ライフサイエンスコーパス: spacecraft

1 early 6 years of observations by the Cassini spacecraft.

2 the plasma-wave instrument on the Voyager 2 spacecraft.

3 , unmanned gliding vehicles and multisegment spacecraft.

4 he embedded dust belts imaged by the Voyager spacecraft.

5 ptured from Comet 81P/Wild 2 by the Stardust spacecraft.

6 and Ionospheric Sounding on the Mars Express spacecraft.

7 ariable at scales that may be sampled by the spacecraft.

8 ter suite of instruments on the Mars Odyssey spacecraft.

9 documented by the instruments on the Cassini spacecraft.

10 ov-Gerasimenko (67P), visited by the Rosetta spacecraft.

11 nstrument on board the orbiting Mars Express spacecraft.

12 g from Earth, and by the Voyager and Cassini spacecraft.

13 the plasma wave instrument on the Voyager 1 spacecraft.

14 lanetary environments on manned and unmanned spacecraft.

15 O observed in a global survey by the Odyssey spacecraft.

16 he Solar and Heliospheric Observatory (SOHO) spacecraft.

17 infrared during the swing-by of the Cassini spacecraft.

18 pectrometer onboard the Mars Global Surveyor spacecraft.

19 board the Solar and Heliospheric Observatory spacecraft.

20 s measured by an instrument on the Voyager 1 spacecraft.

21 tic electron bursts observed by near-Jupiter spacecraft.

22 ld, a task to be soon undertaken by the Juno spacecraft.

23 obability may require direct inspection by a spacecraft.

24 n the Long Duration Exposure Facility (LDEF) spacecraft.

25 ted with extra vehicular activity (EVA) from spacecraft.

26 ng two close fly-bys of Venus by the Cassini spacecraft.

27 lution images obtained by the NEAR-Shoemaker spacecraft.

28 traterrestrial life by modern interplanetary spacecraft.

29 area coverage of the few asteroids imaged by spacecraft.

30 n pose significant hazards to astronauts and spacecraft.

31 he Solar and Heliospheric Observatory (SOHO) spacecraft.

32 erved by the Magnetospheric Multiscale (MMS) spacecraft.

33 able for extreme environment applications in spacecraft.

34 le, in structural components of aircraft and spacecraft.

35 ity Recovery and Interior Laboratory (GRAIL) spacecraft.

36 n observed on many cometary nuclei mapped by spacecraft.

37 sions using the combined perspectives of two spacecraft.

38 would be ejected and could be measured by a spacecraft.

39 n the Mars Atmosphere and Volatile Evolution spacecraft.

40 nalysis mass spectrometer aboard the Rosetta spacecraft.

41 ts) of the SBN over the traditional monolith spacecraft.

42 bing a region that has never been visited by spacecraft.

43 rs Atmosphere and Volatile Evolution (MAVEN) spacecraft.

44 ic particle radiation environment inside the spacecraft.

45 roid Vesta, revealed in images from the Dawn spacecraft.

46 exploration activities and operations aboard spacecraft.

47 The Juno spacecraft acquired direct observations of the jovian ma

48 s first two flybys of Mercury, the MESSENGER spacecraft acquired images confirming that pervasive vol

49 On 27 August 2016, the Juno spacecraft acquired science observations of Jupiter, pas

50 and Neutral Analysis (ROSINA) on the Rosetta spacecraft analyzed the isotopes of xenon in the coma of

51 Laser Altimeter on the Mars Global Surveyor spacecraft and basal topography from the Mars Advanced R

52 in the hypersonic vehicle, rockets, re-entry spacecraft and defence sectors, but few materials can cu

53 nalyzed 19 years of data from remote-sensing spacecraft and forest inventories to identify the size a

54 2O ice) have been observed numerous times by spacecraft and ground-based telescopes, showing that clo

55 r Earth Asteroid Rendezvous (NEAR)-Shoemaker spacecraft and images of the asteroid's surface landmark

56 uch missions will require crew to transit in spacecraft and live in surface habitats that instantiate

57 Spacecraft and meteorite data now provide a global view

58 more than twice that observed by the Galileo spacecraft and modelled successfully.

59 olution images from the Mars Global Surveyor spacecraft and moderately high-resolution Thermal Emissi

60 - as part of instrumental suites on robotic spacecraft and planetary landers; this necessitates robu

61 To communicate, spacecraft and satellites rely on microwave devices, whi

62 sharply, according to the interpretation of spacecraft and stellar occultations.

63 However, spacecraft and telescope observations have been unable t

64 Observations by the Galileo spacecraft and the Keck telescope showed that Jupiter's

65 alogy Mapper instrument on the Chandrayaan-1 spacecraft and the Lunar Reconnaissance Orbiter Camera (

66 pace ENvironment, GEochemistry, and Ranging) spacecraft and the NASA Goddard Geophysical and Astronom

67 2) samples returned to Earth by the Stardust spacecraft appear to be weakly constructed mixtures of n

68 As the Shepherding Spacecraft approached the surface, it imaged a 25- to-30

69 larly important at the time when the Voyager spacecraft are leaving our heliosphere.

70 An international flotilla of spacecraft are to be sent to Mars over the next decade i

71 ound-based Doppler and range tracking of the spacecraft as well as spacecraft images of the asteroid'

72 comet 81P/Wild 2 collided with the Stardust spacecraft at 6.1 kilometers per second, producing hyper

73 nment, GEochemistry, and Ranging (MESSENGER) spacecraft at altitudes below 150 kilometers, we have de

74 ody, acquired during occultation by the Dawn spacecraft at asteroid Vesta.

75 al remote sensing instruments on the Cassini spacecraft at closest approach during a fly-by on 25-26

76 The flyby measurements of the Cassini spacecraft at Saturn's moon Rhea reveal a tenuous oxygen

77 onboard the European Space Agency's Rosetta spacecraft at scales of better than 0.8 meter per pixel

78 he dust detectors on the Ulysses and Galileo spacecrafts at heliocentric distances from 2 to 4 astron

79 mentation of the sunshade as a cloud of many spacecraft, autonomously stabilized by modulating solar

80 nment, GEochemistry, and Ranging (MESSENGER) spacecraft became the first probe to fly past the planet

81 The MESSENGER spacecraft began detecting energetic electrons with ener

82 ss mission, an aerobraking campaign took the spacecraft below the ionosphere into the very weakly ele

83 with comet Halley was provided by the Giotto spacecraft, but alternative interpretations exist.

84 graph is traded for the inconvenience of two spacecraft, but the daunting optics challenges are repla

85 by the Interstellar Boundary Explorer (IBEX) spacecraft, but they miss the ribbon.

86 The New Horizons spacecraft carried three instruments that measured the s

87 Images returned by the spacecraft Clementine have been used to produce a quanti

88 The Stardust spacecraft collected thousands of particles from comet 8

89 The Cassini spacecraft completed three close flybys of Saturn's enig

90 The Mars Science Laboratory spacecraft, containing the Curiosity rover, was launched

91 round Saturn bode well for the future as the spacecraft continues to orbit the planet.

92 c fields measured by Voyager 1 show that the spacecraft crossed or was crossed by the termination sho

93 lds measured by Voyager 1 (V1) show that the spacecraft crossed the boundary of an unexpected region

94 at 94.1 astronomical units, just before the spacecraft crossed the termination shock.

95 tribution of dust impacts indicates that the spacecraft crossed thin, densely populated sheets of par

96 Spacecraft data suggest that martian meteorites are not

97 experiments, and there is good evidence from spacecraft data that the process is active on asteroid s

98 More than 50 spacecraft debris particles were also identified.

99 As the spacecraft descended from 150 to 140 km altitude, the ma

100 rs Atmosphere and Volatile Evolution (MAVEN) spacecraft, detected auroral emission in virtually all n

101 resent data collected from Ulysses and other spacecraft during 1992-2002 and a variety of older measu

102 adio Doppler data generated with the Galileo spacecraft during its second encounter with Ganymede on

103 of Phoebe resulting from the Cassini-Huygens spacecraft encounter on 11 June 2004.

104 regime from 10(-14) to 10(-7) kilograms, the spacecraft encountered regions of intense swarms of part

105 t 26,000 images of the Jupiter system as the spacecraft encountered the giant planet en route to Satu

106 acecraft on 11 June 2004 (19 days before the spacecraft entered orbit around Saturn) provided an oppo

107 g of the health of all astronauts and of the spacecraft environment.

108 ar Earth Asteroid Rendevous (NEAR)-Shoemaker spacecraft executed a low-altitude flyover of asteroid 4

109 We argue that the spacecraft exited the supersonic solar wind and passed i

110 Spacecraft exploring Mars such as the Mars Exploration R

111 The Dawn spacecraft extensively imaged Vesta's surface, revealing

112 The Cassini Orbiter spacecraft first skimmed through the tenuous upper atmos

113 The Cassini spacecraft flew close to Saturn's small moon Enceladus t

114 The Near Earth Asteroid Rendezvous (NEAR) spacecraft flew within 3830 kilometers of asteroid 433 E

115 cent discovery of a binary asteroid during a spacecraft fly-by generated keen interest, because the o

116 An instrumented Shepherding Spacecraft followed a kinetic impactor and provided--fro

117 sured with Earth-orbiting and interplanetary spacecraft for 40 years.

118 measurement devices and it is widely used in spacecraft for its high accuracy.

119 s December 1990 fly-by of Earth, the Galileo spacecraft found evidence of abundant gaseous oxygen, a

120 The Galileo spacecraft found localized regions of strong northward a

121 is generally anhydrous, yet the Deep Impact spacecraft found the entire surface to be hydrated durin

122 Analysis of Dawn spacecraft Framing Camera image data allows evaluation o

123 The camera onboard the Cassini spacecraft has allowed us to observe many of Saturn's cl

124 The Cassini spacecraft has been in orbit around Saturn since 30 June

125 The Kepler spacecraft has been monitoring the light from 150,000 st

126 unched Interstellar Boundary Explorer (IBEX) spacecraft has completed its first all-sky maps of the i

127 The Galileo spacecraft has detected diffuse optical emissions from I

128 (MARSIS) instrument aboard the Mars Express Spacecraft has detected nadir echoes offset in time-dela

129 The Rosetta spacecraft has investigated comet 67P/Churyumov-Gerasime

130 on and Neutral Analysis) onboard the Rosetta spacecraft has measured the coma composition of comet 67

131 (VIR) mapping spectrometer onboard the Dawn spacecraft has now detected water absorption features wi

132 The Voyager 1 spacecraft has passed an important milestone.

133 The New Horizons spacecraft has performed a comprehensive search for kilo

134 Radio tracking of the MESSENGER spacecraft has provided a model of Mercury's gravity fie

135 pectrometer) instrument on board the Rosetta spacecraft has provided evidence of carbon-bearing compo

136 low from Dawn Framing Camera images.The Dawn spacecraft has provided orbital bistatic radar observati

137 A flotilla of subsequent spacecraft has redefined Mars from a volcanic planet to

138 NASA's New Horizons spacecraft has revealed the complex geology of Pluto and

139 Laser altimetry by the MESSENGER spacecraft has yielded a topographic model of the northe

140 The Huygens probe, launched from the Cassini spacecraft, has made the first direct observations of th

141 the Gravity Recovery and Interior Laboratory spacecraft have clarified the origin of lunar mass conce

142 Optical observations from the New Horizons spacecraft have identified lightning at high latitudes a

143 here made by instruments on the New Horizons spacecraft have implications for the stability and dynam

144 and contorted F ring returned by the Cassini spacecraft have revealed phenomena not previously detect

145 Recent data from the Cassini spacecraft have revealed that Enceladus, the 500-km-diam

146 Measurements by instruments on spacecraft have significantly advanced cosmochemistry.

147 ions have been observed, consistent with the spacecraft having crossed the termination shock into the

148 The spacecraft hovers near the asteroid, with its thrusters

149 s, et l'Activite (OMEGA) on the Mars Express spacecraft identify the distinct mafic, rock-forming min

150 The Galileo spacecraft imaged a pair of superimposed ripple patterns

151 range tracking of the spacecraft as well as spacecraft images of the asteroid's center of figure and

152 ity in the atmospheres of other planets from spacecraft images requires a knowledge of the optical pr

153 Mariner 9 and Viking spacecraft images revealed that the polar regions of Mar

154 roperties and jet activity from the Stardust spacecraft imaging and the onboard dust monitoring syste

155 diation of the Earth as measured by orbiting spacecraft in 1970 and 1997.

156 Images of Amalthea from two Voyager spacecraft in 1979 and Galileo imaging between November

157 Magnetometer data acquired by the MESSENGER spacecraft in orbit about Mercury permit the separation

158 Simultaneous measurements by more than ten spacecraft in the near-Earth environment reveal the evan

159 Each spacecraft in the network can have different subsystem c

160 entes have been observed by the New Horizons spacecraft in the Tartarus Dorsa region of Pluto (220 de

161 The Mars Global Surveyor spacecraft, in a highly elliptical polar orbit, obtained

162 es in technology have enabled telescopic and spacecraft instruments to provide important data that si

163 The Kepler spacecraft is monitoring more than 150,000 stars for evi

164 on the European Space Agency's Mars Express spacecraft is providing new constraints on the martian s

165 mapping altitude by the Mars Global Surveyor spacecraft, is presented here.

166 fter 40 close flybys of Titan by the Cassini spacecraft, it has become clear that no such oceans exis

167 Emission Imaging System on the Mars Odyssey spacecraft, it is possible to observe such heterogeneiti

168 highly variable within the potential Phoenix spacecraft landing ellipses, and is likely to be variabl

169 Spacecraft launched from Earth can transport hitchhiker

170 rs Atmosphere and Volatile Evolution (MAVEN) spacecraft made comprehensive measurements of the Mars u

171 The cameras aboard the Cassini spacecraft mainly observe small (1 to 10 micrometers) du

172 was recently explored by NASA's New Horizons spacecraft, making closest approach on 14 July 2015.

173 The New Horizons spacecraft mapped colors and infrared spectra across the

174 al-velocity plasma flow, indicating that the spacecraft may be close to the heliopause, the border be

175 launch opportunity, and at times up to four spacecraft may be operating simultaneously at the planet

176 As it is, Mars-bound spacecraft may frequently be contaminated with aspergill

177 e gamma ray spectrometer on the Mars Odyssey spacecraft measured an enhancement of atmospheric argon

178 ng its first flyby of Mercury, the MESSENGER spacecraft measured the planet's near-equatorial magneti

179 e after solar eruptions has been verified by spacecraft measurements near Earth, its formation on the

180 The Mars Phoenix spacecraft measurements of carbon isotopes [referenced t

181 with high spatial resolution, obtained from spacecraft measurements of infrared spectra of Jupiter's

182 New laboratory and spacecraft measurements strongly indicate that much of t

183 Spacecraft missions impose serious limitations on instru

184 aled in increasing detail by a succession of spacecraft missions.

185 n and Sensing Satellite (LCROSS) Shepherding Spacecraft monitored the impact and ejecta.

186 Using images acquired by the Chang'e-2 spacecraft, more than 200 boulders have been identified

187 e magnetometer data collected by the Galileo spacecraft near Io provide evidence of electromagnetic i

188 he reliability of the wireless links between spacecraft (nodes) to enable any survivability improveme

189 At Earth, multiple-spacecraft observations have been implemented to underst

190 Here we report Kepler spacecraft observations of a single Sun-like star, which

191 Here we report three-spacecraft observations of accelerated flow associated w

192 Here we report in situ two-spacecraft observations of bi-directional jets at the ma

193 Limited single-spacecraft observations of Jupiter's magnetopause have b

194 Here we report the combined spacecraft observations of Saturn acquired over one Satu

195 situ energy-specific and temporally resolved spacecraft observations reveal an isolated third ring, o

196 Previous single-spacecraft observations revealed only single jets at the

197 Spacecraft observations show that the presence of lightn

198 Spacecraft observations suggest that the plumes of Satur

199 gnetic field is different compared with past spacecraft observations.

200 r cap has remained enigmatic since the first spacecraft observations.

201 ations of supernova remnant W44 by the Fermi spacecraft observatory support the idea that the bulk of

202 On approach, the spacecraft observed frequent natural outbursts, a mean r

203 The New Horizons (NH) spacecraft observed Io's aurora in eclipse on four occas

204 The New Horizons spacecraft observed Jupiter's icy satellites Europa and

205 ansition Region and Coronal Explorer (TRACE) spacecraft observed the decaying transversal oscillation

206 maging Instrument (MIMI) onboard the Cassini spacecraft observed the saturnian magnetosphere from Jan

207 nt periodic structures in waves, the Cluster spacecraft observes 'ring' distributions of protons in v

208 s, the Near-Earth Asteroid Rendezvous (NEAR) spacecraft obtained 222 images of Eros, as well as suppo

209 In February and March 2007, the New Horizons spacecraft obtained a global snapshot of Io's volcanism.

210 Here we report the discovery by the Cassini spacecraft of a fast (>103[?]km[?]s-1) and hot magnetosp

211 s observations using the Cassini and Galileo spacecraft of hectometric radio emissions and extreme ul

212 We combine measurements made by the four spacecraft of the Magnetospheric Multiscale mission to d

213 Here we report a fortuitous crossing by a spacecraft of the plasma tail of comet Hyakutake (C/1996

214 lose fly-by of Phoebe by the Cassini-Huygens spacecraft on 11 June 2004 (19 days before the spacecraf

215 era and Spectrometer aboard the Deep Space 1 spacecraft on 22 September 2001.

216 e-based networks (SBNs) allow the sharing of spacecraft on-orbit resources, such as data storage, pro

217 nd is accordingly favoured as a location for spacecraft operation because of the benign environment.

218 iment on the European Space Agency's Rosetta spacecraft orbiting comet 67P/Churyumov-Gerasimenko.

219 uorescence spectra obtained by the MESSENGER spacecraft orbiting Mercury indicate that the planet's s

220 Data that were collected from the Polar spacecraft over the course of 1 year show that the flow

221 On 3 January 2000, the Galileo spacecraft passed close to Europa when it was located fa

222 In 2017, the Cassini spacecraft passed inside the planet's rings, allowing in

223 The Cassini spacecraft passed within 168.2 kilometers of the surface

224 System visible images from the Mars Odyssey spacecraft permit more comprehensive geologic and climat

225 or an outbreak of an infectious disease in a spacecraft presents one such concern, which is compounde

226 tandard ground timing allowed a solution for spacecraft range, range rate, and acceleration, as well

227 Since the Cassini spacecraft reached Saturn's orbit in 2004, its instrumen

228 olid state imaging experiment on the Galileo spacecraft returned more than 100 high-resolution (5 to

229 ued planetary scientists since the Mariner 9 spacecraft returned the first close-up image in 1972, bu

230 radio-communications between the ground and spacecraft returning to Earth.

231 ptured from comet 81P/Wild 2 by the Stardust spacecraft reveal indigenous aliphatic hydrocarbons simi

232 Instruments on the Cassini spacecraft reveal that a heat source within Saturn's moo

233 mera onboard the Mars Reconnaissance Orbiter spacecraft reveal that Athabasca Valles is now entirely

234 images of Mercury obtained by the MESSENGER spacecraft reveal that its surface has an overall relati

235 he Cosmic Dust Analyzer on board the Cassini spacecraft reveal that the Saturnian system is passed by

236 Data from the Kepler spacecraft reveal transits of the planet across both sta

237 ocal plasma flow speed is high, and near the spacecraft's closest approach, where atmospheric density

238 Radio Doppler data from the Galileo spacecraft's encounter with Amalthea, one of Jupiter's s

239 By using the Cassini spacecraft's gravitational data, along with Pioneer and

240 The Cassini spacecraft's in situ observations reveal that energetic

241 The MESSENGER spacecraft's observations of Mercury's ionized exosphere

242 ument onboard the Cassini Orbiter during the spacecraft's passage over the rings.

243 on dust impacts detected during the Galileo spacecraft's traversal of the outer ring region: we find

244 1998 until September 2005, when the Cassini spacecraft saw them reappear.

245 rstellar dust clouds, ballistic penetrators, spacecraft shielding and ductility in high-performance c

246 raRed Mapping Spectrometer on board the Dawn spacecraft show a clear detection of an organic absorpti

247 ti-jovian quadrant observed from the Galileo spacecraft show absorption features resulting from hydro

248 btained during the flyby of the New Horizons spacecraft show an unexpected lack of ultraviolet nightg

249 tary nuclei imaged from flyby and rendezvous spacecraft show common evidence of layered structures an

250 nment, GEochemistry, and Ranging (MESSENGER) spacecraft show decreases in the flux of epithermal and

251 om the Interstellar Boundary Explorer (IBEX) spacecraft show that the relative motion of the Sun with

252 nment, GEochemistry, and Ranging (MESSENGER) spacecraft, show that the spatial distribution of region

253 measurements of Ceres obtained from the Dawn spacecraft, showing that it is in hydrostatic equilibriu

254 The variations measured from spacecraft since 1978 are too small to have contributed

255 the Mercury Laser Altimeter on the MESSENGER spacecraft spans approximately 20% of the near-equatoria

256 The Rosetta spacecraft spent 2 years orbiting comet 67P/Churyumov-G

257 The Dawn spacecraft targeted 4 Vesta, believed to be a remnant in

258 aging science experiment onboard the Cassini spacecraft that address some of these issues.

259 We present a design concept for a spacecraft that can controllably alter the trajectory of

260 ions considered consist of several networked spacecraft that can tap into each other's Command and Da

261 from the European Space Agency Mars Express spacecraft that indicate that such lakes may still exist

262 We present observations by the Dawn spacecraft that reveal a heavily cratered surface, a het

263 ing Spectrometer (VIMS) on board the Cassini spacecraft, that strongly indicate that ethane, probably

264 was collected during passage of the Stardust spacecraft through the coma of comet 81P/Wild 2.

265 mical units from the Sun, becoming the first spacecraft to begin exploring the heliosheath, the outer

266 eutral Mass Spectrometer onboard the Cassini spacecraft to detect molecular hydrogen in the plume.

267 cs and Space Administration's (NASA) Cassini spacecraft to generate transit spectra.

268 on the European Space Agency's Venus Express spacecraft to identify compositional differences in lava

269 ity Recovery and Interior Laboratory (GRAIL) spacecraft to investigate the gravitational field of Ori

270 We used the spectrometer onboard the Dawn spacecraft to map their spatial distribution on the basi

271 Emission Spectrometer (TES) aboard the Aura spacecraft, to investigate aspects of the atmospheric hy

272 Spacecraft-to-spacecraft tracking observations from the

273 occasional temporary re-orientations of the spacecraft (totalling about 10-25 hours every 2 months)

274 onal perturbation on NEAR was evident in the spacecraft tracking data.

275 Spacecraft-to-spacecraft tracking observations from the Gravity Recove

276 The New Horizons spacecraft traversed the length of the jovian magnetotai

277 The New Horizons spacecraft traversed the magnetotail to distances exceed

278 The IMAGE spacecraft uses photon and neutral atom imaging and radi

279 and gravity field are derived from measured spacecraft velocity perturbations at fly-by distances be

280 Over the past five decades, however, spacecraft visits to many targets transformed these earl

281 in the solar wind have been measured by the spacecraft Voyager 1 and Voyager 2.

282 The spacecraft Voyager 1 is at a distance greater than 85 au

283 we show, based on observations from the NASA spacecraft Voyager and Cassini, that gases alone cannot

284 The NEAR-Shoemaker spacecraft was designed to provide a comprehensive chara

285 Recently, the Hinode spacecraft was launched to observe and measure the plasm

286 onitoring ppm levels of iodine and iodide in spacecraft water.

287 Iodine is used as a biocide in spacecraft water.

288 Using imaging from three spacecraft, we have mapped two global-scale organized co

289 Altimeter on the Mars Global Surveyor (MGS) spacecraft, we have measured temporal changes in the ele

290 d energy/charge spectrometers on the Cassini spacecraft, we have obtained evidence for tholin formati

291 (TEC) maps and measurements from the THEMIS spacecraft, we investigated simultaneous ionosphere and

292 By using data from the Kepler spacecraft, we report the detection of such a "self-lens

293 Using a conjunction between eight spacecraft, we show that this conversion takes place wit

294 1999 and February 2000 flybys of the Galileo spacecraft, were used to study the thermal structure and

295 erial was observed by a second "shepherding" spacecraft, which carried nine instruments, including ca

296 onnaissance Orbiter Camera (LROC) on the LRO spacecraft, which indicates the peak ring is composed of

297 r aboard the European Space Agency's Rosetta spacecraft, which is found to be (5.3 +/- 0.7) x 10(-4)-

298 combining data from the Voyager and Galileo spacecraft, which reveal bright, smooth terrains that li

299 At least two spacecraft will be sent at each launch opportunity, and

300 port the serendipitous encounter of the Wind spacecraft with an active reconnection diffusion region,