Results 171 to 180 of about 588 (209)

Primordial black holes and their gravitational-wave signatures. [PDF]

Living Rev Relativ
Bagui E, Clesse S, De Luca V, Ezquiaga JM, Franciolini G, García-Bellido J, Joana C, Kumar Jain R, Kuroyanagi S, Musco I, Papanikolaou T, Raccanelli A, Renaux-Petel S, Riotto A, Ruiz Morales E, Scalisi M, Sergijenko O, Ünal C, Vennin V, Wands D, LISA Cosmology Working Group.   +20 more
europepmc   +1 more source

Heliosheath Processes and the Structure of the Heliopause: Modeling Energetic Particles, Cosmic Rays, and Magnetic Fields [PDF]

Space Science Reviews, 2017
This paper summarizes the results obtained by the team “Heliosheath Processes and the Structure of the Heliopause: Modeling Energetic Particles, Cosmic Rays, and Magnetic Fields” supported by the International Space Science Institute (ISSI) in Bern ...
Peter Würz, Gary P Zank, Nikolai Pogorelov   +2 more
exaly   +5 more sources

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Heliopause Stability

Fluid Dynamics
M S Ruderman
exaly   +2 more sources

Magnetic field and particle measurements made by Voyager 2 at and near the heliopause [PDF]

Nature Astronomy, 2019
The heliopause is a boundary that separates the heliosheath (which contains magnetic fields and plasmas that originate in the Sun) from the interstellar medium (which contains magnetic fields and particles of stellar/interstellar origin). Observations of
Edward Stone, Leonard Burlaga, Jeewoo Park   +2 more
exaly   +1 more source

Heliopause and asteropauses

Astrophysics and Space Science, 2001
In this paper I will use recent results about the heliosphere and the so-called ‘H walls’ around nearby star ‘asteropauses’ (the equivalent of the heliopause for other stars) to show new connections between heliospheric physics and other fields in space physics.
openaire   +1 more source

MHD Instabilities at the Heliopause

AIP Conference Proceedings, 2006
The heliopause (HP) is the outer edge of the heliosphere which separates the tenuous and hot heliosheath plasma on one side and the relatively dense and cool magnetized interstellar plasma on the other side. As a surface of tangential discontinuity, the HP is subjected to both Rayleigh‐Taylor (RT) and Kelvin‐Helmholtz (KH) instabilities.
B. Dasgupta, V. Florinski, J. Heerikhuisen, G. P. Zank   +3 more
openaire   +1 more source

The heliopause

Reviews of Geophysics, 1990
There is a growing anticipation among space scientists that a Pioneer or Voyager spacecraft will soon pass through one of the last major frontiers in the solar system—the heliospheric terminal shock. Some unknown, but perhaps small, distance beyond the terminal shock is the heliopause, marking the final boundary between solar wind and galactic plasmas ...
openaire   +1 more source

The interstellar heliopause probe

Acta Astronautica, 2005
Abstract The Interstellar Heliopause Probe (IHP) is one of four Technology Reference Studies (TRS) introduced by the Planetary Exploration Studies Section of the Science Payload & Advanced Concepts Office (SCI-A) at ESA. The overall purpose of the TRSs is to focus the development of strategically important technologies of likely relevance to future ...
A. Lyngvi, P. Falkner, S. Kemble, M. Leipold, A. Peacock   +4 more
openaire   +1 more source

A cold plasma layer at the heliopause

Advances in Space Research, 1995
Abstract The shocked solar wind plasma cools down by charge-exchange with neutral hydrogen of LISM origin. The effect accumulates in time and leads to creation of a cold, high density plasma layer spreading out from the stagnation point along the inner surface of the heliopause.
A. Czechowski, S. Grzedzielski
openaire   +1 more source

Reconnection at the heliopause

Advances in Space Research, 1989
Abstract Views of the front side heliopause and different areas, where magnetic field reconnection takes place, are provided for various assumed orientations of the magnetic field of the local interstellar medium. Within these reconnection patches the lines of constant angle between the magnetic field of the unperturbed solar wind (standard Parker's ...
openaire   +1 more source