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Observed field in the IC 348 cluster

Evidence of Transverse Magnetospheric Field Line Oscillations as Observed from Cluster and Ground Magnetometers

Evidence of Transverse Magnetospheric Field Line Oscillations as Observed from Cluster and Ground Magnetometers

... from Cluster combined with ground observation that sup- ports the theory of field line ...like Cluster provides a unique opportunity of detecting these field line oscillations because it ...

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Source location of chorus emissions observed by Cluster

Source location of chorus emissions observed by Cluster

... magnetic field as a function of frequency and of time. Due to the Cluster orbit, chorus emissions are often observed close to perigee, and the data analysis determines the direction of these ...

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Anomalous foreshock field-aligned beams observed by Cluster

Anomalous foreshock field-aligned beams observed by Cluster

... magnetic field components, which ap- pear after ∼14:06:30 UT and last a few ...the field perturbations (λ 1 > λ 2 > λ 3 ) (maximum, intermedi- ate and minimum variances, ...ambient field B 0 computed ...

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Characteristics of magnetospherically reflected chorus waves observed by CLUSTER

Characteristics of magnetospherically reflected chorus waves observed by CLUSTER

... often observed by the STAFF spectrum analyser on board the 4 satellites of CLUS- ...waves observed on the magnetic and electric power ...been observed that lower in- tensity waves propagate toward ...

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Solitary potential structures observed in the magnetosheath by the Cluster spacecraft

Solitary potential structures observed in the magnetosheath by the Cluster spacecraft

... magnetic field data from multi-Cluster spacecraft, should provide us with the first opportunity to de- termine experimentally the generation mechanism, propaga- tion, growth, and decay properties of these ...

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Wave-particle interaction in a plasmaspheric plume observed by a Cluster satellite

Wave-particle interaction in a plasmaspheric plume observed by a Cluster satellite

... means that cold He + ions in the plasmaspheric plume have a strong influence on the generation of EMIC waves in the equatorial plane. In the frequency range denoted by two vertical solid lines, the COMP component is much ...

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Ion multi-nose structures observed by Cluster in the inner Magnetosphere

Ion multi-nose structures observed by Cluster in the inner Magnetosphere

... the observed one and its energy width is much ...electric field model, the distribution function of the source plays a crucial role in the features observed at the Cluster ...

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Scale sizes of intense auroral electric fields observed by Cluster

Scale sizes of intense auroral electric fields observed by Cluster

... electric field scale ...electric field magnitudes are typically larger (as seen in ...electric field scale size increased as ...electric field scale sizes in the downward current region are ...

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On the generation of solitary waves observed by Cluster in the near-Earth magnetosheath

On the generation of solitary waves observed by Cluster in the near-Earth magnetosheath

... involving Cluster waveform observations, solitary waves in the form of bipolar and tripo- lar pulses have recently been found to be quite abundant in the near-Earth dayside ...using Cluster waveform ...be ...

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Transients in oxygen outflow above the polar cap as observed by the Cluster spacecraft

Transients in oxygen outflow above the polar cap as observed by the Cluster spacecraft

... same field-line we may see fronts approaching along the field line rather than drifting with ...the field-line according to their parallel ...assumption. Field-aligned flow will create a ...

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Evidence of standing waves during a Pi2 pulsation event observed on Cluster

Evidence of standing waves during a Pi2 pulsation event observed on Cluster

... C4 V Fig. 3: EFW probe potential on 21 January 2003. data are not available in MFA coordinates for C3 during the event since the background magnetic field direction was passing through the spin plane of the ...

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Plasma flow channels with ULF waves observed by Cluster and Double Star

Plasma flow channels with ULF waves observed by Cluster and Double Star

... Baumjohann, W. and Glassmeier, K.-H.: The transient response mechanism and pi2 pulsations at substorm onset-review and out- look, Planet. Space Sci., 11, 1361–1370, 1984. Carr, C., Brown, P., Zhang, T. L., Gloag, J., ...

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Magnetotail dipolarization and associated current systems observed by Cluster and Double Star

Magnetotail dipolarization and associated current systems observed by Cluster and Double Star

... using Cluster, Double Star TC1, and ground-based observations. The Cluster spacecraft are located approximately 16 R E downtail near 0030 ...by field-aligned currents, which in their turn generate ...

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Solitary waves observed in the auroral zone: the Cluster multi-spacecraft perspective

Solitary waves observed in the auroral zone: the Cluster multi-spacecraft perspective

... Assuming this to be this case, we obtain a velocity of the tripolar solitary waves of several hundred to a few thousand km/s, which is on the order of the average propagation speed associated with the bipolar solitary ...

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Equatorial magnetosonic waves observed by cluster satellites: the Chirikov resonance overlap criterion

Equatorial magnetosonic waves observed by cluster satellites: the Chirikov resonance overlap criterion

... magnetic field since they are highly elliptical in nature and the wave magnetic field oscillates parallel to the external ...emissions observed in this ...wave observed in this particular ...

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Kinetic structure and wave properties associated with sharp dipolarization front observed by Cluster

Kinetic structure and wave properties associated with sharp dipolarization front observed by Cluster

... not observed during a storm-time, so the heavy ion species, such as O + , He + and He ++ , are ten- ...electromagnetic field is transferred to plasma thermal and kinetic energy, ...

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Occurrence and location of concentrated load and generator regions observed by Cluster in the plasma sheet

Occurrence and location of concentrated load and generator regions observed by Cluster in the plasma sheet

... | E y J y /E·J |∼1, i.e., E y J y dominates the power density both for CLRs and CGRs (and also for the RAND data). It is well known that the plasma sheet on the average be- haves as a load due to the large scale ...

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Magnetic clouds’ structure in the magnetosheath as observed by Cluster and Geotail: four case studies

Magnetic clouds’ structure in the magnetosheath as observed by Cluster and Geotail: four case studies

... as observed in the upstream solar ...magnetic field strength and direc- ...the Cluster and Geotail spacecraft in- side the magnetosheath and from the Advanced Composition Explorer (ACE) upstream of ...

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The magnetic structure of an earthward-moving flux rope observed by Cluster in the near-tail

The magnetic structure of an earthward-moving flux rope observed by Cluster in the near-tail

... core field, which exists inside the flux rope, we can infer that the magnetic flux rope is produced by component reconnection, because anti-parallel reconnection cannot produce a magnetic struc- ture containing a ...

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The spectacular cluster chain Abell 781 as observed with LOFAR, GMRT, and XMM-Newton

The spectacular cluster chain Abell 781 as observed with LOFAR, GMRT, and XMM-Newton

... Key words. radiation mechanisms: non-thermal – radiation mechanisms: thermal – galaxies: clusters: general – galaxies: clusters: individual: A781 – galaxies: clusters: intracluster medium – radio continuum: general 1. ...

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