Results 211 to 220 of about 592,047 (243)

Voyager 1 in the Foreshock, Termination Shock, and Heliosheath

Science, 2005
Voyager 1 (V1) began measuring precursor energetic ions and electrons from the heliospheric termination shock (TS) in July 2002. During the ensuing 2.5 years, average particle intensities rose as V1 penetrated deeper into the energetic particle foreshock of the TS.
R B, Decker, S M, Krimigis, E C, Roelof, M E, Hill, T P, Armstrong, G, Gloeckler, D C, Hamilton, L J, Lanzerotti   +7 more
openaire   +2 more sources

On terminating Poisson processes in some shock models

Reliability Engineering & System Safety, 2010
Abstract A system subject to a point process of shocks is considered. Shocks occur in accordance with the homogeneous Poisson process. Different criteria of system failure (termination) are discussed and the corresponding probabilities of failure (accident)-free performance are derived.
Maxim Finkelstein, Francois Marais
openaire   +1 more source

Crossing the Termination Shock into the Heliosheath: Magnetic Fields

Science, 2005
Magnetic fields measured by Voyager 1 show that the spacecraft crossed or was crossed by the termination shock on about 16 December 2004 at 94.0 astronomical units. An estimate of the compression ratio of the magnetic field strength B (± standard error of the mean) across the shock is B 2
L F, Burlaga, N F, Ness, M H, Acuña, R P, Lepping, J E P, Connerney, E C, Stone, F B, McDonald   +6 more
openaire   +2 more sources

Structure and properties of the termination shock

AIP Conference Proceedings, 2004
Conventionally, the heliospheric termination shock (HTS) is regarded as a sharp MHD discontinuity. More recent models suggest that the back‐reaction of energetic cosmic rays accelerated at the HTS will create a broad shock with an extended precursor. Here we suggest that a combination of upstream solar wind disturbances interacting with the HTS, the ...
openaire   +1 more source

Anomalous Cosmic Rays outside of the Termination Shock

2001
Anomalous Cosmic Rays (ACR) are most probably generated at the solar wind termi- nation shock. When observed in the region inside the shock, the ACR energy spectrum is significantly modulated. The region outside the shock is so far inaccessible to obser- vations. However, the low energy (~ 100 keV) part of the spectrum beyond the shock could be sampled
Czechowski, A., Grzedzielski, S., Fichtner, H., Hilchenbach, M., Hsieh, K.C.   +4 more
openaire   +2 more sources

Observations of the Termination Shock and Heliosheath

2010
Voyagers 1 and 2 have both crossed the solar wind termination shock and are now in the heliosheath, the region of shocked solar wind plasma before the heliopause. This paper reviews observations of the termination foreshock, the termination shock (TS), and the heliosheath.
openaire   +1 more source

Heat shock induces premature transcript termination and reconfigures the human transcriptome

Molecular Cell, 2022
Aengus Stewart, Gavin Kelly, Michael Wierer   +2 more
exaly  

On freejet terminal shocks

AIAA Journal, 1970
MICHAEL J. WERLE, DAVID G. SHAFFER, RICHARD T. DRIFTMYER   +2 more
openaire   +1 more source

THE TERMINATION SHOCK AND THE HELIOSHEATH

2018
S. T. SUESS, STEVEN NERNEY
openaire   +1 more source

Properties of the termination shock observed by Voyager 2

Geophysical Research Letters, 2008
Chi Wang, Hui Li, John Richardson
exaly