Results 61 to 70 of about 588 (209)

Hybrid Kinetic Modeling of the Magnetosheath Impulsive Plasma Cloud Penetration Through the Magnetopause and Comparison With MMS and Other Spacecraft Observations

open access: yesJournal of Geophysical Research: Space Physics, Volume 129, Issue 7, July 2024.
Abstract This research examines the plasma processes under penetration of the plasma clouds (plasmoids) across the magnetopause which is modeled as a tangential discontinuity (TD). Cases with the parallel magnetic field in both sides out of the TD are under investigation.
A. S. Lipatov   +3 more
wiley   +1 more source

ON COSMIC RAY MODULATION BEYOND THE HELIOPAUSE: WHERE IS THE MODULATION BOUNDARY? [PDF]

open access: yes, 2011
Two of the paradigms in modeling the transport of galactic cosmic rays are that the modulation boundary is the heliopause and that the local interstellar spectra are identical to the galactic cosmic ray spectra.
Strauss, R.D.   +10 more
core   +2 more sources

The Shape of the Heliosphere Derived from the IBEX Ribbon

open access: yesThe Astrophysical Journal Letters
The shape of the heliosphere remains largely uncertain due to the lack of in situ measurements. However, the energetic neutral atom (ENA) ribbon structure discovered by the Interstellar Boundary EXplorer (IBEX) satellite provides a new perspective.
Shuai Zhang   +4 more
doaj   +1 more source

A Numerical Model for the Dynamics of Pickup Ions Outside the Heliopause and IBEX “Ribbon” Observation

open access: yesThe Astrophysical Journal
The leading mechanism for the origin of the Interstellar Boundary Explorer (IBEX) “ribbon” of enhanced energetic neutral atoms (ENAs) from the outer heliosphere is the so-called secondary ENA process.
Yifan Huang   +6 more
doaj   +1 more source

The Characterization of Secondary Interstellar Neutral Oxygen beyond the Heliopause: A Detailed Analysis of the IBEX-Lo Oxygen Observations [PDF]

open access: yes, 2019
In this study, we analyze the directional distribution of the secondary interstellar neutral (ISN) O population observed by the IBEX-Lo neutral atom camera on the Interstellar Boundary EXplorer (IBEX) via the comparison with simulated ISN O intensity ...
Schwadron, Nathan A.   +8 more
core   +1 more source

Cosmic ray transport near the heliopause [PDF]

open access: yesJournal of Physics: Conference Series, 2015
In this paper we summarize our modelling efforts for cosmic rays near the heliopause, and discuss whether galactic cosmic ray modulation beyond the heliopause is possible and present an explanation for the anisotropic nature of the observed cosmic ray intensities in the very local interstellar medium.
R D Strauss   +4 more
openaire   +1 more source

Solar sail science mission applications and advancement : solar sailing: concepts, technology, missions [PDF]

open access: yes, 2011
Solar sailing has long been envisaged as an enabling or disruptive technology. The promise of open-ended missions allows consideration of radically new trajectories and the delivery of spacecraft to previously unreachable or unsustainable observation ...
Macdonald, Malcolm   +3 more
core   +1 more source

Heliopause explorer: a sailcraft mission to the outer boundaries of the solar system [PDF]

open access: yes, 2003
Solar sail technology holds the promise of enhancing the interplanetary transportation infrastructure for low-cost space exploration missions in the new millennium, by exploiting the freely available, space-pervading resource of solar radiation pressure ...
Niederstadt, T.   +14 more
core   +1 more source

Transient shocks beyond the heliopause

open access: yesJournal of Physics: Conference Series, 2015
The heliopause is a rich, dynamic surface affected by the time-dependent solar wind. Stream interactions due to coronal mass ejections (CMEs), corotating interaction regions (CIRs), and other transient phenomena are known to merge producing global merged interaction regions (GMIRs).
R L Fermo, N V Pogorelov, L F Burlaga
openaire   +1 more source

2D Kelvin–Helmholtz Instability with Anisotropic Pressure

open access: yesThe Astrophysical Journal
The Kelvin–Helmholtz (KH) instability occurs in multiple heliospheric (solar-wind stream interfaces, planetary magnetospheres, cometary tails, heliopause flanks) and interstellar (protoplanetary disks, relativistic jets, neutron star accretion disks ...
Shishir Biswas   +4 more
doaj   +1 more source

Home - About - Disclaimer - Privacy