Showing 1–20 of 20 results
/ Date/ Name
Nov 6, 2023A WISPR of the Venus Surface: Analysis of the Venus Nightside Thermal Emission at Optical WavelengthsAug 1, 2018Characterisation of the HD219134 multi-planet system II. Stellar-wind sputtered exospheres in rocky planets b & cDec 7, 2001Deuterium abundance toward G191-B2B: Results from the Far Ultraviolet Spectroscopic Explorer (FUSE) MissionJan 18, 2002Abundances of Deuterium, Nitrogen, and Oxygen toward HZ 43A: Results from the FUSE MissionMar 16, 2001FUSE Observations of CapellaJul 4, 2023Far beyond the Sun: II. Probing the stellar magnetism of the young Sun ι Horologii from the photosphere to its coronaNov 10, 2010Ultraviolet Coronagraph Spectroscopy: A Key Capability for Understanding the Physics of Solar Wind AccelerationJul 30, 2014Astrophysical Conditions for Planetary HabitabilityOct 26, 2021Galactic cosmic ray propagation through M dwarf planetary systemsAug 1, 2018Characterisation of the HD 219134 multi-planet system I. Observations of stellar magnetism, wind, and high-energy fluxMar 12, 2025Exploring coronal abundances of M dwarfs at moderate activity levelsMar 4, 2015Characterising exoplanets and their environment with UV transmission spectroscopyJul 29, 2017The Grad-Shafranov Reconstruction of Toroidal Magnetic Flux Ropes: First ApplicationsDec 7, 2001Deuterium Abundance Toward WD2211-495: Results from the Far Ultraviolet Spectroscopic Explorer (FUSE) MissionNov 19, 2008Comprehensive Observations of a Solar Minimum CME with STEREOJan 6, 2023Parker Solar Probe: Four Years of Discoveries at Solar Cycle MinimumDec 21, 2001Abundances of Deuterium, Oxygen, and Nitrogen in the Local Interstellar Medium: Overview of First Results from the Far Ultraviolet Spectroscopic Explorer MissionDec 12, 2001Deuterium Toward WD1634-573: Results from the Far Ultraviolet Spectroscopic Explorer (FUSE) MissionOct 12, 2022Connecting Solar and Stellar Flares/CMEs: Expanding Heliophysics to Encompass Exoplanetary Space WeatherJun 15, 2012A Coronal Hole's Effects on CME Shock Morphology in the Inner Heliosphere