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1 probe the dynamics of the natural aurora and magnetosphere.
2 eleration and loss processes deep within the magnetosphere.
3 o probe magneto-ionic properties of a pulsar magnetosphere.
4 nfluence of J0737-3039A's energy flux on its magnetosphere.
5 gh direct interaction with the white dwarf's magnetosphere.
6 re of, and the energy flow within, Jupiter's magnetosphere.
7 anet has a strong magnetic field and a large magnetosphere.
8 ation of energetic heavy ions from the inner magnetosphere.
9 hat excite the aurora originate in the outer magnetosphere.
10 ward of the latitudes connected to the inner magnetosphere.
11 on connected magnetically to Jupiter's outer magnetosphere.
12 e magnetotail allows the solar wind into the magnetosphere.
13 h the interaction of the solar wind with the magnetosphere.
14 substantial entry of the solar wind into the magnetosphere.
15 y which solar-wind energy enters the Earth's magnetosphere.
16 e postmidnight, predawn sector of the jovian magnetosphere.
17 a jets at 10-14 Earth radii in the nightside magnetosphere.
18 f ice by energetic particles from the jovian magnetosphere.
19 bardment of energetic ions from the planet's magnetosphere.
20 slowly varying background field of Jupiter's magnetosphere.
21 rocess by which solar wind plasma enters the magnetosphere.
22 is not expected in the textbook model of the magnetosphere.
23 sitron (hereafter e(+/-)) plasma of the star magnetosphere.
24 ed and are caused by changes in the pulsar's magnetosphere.
25 ion for hot electrons in the nightside outer magnetosphere.
26  convection of photoions produced inside the magnetosphere.
27 n between the shocked solar wind and Earth's magnetosphere.
28  the shocked solar wind, outside of Saturn's magnetosphere.
29 net, but these Mercury-derived ions fill the magnetosphere.
30  using our current understanding of Saturn's magnetosphere.
31 sphere capable of locally affecting Saturn's magnetosphere.
32 olt are substantially energized in Mercury's magnetosphere.
33 of Earth, Saturn imposes a rapid spin on its magnetosphere.
34 's electrodynamic interaction with Jupiter's magnetosphere.
35 rce region along the dusk flank of Jupiter's magnetosphere.
36  only humans to have traveled beyond Earth's magnetosphere.
37 y hotter, more tenuous plasma from the outer magnetosphere.
38 tmosphere and its interaction with Jupiter's magnetosphere.
39 ent with centrifugal interchange in Saturn's magnetosphere.
40 sphere and corotating ions in Saturn's inner magnetosphere.
41 stituents in the ionosphere, plasmasphere or magnetosphere.
42 es of trapped ions from the middle and inner magnetosphere.
43  but persistent signal was observed from the magnetosphere.
44  it differ from those that drive the Earth's magnetosphere.
45 us to investigate the structure of planetary magnetospheres.
46 nificant amounts of energy and mass from the magnetospheres.
47 he rotation rates of Saturn's atmosphere and magnetosphere?
48 ysical processes coupling the ionosphere and magnetosphere?
49 gyro-radius of a Na+ pickup ion entering the magnetosphere after being accelerated in the magnetoshea
50 agnetic field to the surface, exosphere, and magnetosphere, all of which interact with the solar wind
51 d acceleration of electron beams in Saturn's magnetosphere along field lines that statistically map i
52 th-like injections of electrons in Jupiter's magnetosphere and a transient auroral feature in Jupiter
53 ater sensitivity for imaging the terrestrial magnetosphere and allow the bulk of the magnetospheric i
54       It has often been stated that Saturn's magnetosphere and aurorae are intermediate between those
55 t acquired direct observations of the jovian magnetosphere and auroral emissions from a vantage point
56    This review focuses on the atmosphere and magnetosphere and briefly outlines the state of our know
57 e electrodynamic interaction between Earth's magnetosphere and ionosphere produces an asymmetry consi
58 ergy and momentum from the solar wind to the magnetosphere and ionosphere.
59 rgy couples from the solar wind into Earth's magnetosphere and ionosphere.
60 Earth's magnetotail, encompassing the entire magnetosphere and producing spectacular auroral displays
61 ectromagnetic interactions, escape Jupiter's magnetosphere and then populate the environment around t
62 es to provide global images of Earth's inner magnetosphere and upper atmosphere.
63 harge exchange neutrals from the terrestrial magnetosphere and would also have applications for simil
64      Solar wind energy transfer to planetary magnetospheres and ionospheres is controlled by magnetic
65                              The solar wind, magnetosphere, and ionosphere form a single system drive
66 masphere is one inner component of the whole magnetosphere, and the configuration of the plasmasphere
67 s both in the incident solar wind and in the magnetosphere are important in determining the efficienc
68  to be caused by interaction with the middle magnetosphere around the planet.
69 Multiscale (MMS) mission, we utilize Earth's magnetosphere as a plasma physics laboratory.
70 by precipitation of electrons from Neptune's magnetosphere as previously proposed, Triton could have
71 s to a seemingly different wave in the outer magnetosphere, but this theory was difficult to test bec
72  believed to be flung outward from the inner magnetosphere by centrifugal force and replaced by hotte
73 rn, the electric field produced in the inner magnetosphere by Earth's rotation can change the velocit
74 ectrons and ions that are trapped in Earth's magnetosphere can suddenly be accelerated towards the pl
75  plasma-turbulent wave packets in the pulsar magnetosphere--can account for the nanopulses we observe
76 ssini's initial orbit, we observed a dynamic magnetosphere composed primarily of a complex mixture of
77  radiation belts during a type of solar wind-magnetosphere coupling which is unusual for planets in o
78 arely understood electron beams in Jupiter's magnetosphere, demonstrate that anti-planetward accelera
79 atom imaging of ions injected into the inner magnetosphere during magnetospheric disturbances shows a
80 mate the magnetospheric currents in a pulsar magnetosphere during the occurrence of radio emission.
81  Saturn's largest moon, Titan, with Saturn's magnetosphere during two close flybys of Titan on 26 Oct
82                               In the Earth's magnetosphere, electron energies reach hundreds of thous
83                About 10 days before SOI, the magnetosphere exhibited a day-night asymmetry that varie
84  interstellar dust grains entering Jupiter's magnetosphere form a detectable diffuse faint ring of ex
85      Juno's capture orbit spanned the jovian magnetosphere from bow shock to the planet, providing ma
86 he Cassini spacecraft observed the saturnian magnetosphere from January 2004 until Saturn orbit inser
87 e interaction of the solar wind with Earth's magnetosphere gives rise to the bright polar aurorae and
88 ernal to the jovian system, whereas Saturn's magnetosphere has generally been considered to have both
89              Recent observations in Saturn's magnetosphere have revealed narrow injections of hot, te
90 se waves are important not only in planetary magnetospheres, heliospheres and astrophysical systems b
91                                    The Inner Magnetosphere Imaging Mission, which the National Aerona
92    This remarkable deformation of the entire magnetosphere implies surprisingly powerful acceleration
93 s provided the first examination of Saturn's magnetosphere in 23 years, revealing a dynamic plasma an
94 etic fields (associated with Jupiter's inner magnetosphere) in the vicinity of both Europa and Callis
95                     Once Cassini entered the magnetosphere, in situ measurements showed high concentr
96 s to directly observe the state of the inner magnetosphere, including the radiation belts during a ty
97          But the plasma content in the outer magnetosphere increases during northward solar-wind magn
98 as travel goes beyond the Earth's protective magnetosphere into the more intense deep space radiation
99 and oxygen ions precipitating from the inner magnetosphere into the planet's polar regions.
100 -scale oscillation powered by the solar wind-magnetosphere-ionosphere (SW-M-I) interaction.
101   The sawtooth mode of convection of Earth's magnetosphere is a 2- to 4-hour planetary-scale oscillat
102  ionized atmosphere define its boundaries: A magnetosphere is born.
103 bservations by MESSENGER show that Mercury's magnetosphere is immersed in a comet-like cloud of plane
104  The coupling between the solar wind and the magnetosphere is mediated and controlled by the magnetic
105   These observations indicate that Mercury's magnetosphere is much more responsive to IMF direction a
106 nisms by which the solar wind enters Earth's magnetosphere is one of the biggest goals of magnetosphe
107                     The structure of Earth's magnetosphere is poorly understood when the interplaneta
108 d an external heating source from the jovian magnetosphere is required.
109                                          The magnetosphere is shown to be highly variable and influen
110 hat the interaction between Io and Jupiter's magnetosphere is stabilized by a feedback mechanism in w
111 nnection, but which process dominates in the magnetosphere is still debated.
112  to cross the magnetopause and enter Earth's magnetosphere is the merging between solar-wind and terr
113  Patchy reconnection observed in the Earth's magnetosphere is therefore likely to be a geophysical ef
114                 The current sheet within the magnetosphere is thinner and more extended, and we obser
115 nderstanding built on studies of the Earth's magnetosphere is valid.
116                                     Saturn's magnetosphere is, therefore, strongly driven by the sola
117  wind and the dynamics of the outer planets' magnetospheres is poorly understood.
118  most electrons as they drift around Earth's magnetosphere, leading to the development of observed pa
119 itatis and has discovered the smallest known magnetosphere, magnetosheath, and bow shock complex in t
120 e (100 to several hundred kilometers across) magnetosphere, magnetosheath, and bow shock system.
121 et, allowing plasma produced deep inside the magnetosphere near Io's orbit to escape in the antisolar
122  we investigated simultaneous ionosphere and magnetosphere observations of the plasmaspheric plume an
123 e satellites Rhea and Dione orbit within the magnetosphere of Saturn, where they are exposed to parti
124 rocesses originating much further out in the magnetosphere of the dwarf star that couple energy into
125                                      But the magnetospheres of Jupiter and Earth are so different---p
126 here are substantial differences between the magnetospheres of Jupiter and Saturn, it has been sugges
127                   The space environments--or magnetospheres--of magnetized planets emit copious quant
128 he existence of an extended, complex coronal magnetosphere originating at the cooler K subgiant.
129  associated with reconnection in the Earth's magnetosphere raise the possibility that reconnection is
130  interactions between the solar wind and the magnetosphere, rather than by local conditions at the ma
131 e larger than what is produced in the Jovian magnetosphere, revealing aurorae to be a potentially ubi
132 g the full wave energy budget in the Earth's magnetosphere, revealing that a significant fraction of
133  present-day value, indicating that a viable magnetosphere sheltered the early Earth's atmosphere fro
134 pite the large differences between planetary magnetospheres, some processes that generate aurorae are
135 hear observed at the edge of Titan's induced magnetosphere suggests that reconnection may have been i
136 scribes plasma circulation through Mercury's magnetosphere, suggests that such circulation determines
137 currently unexplained processes in the outer magnetosphere that produce highly localized and highly v
138 entially ubiquitous signature of large-scale magnetospheres that can scale to luminosities far greate
139 ending back a wealth of data on the planet's magnetosphere (the region dominated by the magnetic fiel
140                    The structure of Saturn's magnetosphere, the extended region of space threaded by
141 ng Galileo's passage through Jupiter's inner magnetosphere, the observed composition of these heavy i
142 a systems ranging from laboratories, Earth's magnetosphere, the solar corona and astrophysical enviro
143 ommon and can significantly affect planetary magnetospheres, the mechanisms by which cavities evolve
144        As the outflowing ions fill the inner magnetosphere, their pressure distends the nightside mag
145                           A similarly shaped magnetosphere then results from the remnant magnetic fie
146                     Below the threshold, the magnetosphere undergoes quasi-steady convection.
147 ervations revealed that Titan's flow-induced magnetosphere was populated by "fossil" fields originati
148 hus solar wind energy input into the Earth's magnetosphere was reduced, resulting in a more Jupiter-l
149 ntrifugal interchange of plasmas in rotating magnetospheres was predicted many years ago and was conc
150 the loss of charged particles from Jupiter's magnetosphere---were unknown.
151 ver to transport solar wind into the Earth's magnetosphere when the magnetopause features a large mag
152  sites along the sunward boundary of Earth's magnetosphere where the interplanetary magnetic field re
153 ectromagnetic waves pervasive in the Earth's magnetosphere, where they continuously remove or energiz
154 nalysis of 50-80 keV ENA images of Jupiter's magnetosphere, where two distinct emission regions domin
155 rents flowing between the ionosphere and the magnetosphere which accelerate energetic charged particl
156  for the source of the missing energy is the magnetosphere, which injects energy mostly in the polar
157 major compression and reconfiguration of the magnetosphere, which produces strong electric fields and
158 ly demonstrated by observations in Jupiter's magnetosphere, which--like that of Saturn (but unlike th
159                                   Within the magnetosphere, whistler-mode auroral hiss emissions were
160  gained into the chemical composition of the magnetosphere, with surprising results.

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