コーパス検索結果 (１語後でソート)
通し番号をクリックするとPubMedの該当ページを表示します
1 tional utility and dictates the shape of the magnetosphere.
2 but persistent signal was observed from the magnetosphere.
3 it differ from those that drive the Earth's magnetosphere.
4 probe the dynamics of the natural aurora and magnetosphere.
5 eleration and loss processes deep within the magnetosphere.
6 o probe magneto-ionic properties of a pulsar magnetosphere.
7 nfluence of J0737-3039A's energy flux on its magnetosphere.
8 re of, and the energy flow within, Jupiter's magnetosphere.
9 anet has a strong magnetic field and a large magnetosphere.
10 ation of energetic heavy ions from the inner magnetosphere.
11 hat excite the aurora originate in the outer magnetosphere.
12 ward of the latitudes connected to the inner magnetosphere.
13 on connected magnetically to Jupiter's outer magnetosphere.
14 e magnetotail allows the solar wind into the magnetosphere.
15 h the interaction of the solar wind with the magnetosphere.
16 substantial entry of the solar wind into the magnetosphere.
17 y which solar-wind energy enters the Earth's magnetosphere.
18 e postmidnight, predawn sector of the jovian magnetosphere.
19 f ice by energetic particles from the jovian magnetosphere.
20 bardment of energetic ions from the planet's magnetosphere.
21 slowly varying background field of Jupiter's magnetosphere.
22 onses to the solar energy input into Earth's magnetosphere.
23 n between the shocked solar wind and Earth's magnetosphere.
24 netospheric Multiscale spacecraft in Earth's magnetosphere.
25 RENA ion sensors nearby and inside Mercury's magnetosphere.
26 only humans to have traveled beyond Earth's magnetosphere.
27 ellite outgassing, were detected outside the magnetosphere.
28 stituents in the ionosphere, plasmasphere or magnetosphere.
29 nto the physics of Jupiter's magnetodisk and magnetosphere.
30 scale is a fundamental feature of planetary magnetosphere.
31 channel to transport lightning energy to the magnetosphere.
32 thermal ring current populations in Saturn's magnetosphere.
33 than expected, signature of a highly eroded magnetosphere.
34 ich regulates the field configuration of the magnetosphere.
35 d by scattering off charged particles in the magnetosphere.
36 gh direct interaction with the white dwarf's magnetosphere.
37 partially open field lines within Ganymede's magnetosphere.
38 h explosive events in a dynamically evolving magnetosphere.
39 istlers to the lightning energy reaching the magnetosphere.
40 et, it induces currents that form an induced magnetosphere.
41 a jets at 10-14 Earth radii in the nightside magnetosphere.
42 rocess by which solar wind plasma enters the magnetosphere.
43 is not expected in the textbook model of the magnetosphere.
44 sitron (hereafter e(+/-)) plasma of the star magnetosphere.
45 ed and are caused by changes in the pulsar's magnetosphere.
46 ion for hot electrons in the nightside outer magnetosphere.
47 convection of photoions produced inside the magnetosphere.
48 ant planet, as well as its rings, moons, and magnetosphere.
49 the shocked solar wind, outside of Saturn's magnetosphere.
50 net, but these Mercury-derived ions fill the magnetosphere.
51 nt wave-particle interactions in the Earth's magnetosphere.
52 using our current understanding of Saturn's magnetosphere.
53 sphere capable of locally affecting Saturn's magnetosphere.
54 olt are substantially energized in Mercury's magnetosphere.
55 of Earth, Saturn imposes a rapid spin on its magnetosphere.
56 's electrodynamic interaction with Jupiter's magnetosphere.
57 rce region along the dusk flank of Jupiter's magnetosphere.
58 y hotter, more tenuous plasma from the outer magnetosphere.
59 tmosphere and its interaction with Jupiter's magnetosphere.
60 ent with centrifugal interchange in Saturn's magnetosphere.
61 sphere and corotating ions in Saturn's inner magnetosphere.
62 es of trapped ions from the middle and inner magnetosphere.
63 us to investigate the structure of planetary magnetospheres.
64 nificant amounts of energy and mass from the magnetospheres.
65 en presented as a template for fast-rotating magnetospheres.
66 to the auroral formation in other planetary magnetospheres.
67 y observed only in planetary-scale intrinsic magnetospheres.
68 entally resemble those observed in intrinsic magnetospheres.
69 f chorus waves in other magnetized planetary magnetospheres.
70 he rotation rates of Saturn's atmosphere and magnetosphere?
71 ysical processes coupling the ionosphere and magnetosphere?
73 vours emission arising from the neutron-star magnetosphere(3,4), as opposed to emission regions locat
74 erent emission from FRBs invoke neutron star magnetospheres(3-5) or relativistic shocks far from the
75 at mechanical-optical rotation in the pulsar magnetosphere affects polarisation in a way which is ind
76 gyro-radius of a Na+ pickup ion entering the magnetosphere after being accelerated in the magnetoshea
77 the ionosphere at low latitudes reaches the magnetosphere after undergoing a specular reflection in
78 agnetic field to the surface, exosphere, and magnetosphere, all of which interact with the solar wind
79 d acceleration of electron beams in Saturn's magnetosphere along field lines that statistically map i
80 c field, this interaction creates an induced magnetosphere and a bow shock in front of the planet(2).
81 th-like injections of electrons in Jupiter's magnetosphere and a transient auroral feature in Jupiter
82 ater sensitivity for imaging the terrestrial magnetosphere and allow the bulk of the magnetospheric i
84 t acquired direct observations of the jovian magnetosphere and auroral emissions from a vantage point
85 This review focuses on the atmosphere and magnetosphere and briefly outlines the state of our know
86 e electrodynamic interaction between Earth's magnetosphere and ionosphere produces an asymmetry consi
90 tions achieved by the Arase satellite in the magnetosphere and optical observations of the aurora fro
91 Earth's magnetotail, encompassing the entire magnetosphere and producing spectacular auroral displays
93 ectromagnetic interactions, escape Jupiter's magnetosphere and then populate the environment around t
96 harge exchange neutrals from the terrestrial magnetosphere and would also have applications for simil
99 e planetary interior, extends into the outer magnetosphere, and piles up near its dawnside flank wher
100 masphere is one inner component of the whole magnetosphere, and the configuration of the plasmasphere
101 Observations of heated O(+) ions in the magnetosphere are consistent with resonant wave-particle
102 teractions between this field and the Jovian magnetosphere are expected to funnel most of the associa
103 s both in the incident solar wind and in the magnetosphere are important in determining the efficienc
105 c electrons entering the atmosphere from the magnetosphere, are one of the key loss mechanisms contro
106 ers will be exposed to when going beyond the magnetosphere around Earth, might have a negative effect
109 by precipitation of electrons from Neptune's magnetosphere as previously proposed, Triton could have
110 er of astrophysical systems, e.g., planetary magnetosphere, astrophysical shocks, stellar corona and
111 ric ion drift patterns, typical of intrinsic magnetospheres, at Mars using measurements from Mars Atm
112 ons are important for understanding the weak magnetosphere behavior so close to the Sun, revealing de
114 ses originate from a fixed region within the magnetosphere, but bursts occur in random locations and
115 s to a seemingly different wave in the outer magnetosphere, but this theory was difficult to test bec
116 believed to be flung outward from the inner magnetosphere by centrifugal force and replaced by hotte
117 rn, the electric field produced in the inner magnetosphere by Earth's rotation can change the velocit
118 ncreases the supply of cold O(+) ions to the magnetosphere by more than 3,800%, in which other mechan
120 ectrons and ions that are trapped in Earth's magnetosphere can suddenly be accelerated towards the pl
121 plasma-turbulent wave packets in the pulsar magnetosphere--can account for the nanopulses we observe
122 missions play an important role in planetary magnetospheres, causing scattering loss of radiation bel
123 ssini's initial orbit, we observed a dynamic magnetosphere composed primarily of a complex mixture of
124 t timescale also reveal enhancements in both magnetosphere convection and the ionosphere's two-cell c
125 sights into the mechanisms driving planetary magnetosphere convection, with implications for the upco
127 radiation belts during a type of solar wind-magnetosphere coupling which is unusual for planets in o
129 arely understood electron beams in Jupiter's magnetosphere, demonstrate that anti-planetward accelera
130 wly identified current system in the Martian magnetosphere directly coupled to the wind-driven ionosp
131 global lightning energy contribution to the magnetosphere doubles, implying that the previous estima
132 space hurricane in the polar ionosphere and magnetosphere during low solar and otherwise low geomagn
133 atom imaging of ions injected into the inner magnetosphere during magnetospheric disturbances shows a
134 s an important role in plasma entry into the magnetosphere during northward interplanetary magnetic f
135 mate the magnetospheric currents in a pulsar magnetosphere during the occurrence of radio emission.
136 Saturn's largest moon, Titan, with Saturn's magnetosphere during two close flybys of Titan on 26 Oct
137 nt in all large-scale Solar System planetary magnetospheres: Earth, Jupiter, Saturn, Uranus and Neptu
140 first glitch couples the star's crust to its magnetosphere, enhances the various X-ray signals and sp
142 interstellar dust grains entering Jupiter's magnetosphere form a detectable diffuse faint ring of ex
143 , serves as a textbook example of an induced magnetosphere, formed by interplanetary magnetic fields
144 Juno's capture orbit spanned the jovian magnetosphere from bow shock to the planet, providing ma
145 he Cassini spacecraft observed the saturnian magnetosphere from January 2004 until Saturn orbit inser
147 e interaction of the solar wind with Earth's magnetosphere gives rise to the bright polar aurorae and
148 ernal to the jovian system, whereas Saturn's magnetosphere has generally been considered to have both
150 se waves are important not only in planetary magnetospheres, heliospheres and astrophysical systems b
151 cy satellites embedded within their planets' magnetospheres, hydrazine monohydrate is argued to be th
154 This remarkable deformation of the entire magnetosphere implies surprisingly powerful acceleration
155 s provided the first examination of Saturn's magnetosphere in 23 years, revealing a dynamic plasma an
156 etic fields (associated with Jupiter's inner magnetosphere) in the vicinity of both Europa and Callis
159 s to directly observe the state of the inner magnetosphere, including the radiation belts during a ty
162 as travel goes beyond the Earth's protective magnetosphere into the more intense deep space radiation
164 nd suggest new remote-sensing methods of the magnetosphere, ionosphere, Earth-ionosphere waveguide, a
166 observational findings for the scale of the magnetosphere-ionosphere coupling-interaction, there res
167 ith implications for the upcoming Solar-Wind-Magnetosphere-Ionosphere Link Explorer (SMILE) mission.
168 The sawtooth mode of convection of Earth's magnetosphere is a 2- to 4-hour planetary-scale oscillat
171 bservations by MESSENGER show that Mercury's magnetosphere is immersed in a comet-like cloud of plane
172 The coupling between the solar wind and the magnetosphere is mediated and controlled by the magnetic
173 These observations indicate that Mercury's magnetosphere is much more responsive to IMF direction a
174 recipitation of energetic electrons from the magnetosphere is not always expected in this region of o
176 nisms by which the solar wind enters Earth's magnetosphere is one of the biggest goals of magnetosphe
180 hat the interaction between Io and Jupiter's magnetosphere is stabilized by a feedback mechanism in w
182 magnetosphere with the ionosphere, where the magnetosphere is the large region of space affected by E
183 to cross the magnetopause and enter Earth's magnetosphere is the merging between solar-wind and terr
184 Patchy reconnection observed in the Earth's magnetosphere is therefore likely to be a geophysical ef
189 Distinct from Earth-like, solar wind-driven magnetospheres, it contains an extended magnetodisk enci
190 most electrons as they drift around Earth's magnetosphere, leading to the development of observed pa
192 on populations have been observed inside the magnetosphere, like low latitude boundary layer at magne
193 nse electromagnetic emissions in the Earth's magnetosphere, magnetized planets, and laboratory plasma
194 itatis and has discovered the smallest known magnetosphere, magnetosheath, and bow shock complex in t
195 e (100 to several hundred kilometers across) magnetosphere, magnetosheath, and bow shock system.
196 et, allowing plasma produced deep inside the magnetosphere near Io's orbit to escape in the antisolar
197 we investigated simultaneous ionosphere and magnetosphere observations of the plasmaspheric plume an
198 re from the distant magnetotail to the inner magnetosphere occurs largely in the form of mesoscale fl
201 e satellites Rhea and Dione orbit within the magnetosphere of Saturn, where they are exposed to parti
202 rocesses originating much further out in the magnetosphere of the dwarf star that couple energy into
203 ategories of radiation model invoking either magnetospheres of compact objects (neutron stars or blac
205 spheres throughout the solar system, and the magnetospheres of exoplanets, and provide knowledge of p
207 here are substantial differences between the magnetospheres of Jupiter and Saturn, it has been sugges
209 uts will once again leave Earth's protective magnetosphere only to endure higher levels of radiation
210 he existence of an extended, complex coronal magnetosphere originating at the cooler K subgiant.
211 xternally accelerated cosmic rays, Jupiter's magnetosphere powers this oxygen source internally.
212 solar wind and its interaction with Earth's magnetosphere provide valuable insights into jets across
213 associated with reconnection in the Earth's magnetosphere raise the possibility that reconnection is
214 interactions between the solar wind and the magnetosphere, rather than by local conditions at the ma
215 ate convection within the closed part of the magnetosphere relies on magnetic reconnection in the nig
216 e larger than what is produced in the Jovian magnetosphere, revealing aurorae to be a potentially ubi
217 g the full wave energy budget in the Earth's magnetosphere, revealing that a significant fraction of
218 present-day value, indicating that a viable magnetosphere sheltered the early Earth's atmosphere fro
219 pite the large differences between planetary magnetospheres, some processes that generate aurorae are
220 hear observed at the edge of Titan's induced magnetosphere suggests that reconnection may have been i
221 scribes plasma circulation through Mercury's magnetosphere, suggests that such circulation determines
222 gnetic reconnection event in Jupiter's inner magnetosphere that presents the detection of an ion diff
223 currently unexplained processes in the outer magnetosphere that produce highly localized and highly v
224 entially ubiquitous signature of large-scale magnetospheres that can scale to luminosities far greate
225 ending back a wealth of data on the planet's magnetosphere (the region dominated by the magnetic fiel
227 systems, with the outer boundary of Earth's magnetosphere, the magnetopause, providing an accessible
228 ng Galileo's passage through Jupiter's inner magnetosphere, the observed composition of these heavy i
229 a systems ranging from laboratories, Earth's magnetosphere, the solar corona and astrophysical enviro
231 ommon and can significantly affect planetary magnetospheres, the mechanisms by which cavities evolve
234 These results are relevant for planetary magnetospheres throughout the solar system, and the magn
237 ervations revealed that Titan's flow-induced magnetosphere was populated by "fossil" fields originati
238 hus solar wind energy input into the Earth's magnetosphere was reduced, resulting in a more Jupiter-l
239 ntrifugal interchange of plasmas in rotating magnetospheres was predicted many years ago and was conc
240 of lightning and superbolts, for ionosphere-magnetosphere wave transmission, wave propagation in spa
242 ver to transport solar wind into the Earth's magnetosphere when the magnetopause features a large mag
243 sites along the sunward boundary of Earth's magnetosphere where the interplanetary magnetic field re
244 ectromagnetic waves pervasive in the Earth's magnetosphere, where they continuously remove or energiz
245 nalysis of 50-80 keV ENA images of Jupiter's magnetosphere, where two distinct emission regions domin
246 ronments such as black-hole and neutron-star magnetospheres, where accretion-powered jets and pulsar
247 rents flowing between the ionosphere and the magnetosphere which accelerate energetic charged particl
248 ods ranging from 1.3 to 1.6 years in Earth's magnetosphere, which can be associated with the solar QB
249 tional evidence of ring current in Mercury's magnetosphere, which has a significantly weaker dipole m
250 for the source of the missing energy is the magnetosphere, which injects energy mostly in the polar
251 an be compared with radio emissions from the magnetosphere, which is connected to the planet's interi
252 major compression and reconfiguration of the magnetosphere, which produces strong electric fields and
253 ly demonstrated by observations in Jupiter's magnetosphere, which--like that of Saturn (but unlike th
255 ntity that determines the interaction of the magnetosphere with the ionosphere, where the magnetosphe
257 ng the most dynamic phenomena in the Earth's magnetosphere, yet their triggering mechanisms remain un