Results 251 to 260 of about 1,774 (287)

Advances and Challenges in Understanding Atmospheric Oxidizing Capacity in China: Insights from Chemical Mechanisms and Model Applications. [PDF]

Toxics
Li P, Ren Y, Bi F, Long F, Li J, Zhang H, Wu Z, Li H.   +7 more
europepmc   +1 more source

Interfacial design strategies for stable and high-performance perovskite/silicon tandem solar cells on industrial silicon cells. [PDF]

Nat Commun
Fang L, Ren M, Li B, Liu X, Liang S, Petermann J, Gholipoor M, Zhao T, Sutter J, Fassl P, Weber H, Niemann R, Dai L, Guo R, Lemmer U, Fertig F, Paetzold UW.   +16 more
europepmc   +1 more source

A cosmic-ray loaded nascent outflow driven by a massive star cluster. [PDF]

Nat Commun
Lemoine-Goumard M, Härer L, Mohrmann L, Bernet R, Hinton J, Peron G, Reville B, Tibaldo L, Vieu T.   +8 more
europepmc   +1 more source

Global climate governance remains resilient under Trump 2.0. [PDF]

Glob Public Policy Gov
Sun Y, Ye Y.
europepmc   +1 more source

Some of the next articles are maybe not open access.

Related searches:

The termination shock of the solar wind

Space Science Reviews, 1996
An overview of the solar wind termination shock is presented including: its place in the heliosphere and its origin; its structure including the role of interstellar pickup ions and galactic and anomalous cosmic rays; its inferred location based on Lyman-α backscatter, Voyager radio signals, and anomalous cosmic rays; its shape and movement.
Martin A Lee, Lee Martin A
exaly   +3 more sources

The role of solar wind electrons at the solar wind termination shock [PDF]

Monthly Notices of the Royal Astronomical Society: Letters, 2013
Abstract Voyager 2 plasma observations have recently revealed that, as predicted by theory, there exists a solar wind termination shock at 87 au. However, it is evidently different from classical expectations, for instance revealing the downstream solar wind protons still to be in a supersonic mode. In this paper we show that in order to
S V Chalov, Fahr H J
exaly   +2 more sources

Superdiffusive Transport Upstream of the Solar Wind Termination Shock

AIP Conference Proceedings, 2010
In this work the properties of transport of ions accelerated at the solar wind termination shock are studied. The approach used to investigate the propagation of those particles is probabilistic and is based on the analysis of particle time profiles upstream of the shock front.
G Zimbardo, S Perri, M Maksimovic
exaly   +4 more sources

The termination of the solar wind

Icarus, 1971
Abstract It has previously been suggested that the solar wind might terminate at distances of 5 AU to 20 AU from the Sun, and that the solar wind might be drastically slowed down by charge exchange and photoionization of interstellar hydrogen atoms which approach the Sun.
Thomas R. McDonough, Neil M. Brice
openaire   +1 more source

The solar wind shock termination

Advances in Space Research, 1986
Abstract We analyse the possibility that the shock termination of the solar wind should occur at a heliocentric distance of 50 a.u. It is concluded that this is possible if the density of the interstellar medium near the Sun is of the order of 0.5 cm −3 , or the pressure of low energy cosmic rays (less than about 300 MeV/nucleon) is of the order of 6×
Axford, W., Ip, W.
openaire   +2 more sources