Results 201 to 210 of about 1,361 (233)
Interstellar hydrogen ionization in the heliosheath [PDF]
Journal of Geophysical Research: Space Physics, 2015 AbstractThe expanding solar wind plasma undergoes a shock transition at the interstellar boundary of the solar system and fills the inner heliosheath, the region between the termination shock and the heliopause. The nonequilibrium heliosheath plasma is a main source of energetic neutral atoms that allow remote probing of the heliospheric interface ...
Mike Gruntman
exaly +2 more sources
Current sheets in the heliosheath: Voyager 1, 2009 [PDF]
Journal of Geophysical Research, 2011 L F Burlaga
exaly +2 more sources
Some of the next articles are maybe not open access.
Related searches:
Related searches:
AIP Conference Proceedings, 2010
This paper describes recent results from Voyager 2 in the heliosheath (HSh). The speed has been constant across the HSh. The density and temperature have decreased, probably due both to a decrease in solar output and deflection of plasma toward the heliotail.
John D. Richardson +5 more
openaire +1 more source
This paper describes recent results from Voyager 2 in the heliosheath (HSh). The speed has been constant across the HSh. The density and temperature have decreased, probably due both to a decrease in solar output and deflection of plasma toward the heliotail.
John D. Richardson +5 more
openaire +1 more source
Cassini ENA images of the heliosheath and Voyager “ground truth”: Thickness of the heliosheath
AIP Conference Proceedings, 2012Cassini/INCA (Ion and Neutral Camera) ENA images of the heliosheath, when combined with the “ground truth” of in situ measurements of ion intensities throughout the heliosheath obtained by Voyager/LECP (Low Energy Charged Particle Experiment), allow us to estimate a thickness parameter (L) along the two lines of sight (LOS) to the Voyager 1/2 ...
E. C. Roelof +4 more
openaire +1 more source
Magnetic fields in the heliosheath
AIP Conference Proceedings, 2006We review observations of the magnetic field made by Voyager 1 in the heliosheath from DOY 351, 2004 to 125, 2005, and we discuss their significance in regard to the structure and dynamics of the heliosheath. The probability distribution of hourly averages of B in the heliosheath is a Gaussian distribution.
L. F. Burlaga, N. F. Ness, M. H. Acuna
openaire +1 more source
Mirror Modes in the Heliosheath
AIP Conference Proceedings, 2011Mirror mode (MM) structures are identified in the Voyager 1 heliosheath magnetic field data. Their characteristics are: 1) quasiperiodic structures with a typical scale size of ∼57 ρp (proton gyroradii), 2) little or no angular changes across the structures (∼3° longitude and ∼3° latitude), and 3) a lack of sharp boundaries at the magnetic dip edges ...
B. T. Tsurutani +9 more
openaire +1 more source
Cosmic rays in the dynamic heliosheath
Advances in Space Research, 2008Cosmic ray modulation in the outer heliosphere is discussed from a modeling perspective. Emphasis is on the transport and acceleration of these particles at and beyond the solar wind termination shock in the inner heliosheath region and how this changes over a solar cycle.
S E S Ferreira +2 more
exaly +3 more sources
Planetary and Space Science, 2002
Abstract This paper is an introduction to the topic of stellarsheaths that are formed due to the interaction of stellar winds and interstellar gas flow. Heliosheath formation and possible methods of its detection are discussed in detail. This invited talk was presented at the 2000 Antalya Turkey Conference on the problems of magnetosheaths in the ...
openaire +1 more source
Abstract This paper is an introduction to the topic of stellarsheaths that are formed due to the interaction of stellar winds and interstellar gas flow. Heliosheath formation and possible methods of its detection are discussed in detail. This invited talk was presented at the 2000 Antalya Turkey Conference on the problems of magnetosheaths in the ...
openaire +1 more source
Plasma in the outer heliosphere and the heliosheath
AIP Conference Proceedings, 2006Voyager 2 (V2) measures the plasma parameters in the outer heliosphere. The solar wind speed decreased and dynamic pressure was constant and relatively low in 2005. We use these data to predict the motion of the termination shock (TS) and show that V2 may be close to the TS.
John D. Richardson, Chi Wang, Ming Zhang
openaire +1 more source
Plasma variability in the heliosheath
AIP Conference Proceedings, 2012The heliosheath is a highly variable plasma environment. The plasma parameters across the heliosheath are presented and their time evolution discussed. Large fluctuations in velocity, density, and temperature occur on time scales of tens of minutes throughout the heliosheath.
openaire +1 more source