ライフサイエンスコーパス: spacecraft

1 oposed in order to bound the altitude of the spacecraft.

2 ity Recovery and Interior Laboratory (GRAIL) spacecraft.

3 n observed on many cometary nuclei mapped by spacecraft.

4 sions using the combined perspectives of two spacecraft.

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

6 n the Mars Atmosphere and Volatile Evolution spacecraft.

7 nalysis mass spectrometer aboard the Rosetta spacecraft.

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

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

10 creened here were recovered from actual Mars spacecraft.

11 ic particle radiation environment inside the spacecraft.

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

13 exploration activities and operations aboard spacecraft.

14 early 6 years of observations by the Cassini spacecraft.

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

16 , unmanned gliding vehicles and multisegment spacecraft.

17 he embedded dust belts imaged by the Voyager spacecraft.

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

19 and Ionospheric Sounding on the Mars Express spacecraft.

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

21 ter suite of instruments on the Mars Odyssey spacecraft.

22 documented by the instruments on the Cassini spacecraft.

23 to predict measurements from a second/third spacecraft.

24 nstrument on board the orbiting Mars Express spacecraft.

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

26 the plasma wave instrument on the Voyager 1 spacecraft.

27 lanetary environments on manned and unmanned spacecraft.

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

29 he Solar and Heliospheric Observatory (SOHO) spacecraft.

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

31 pectrometer onboard the Mars Global Surveyor spacecraft.

32 ion using data collected by the New Horizons spacecraft.

33 t high altitudes (~5300 km) by the MESSENGER spacecraft.

34 ntification, and Security-Regolith Explorer) spacecraft.

35 nditions, and subsequently could contaminate spacecraft.

36 rs Atmosphere and Volatile Evolution (MAVEN) spacecraft.

37 eme conditions, such as those encountered by spacecraft.

38 ervations of the main rings from the Cassini spacecraft.

39 erved by the Magnetospheric Multiscale (MMS) spacecraft.

40 rs Atmosphere and Volatile Evolution (MAVEN) spacecraft.

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

42 nd attractors, which bound the motion of the spacecraft.

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

44 able for extreme environment applications in spacecraft.

45 le, in structural components of aircraft and spacecraft.

46 stronomical units) of the Parker Solar Probe spacecraft(13), each lasting ten days.

47 particle population en route to more distant spacecraft(6).

48 The Juno spacecraft acquired direct observations of the jovian ma

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

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

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

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

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

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

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

56 Spacecraft and meteorite data now provide a global view

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

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

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

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

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

62 However, spacecraft and telescope observations have been unable t

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

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

65 horizontal offset distance between the Fermi spacecraft and the TGF source.

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

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

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

69 The Cassini spacecraft arrived at Saturn in 2004, dropped the Huygen

70 The Hayabusa2 spacecraft arrived at the near-Earth carbonaceous astero

71 esearch on growth of microorganisms found in spacecraft assembly clean rooms under simulated Martian

72 onate filter assemblies were deployed in the spacecraft assembly cleanroom facility to collect fallou

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

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

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

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

77 d by spacecraft near Earth(2,3) and later by spacecraft at heliocentric distances as small as 62 sola

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

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

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

81 pressure on the growth of chemoorganotrophic spacecraft bacteria and whether the addition of Mars rel

82 versity of chemoorganotrophic and culturable spacecraft bacteria do not grow under the tested conditi

83 None of the 125 spacecraft bacteria showed active growth under the teste

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

85 The MESSENGER spacecraft began detecting energetic electrons with ener

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

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

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

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

90 The OSIRIS-REx spacecraft carries a sophisticated suite of instruments

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

92 The Stardust spacecraft collected thousands of particles from comet 8

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

94 ill help to determine the biological load of spacecraft components and will also have direct relevanc

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

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

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

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

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

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

101 Spacecraft data suggest that martian meteorites are not

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

103 More than 50 spacecraft debris particles were also identified.

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

105 , particle size and roughness are beyond the spacecraft design specifications.

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

107 From its pole-to-pole orbit, the Juno spacecraft discovered arrays of cyclonic vortices in pol

108 The Cassini spacecraft discovered lakes/seas on Titan, however, it d

109 the final phase of the Cassini mission, the spacecraft dived between the planet and its innermost ri

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

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

112 ophic bacteria typically recovered from Mars spacecraft during planetary protection bioburden screeni

113 The Magnetospheric Multiscale (MMS) spacecraft encounter an electron diffusion region (EDR)

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

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

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

117 In this work, it is shown how a spacecraft equipped with a thrust and subjected to a dra

118 Spacecraft exploring Mars such as the Mars Exploration R

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

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

121 On 1 January 2019, the New Horizons spacecraft flew close to (486958) 2014 MU(69), a cold cl

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

123 In January 2019, the New Horizons spacecraft flew past one of these objects, the 36-kilome

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

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

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

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

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

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

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

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

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

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

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

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

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

137 The Hayabusa2 spacecraft has obtained global multicolor images of Ryug

138 The Voyager 1 spacecraft has passed an important milestone.

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

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

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

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

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

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

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

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

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

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

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

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

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

152 Measurements by instruments on spacecraft have significantly advanced cosmochemistry.

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

154 thermal infrared imager (TIR)(4) onboard the spacecraft Hayabusa2(5), indicating that the asteroid's

155 The spacecraft hovers near the asteroid, with its thrusters

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

157 The Galileo spacecraft imaged a pair of superimposed ripple patterns

158 During its 1989 flyby, the Voyager 2 spacecraft imaged six small moons of Neptune, all with o

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

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

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

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

163 New observations from spacecraft in orbit allowed an estimation of gross carbo

164 on scale magnetic cavity observed by the MMS spacecraft in the magnetosheath.

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

166 Each spacecraft in the network can have different subsystem c

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

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

169 The Hayabusa2 spacecraft investigated the small asteroid Ryugu, which

170 orms of perturbations in the altitude of the spacecraft is also investigated in this work, like the s

171 pecific set of parameters of the thrust, the spacecraft is bounded to a given altitude.

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

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

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

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

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

177 ations, Geodesy and Heat Transport (InSight) spacecraft landed successfully on Mars and imaged the su

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

179 Spacecraft launched from Earth can transport hitchhiker

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

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

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

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

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

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

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

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

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

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

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

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

192 Spacecraft missions impose serious limitations on instru

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

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

195 maging 3D distribution functions during fast spacecraft motion, we also discuss the operation strateg

196 ersonic solar wind(1) was first confirmed by spacecraft near Earth(2,3) and later by spacecraft at he

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

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

199 Here, we show, using spacecraft observations and particle-in-cell (PIC) simul

200 By using fortuitous multipoint spacecraft observations during a rare isolated fast plas

201 Here we show that spacecraft observations during this period were highly s

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

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

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

205 We validated the theory by spacecraft observations of the strong, compressional mag

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

207 Spacecraft observations suggest that the plumes of Satur

208 Because of the lack of in-situ spacecraft observations, the onset mechanism of magnetot

209 gnetic field is different compared with past spacecraft observations.

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

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

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

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

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

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

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

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

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

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

220 ection from Ryugu's surface by the Hayabusa2 spacecraft on 21 February 2019.

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

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

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

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

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

226 The Cassini spacecraft passed within 168.2 kilometers of the surface

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

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

229 a-ray Burst Monitor (GBM) on board the Fermi spacecraft provided the energetic radiation measurements

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

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

232 and Security-Regolith Explorer (OSIRIS-REx) spacecraft recently arrived at the near-Earth asteroid (

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

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

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

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

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

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

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

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

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

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

243 The New Horizons spacecraft's encounter with the cold classical Kuiper Be

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

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

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

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

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

249 1998 until September 2005, when the Cassini spacecraft saw them reappear.

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

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

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

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

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

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

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

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

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

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

260 The Rosetta spacecraft spent 2 years orbiting comet 67P/Churyumov-Ge

261 d, and oligotrophic in nature for assembling spacecraft subsystems.

262 and Security-Regolith Explorer (OSIRIS-REx) spacecraft surveyed Bennu's immediate environment, photo

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

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

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

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

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

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

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

270 solid state passive switchable radiator for spacecraft thermal control have been performed in a simu

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

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

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

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

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

276 use data obtained from the orbiting Akatsuki spacecraft to investigate how the super-rotation is main

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

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

279 lize magnetic cavity observations by one MMS spacecraft to predict measurements from a second/third s

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

281 Spacecraft-to-spacecraft tracking observations from the

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

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

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

285 The New Horizons spacecraft traversed the magnetotail to distances exceed

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

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

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

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

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

291 n the Mars Atmosphere and Volatile Evolution spacecraft, we demonstrate that water is instead transpo

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

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

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

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

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

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

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

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

300 bservations of lightning flashes by the Juno spacecraft with energies of approximately 10(5)-10(8) jo