Results 71 to 80 of about 2,085 (203)
A local interstellar spectrum for galactic electrons
A heliopause spectrum at 122 AU from the Sun is presented for galactic electrons over an energy range from 1 MeV to 50 GeV that can be considered the lowest possible local interstellar spectrum (LIS). The focus is on the spectral shape of the LIS below 1.
Nndanganeni, R. R., Potgieter, M. S.
core +1 more source
Context. Since 1996, during periods of low solar activity, the HSTOF instrument onboard the SOHO satellite has been measuring weak fluxes of He atoms of 28-58 keV/n (helium energetic neutral atoms - He ENA).
Czechowski, A. +3 more
core +1 more source
Transient shocks beyond the heliopause
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
In this paper, we study heliospheric Ly-$\alpha$ absorption toward nearby stars in different lines of sight. We use the Baranov-Malama model of the solar wind interaction with a two-component (charged component and H atoms) interstellar medium ...
Baranov +43 more
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Interstellar neutral (ISN) helium atoms penetrating the heliosphere are used to find the flow velocity and temperature of the very local interstellar medium near the heliosphere.
P. Swaczyna +3 more
doaj +1 more source
Space science: Beyond the heliopause [PDF]
Roger D. Launius savours a masterful account, by a veteran of interplanetary space science, of the Voyager probes' mission to the giant planets.
openaire +2 more sources
2D Kelvin–Helmholtz Instability with Anisotropic Pressure
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
A Large Magnetic Hump in the VLISM Observed by Voyager 1 in 2020–2022
Voyager 1 has been moving through the very local interstellar medium (VLISM) for approximately one solar cycle, from 122.58 au on 2012/DOY 238 (August 25) to 158.5 au on 2023.0. Previously, an abrupt increase (“jump”) in the magnetic field strength B and
L. F. Burlaga +5 more
doaj +1 more source
Cosmic ray anisotropies near the heliopause [PDF]
Context. The Voyager 1 spacecraft became the first man-made probe to cross the heliopause into the local interstellar medium and measure the galactic environment, including charged particle intensities, in situ. Aims. We qualitatively explain the observed anisotropies of galactic and anomalous cosmic rays in the interstellar medium. Methods.
R. D. Strauss, H. Fichtner
openaire +1 more source
The recent observations of the anomalous cosmic ray (ACR) energy spectrum as Voyagers 1 and 2 crossed the heliospheric termination shock have called into question the conventional shock source of these energetic particles.
Burlaga +11 more
core +1 more source

