A Persistent Depletion of Plasma Ions Within Jupiter's Auroral Polar Caps

2020 ◽  
Vol 47 (23) ◽  
Author(s):  
C. J. Pollock ◽  
R. W. Ebert ◽  
F. Allegrini ◽  
F. Bagenal ◽  
D. J. McComas ◽  
...  
Keyword(s):  

1992 ◽  
Vol 128 ◽  
pp. 56-77 ◽  
Author(s):  
Jonathan Arons

AbstractI survey recent theoretical work on the structure of the magnetospheres of rotation-powered pulsars, within the observational constraints set by their observed spindown, their ability to power synchrotron nebulae and their ability to produce beamed collective radio emission, while putting only a small fraction of their energy into incoherent X- and gamma radiation. I find no single theory has yet given a consistent description of the magnetosphere, but I conclude that models based on a dense outflow of pairs from the polar caps, permeated by a lower density flow of heavy ions, are the most promising avenue for future research.



2021 ◽  
Vol 67 (10) ◽  
pp. 3228-3236
Author(s):  
Angel O.U. Parentis ◽  
Bruno S. Zossi ◽  
Hagay Amit ◽  
Ana G. Elias
Keyword(s):  


2012 ◽  
Vol 10 (H16) ◽  
pp. 86-89 ◽  
Author(s):  
J. Todd Hoeksema

AbstractThe almost stately evolution of the global heliospheric magnetic field pattern during most of the solar cycle belies the intense dynamic interplay of photospheric and coronal flux concentrations on scales both large and small. The statistical characteristics of emerging bipoles and active regions lead to development of systematic magnetic patterns. Diffusion and flows impel features to interact constructively and destructively, and on longer time scales they may help drive the creation of new flux. Peculiar properties of the components in each solar cycle determine the specific details and provide additional clues about their sources. The interactions of complex developing features with the existing global magnetic environment drive impulsive events on all scales. Predominantly new-polarity surges originating in active regions at low latitudes can reach the poles in a year or two. Coronal holes and polar caps composed of short-lived, small-scale magnetic elements can persist for months and years. Advanced models coupled with comprehensive measurements of the visible solar surface, as well as the interior, corona, and heliosphere promise to revolutionize our understanding of the hierarchy we call the solar magnetic field.



2007 ◽  
Vol 37 (11) ◽  
pp. 1060-1064 ◽  
Author(s):  
I L Beigman ◽  
V E Levashov ◽  
K N Mednikov ◽  
A S Pirozhkov ◽  
E N Ragozin ◽  
...  


2008 ◽  
Author(s):  
Zach Medin ◽  
Dong Lai ◽  
C. Bassa ◽  
Z. Wang ◽  
A. Cumming ◽  
...  


2008 ◽  
Vol 2008 ◽  
pp. 1-5 ◽  
Author(s):  
R. T. Khaydarov ◽  
U. S. Kunishev

Using a static mass spectrometer, we study the characteristics of multicharge plasma ions generated from solid targets under the action of a 15 nanosecond Nd:YAG laser radiation with maximal intensity 1011 W/cm2. We consider two-element solid targets with a mass of the heavy component ranging from 44.9 (Sc) to 174.9 (Lu) with main attention to the properties of oxygen ions. The time-of-flight measurements show that oxygen ions are obtained in the range of the energy E = 40–250 eV with maximal charge Zmax=2. The latter is independent on the target composition for the given intensity of the laser radiation. However, the properties of the energy spectra of oxygen ions strongly depend on the second component of the target, which is explained by the interaction between the light and heavy elements of the target.



2008 ◽  
Vol 26 (1) ◽  
pp. 37-40 ◽  
Author(s):  
R. G. Evans

AbstractThe charge on plasma ions may fluctuate due to random ionization and recombination processes. The resulting motion has a time dependent Hamiltonian and in simple cases, the ions steadily gain energy. Quantitative rates are estimated for some cases involving high Z plasmas.



1971 ◽  
Vol 19 (11) ◽  
pp. 1541-1577 ◽  
Author(s):  
G.E. Morfill ◽  
J.J. Quenby
Keyword(s):  




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