Results 31 to 40 of about 4,343 (197)
Planar magnetic structures in coronal mass ejection-driven sheath regions [PDF]
Planar magnetic structures (PMSs) are periods in the solar wind during which interplanetary magnetic field vectors are nearly parallel to a single plane.
E. Palmerio +3 more
doaj +1 more source
Sub-ion-gyro scale magnetic field compressions generated by the solar wind interaction with the moon
Short-period magnetic enhancements were detected by the MAP-LMAG magnetometer onboard Kaguya orbiting the moon in the solar wind at an altitude of 100 km.
Tomoko Nakagawa +3 more
doaj +1 more source
Cluster observes the Earth’s magnetopause: coordinated four-point magnetic field measurements [PDF]
The four-spacecraft Cluster mission has provided high-time resolution measurements of the magnetic field from closely maintained separation distances (200–600 km).
M. W. Dunlop +7 more
doaj +1 more source
CLUSTER encounters with the high altitude cusp: boundary structure and magnetic field depletions [PDF]
Data from the four spacecraft Cluster mission during a high altitude cusp crossing on 13 February 2001 are presented. The spacecraft configuration has one leading spacecraft, with the three trailing spacecraft lying in a plane that corresponds roughly
P. J. Cargill +9 more
doaj +1 more source
Martian Atmospheric Loss Through Foreshock Transient Events
Abstract At Mars, the MAVEN spacecraft has made observations of Hot Flow Anomalies (HFAs) in the foreshock. Due to the bow shock's proximity to the planet, it is theorized that HFAs contribute to atmospheric escape at Mars through the excavation of ionospheric ions.
Alexandros C. Cooke‐Politikos +5 more
wiley +1 more source
Computational aspects of multilevel trajectory optimization [PDF]
This paper presents new computational results in multilevel trajectory optimization. The original formulation of trajectory decomposition is extended and applied to a difficult multiple arc trajectory example, the low thrust interplanetary swingby ...
Stubberud, Allen, Sugar, RD
core
On the probability distribution function of small scale interplanetary magnetic field fluctuations [PDF]
In spite of a large number of papers dedicated to study MHD turbulence in the solar wind there are still some simple questions which have never been sufficiently addressed like: a)do we really know how the magnetic field vector orientation fluctuates in ...
Bavassano, B. +6 more
core +4 more sources
The relationship between interplanetary discontinuities and Alfvén waves: Ulysses observations
The rate of occurrence of interplanetary discontinuities (ROID) is examined using Ulysses magnetic field and plasma data from 1 to 5 AU radial distance from the Sun and at high heliographic latitudes. We find two regions where the ROID is high: in stream‐stream interaction regions and in Alfvén wave trains.
B. T. Tsurutani +9 more
openaire +1 more source
Abstract Hot and tenuous plasmas have velocity distribution functions (VDFs) significantly different from Maxwellian distributions. Characterizing how these differences impact wave damping and emission necessitates sophisticated methods for determining the associated dielectric plasma response.
K. G. Klein +8 more
wiley +1 more source
It has been widely recognized that the minimum variance analysis of magnetic fields (MVAB) often fails to accurately predict the direction normal to a discontinuity or current sheet, compared with multiple-spacecraft methods.
Wai-Leong Teh
doaj +1 more source

