's view of the motion of the high-latitude magnetopause [PDF]

open access: yesAnnales Geophysicae
Abstract. The boundary between the interplanetary magnetic field and the terrestrial magnetic field is the magnetopause. This magnetopause is influenced by dynamic changes in the solar wind, that is different solar wind conditions lead to a change in the shape and location of the magnetopause.
N. Grimmich   +15 more
openaire   +6 more sources

Intermittent energy dissipation by turbulent reconnection [PDF]

open access: yes, 2016
Magnetic reconnection—the process responsible for many explosive phenomena in both nature and laboratory—is efficient at dissipating magnetic energy into particle energy.
André, M   +7 more
core   +1 more source

IMPALAS: Investigation of MagnetoPause Activity using Longitudinally-Aligned Satellites—a mission concept proposed for the ESA M3 2020/2022 launch [PDF]

open access: yes, 2012
The dayside magnetopause is the primary site of energy transfer from the solar wind into the magnetosphere, and modulates the activity observed within the magnetosphere itself.
Amm, O.   +19 more
core   +3 more sources

Modulation of NTC frequencies by Pc5 ULF pulsations : experimental test of the generation mechanism and magnetoseismology of the emitting surface [PDF]

open access: yes, 2009
Nonthermal continuum (NTC) radiation is believed to be emitted by the conversion of an electrostatic wave into an electromagnetic one, which takes place at the Earth's magnetic equator.
Anderson   +43 more
core   +2 more sources

On the estimation of the current density in space plasmas: multi versus single-point techniques

open access: yes, 2017
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.
Malara, Francesco   +4 more
core   +1 more source

Cluster observations of the midaltitude cusp under strong northward interplanetary magnetic field [PDF]

open access: yes, 2008
We report on a multispacecraft cusp observation lasting more than 100 min. We determine the cusp boundary motion and reveal the effect on the cusp size of the interplanetary magnetic field (IMF) changing from southward to northward.
Bogdanova, Y. V.   +5 more
core   +1 more source

In situ evidence for the structure of the magnetic null in a 3D reconnection event in the Earth's magnetotail [PDF]

open access: yes, 2006
Magnetic reconnection is one of the most important processes in astrophysical, space and laboratory plasmas. Identifying the structure around the point at which the magnetic field lines break and subsequently reform, known as the magnetic null point, is ...
A Balogh   +60 more
core   +2 more sources

Origin of the turbulent spectra in the high-altitude cusp: Cluster spacecraft observations [PDF]

open access: yesAnnales Geophysicae, 2006
Abstract. High-resolution magnetic field data from Cluster Flux Gate Magnetometer (FGM) and the Spatio-Temporal Analysis of Field Fluctuations (STAFF) instruments are used to study turbulent magnetic field fluctuations during the high-altitude cusp crossing on 17 March 2001.
Nykyri, K.   +8 more
openaire   +7 more sources

Correlation functions of small-scale fluctuations of the interplanetary magnetic field

open access: yes, 2010
The Interplanetary Magnetic Field shows complex spatial and temporal variations. Single spacecraft measurements reveal only a one dimensional section of this rich four dimensional phenomenon.
A. Balogh   +18 more
core   +1 more source

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