about
Isotope ratios of H, C, and O in CO2 and H2O of the martian atmospherePenitentes as the origin of the bladed terrain of Tartarus Dorsa on Pluto.Early MAVEN Deep Dip campaign reveals thermosphere and ionosphere variability.MAVEN observations of the response of Mars to an interplanetary coronal mass ejection.High-altitude dust layers on Mars: Observations with the Thermal Emission SpectrometerThe impact of a realistic vertical dust distribution on the simulation of the Martian General CirculationObservations of planetary waves and nonmigrating tides by the Mars Climate SounderMission to the Trojan asteroids: Lessons learned during a JPL Planetary Science Summer School mission design exerciseThe Vertical Dust Profile Over Gale Crater, MarsWinds measured by the Rover Environmental Monitoring Station (REMS) during the Mars Science Laboratory (MSL) rover's Bagnold Dunes Campaign and comparison with numerical modeling using MarsWRFThe effect of dust on the martian polar vorticesAtmospheric tides in Gale Crater, MarsMars Orbiter Camera climatology of textured dust stormsGeneral circulation models of the dynamics of Pluto’s volatile transport on the eve of the New Horizons encounterSeasonal variations in Pluto’s atmospheric tidesInfluence of water ice clouds on nighttime tropical temperature structure as seen by the Mars Climate SounderThermal tides during the 2001 Martian global-scale dust stormThe vertical distribution of Martian aerosol particle sizeEffects of the MY34/2018 Global Dust Storm as Measured by MSL REMS in Gale Crater
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description
researcher ORCID ID = 0000-0003-1149-7385
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wetenschapper
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name
Scott D. Guzewich
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Scott Guzewich
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type
label
Scott D. Guzewich
@en
Scott Guzewich
@nl
altLabel
S D Guzewich
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S. D. Guzewich
@en
S. Guzewich
@en
S.D. Guzewich
@en
Scott D Guzewich
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Scott Guzewich
@en
prefLabel
Scott D. Guzewich
@en
Scott Guzewich
@nl
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P31
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0000-0003-1149-7385