HelioWebInternational Space Science Institute, Switzerland
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I[International Space Science Institute, Switzerland]
PI["Parent Institutions (0)"]
CI["Child Institutions (0)"]
AW["Affiliated Works (73)"]
CA["Linked Collaborating Authors (22)"]
I== skos:broader ==>PI
CI== skos:broader ==>I
AW== affil ==>I
AW== author ==>CA
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Affiliated Works
sorted by decreasing year, and then by display-name
- Charge-to-Mass Fractionation during Injection into First-order Fermi Acceleration of Suprathermal Ions at an Interplanetary Shock
- Charge-to-mass fractionation during injection and acceleration of suprathermal particles associated with the Bastille Day event: SOHO/CELIAS/HSTOF data
- Temperatures and Temperature Anisotropies of Heavy Solar Wind Ions From Ulysses-SWICS
- Four spacecraft study of dipolarization-like signatures at the lobe/plasma sheet interface
- Latitude Dependence of Element Abundances in the Slow Solar Wind
- Charge states and abundances of heavy ions as signatures of interplanetary coronal mass ejections
- Enrichment of suprathermal <SUP>3</SUP>He<SUP>++</SUP> associated with interplanetary coronal mass ejection events
- Hydromagnetic Wave Excitation at a Heliospheric Shock
- Location of the termination shock: an attempt to reconcile recent Voyager observations with Ulysses/SWICS pickup ion data and other diagnostics
- Penetration of interstellar hydrogen, oxygen and nitrogen atoms into the heliosphere through the solar wind-LIC interaction region
- Solar wind composition measurements during one entire solar cycle
- Variability of N/O in the Solar Wind
- A Model For EUV Flux Throughout The 3-Dimensional Heliosphere
- An Extension of the Quasi-linear Theory on Shock Acceleration to Low-energy Ions
- Are Inner Source Pickup Ions further Accelerated in Interplanetary Space?
- Composition of Interplanetary Coronal Mass Ejections at Very High Latitudes
- Momentum Diffusion of Suprathermal Ions in Compressional Solar Wind Turbulence
- The Holocene Total Solar Irradiance Based on <SUP>10</SUP>Be Extracted From Ice Core
- Variability of the Nitrogen Abundance in the Solar Wind and Implications for Past Solar Activity
- Ion Acceleration and Wave-Particle Interaction at the Interplanetary Shocks Associated with the Halloween 2003 and the 20 January 2005 Events: SOHO/HSTOF, SOHO/EPHIN, and ACE/MAG Observations.
- Is the solar wind termination shock a cosmic-ray mediated shock?
- Modeling of the heliospheric interface: multi-component model of the heliospheric plasma
- The Role of Gypsum in the Mars North Polar Region
- Thermal Properties of Heavy Ions throughout the Heliosphere: 39 Solar Wind Species from Ulysses-SWICS
- Large-scale heliospheric structure in 2004-2006 and its solar origin
- The Composition of the Solar Wind
- Ulysses Transition into the Newly Formed Southern Fast Stream Observed with Ulysses- SWICS
- Ulysses Transition into the Polar Coronal Holes
- Magnetic turbulence in space plasmas: scale dependent effects of anisotropy
- Multi-spacecraft synergy with MEX HRSC and MRO SHARAD: Light-Toned Deposits in crater bulges
- Quiescent Current Sheets in the Solar Wind and Origins of Slow Wind
- Solar EUV Spectral Irradiance Throughout The 3-Dimensional Heliosphere
- Solar Wind MHD Turbulence for Different Phases of the Solar Cycle
- Spatial and Temporal Analysis of Magnetic Helicity in the Solar Wind
- Characterization of short time transitions in the solar wind
- Multi-Spacecraft Observation Of Small-Scale Anisotropy In The Solar Wind Turbulence
- Polar Coronal Holes during the Past Solar Cycle: Ulysses Observations
- Examination of the Earth's Radiation budget using satellite observations and modeling data
- Oxygen Flux in the Solar Wind: Ulysses Observations
- Scaling Properties Of Small-Scale Anisotropy In The Solar Wind Turbulence By Multipoint Measurements
- Scaling properties of the reduced magnetic helicity in the near Earth' space
- Solar wind cross-helicity and residual energy during different solar cycles
- Variability of the solar wind
- Mass flows between the chromosphere and corona - comparison of 1D and 3D coronal loop models
- Origin of the most strongly FIP-fractionated solar wind: Ulysses SWICS results
- Tracking Solar Active Region Outflow Plasma from its Source to the near-Earth Environment
- A Rigorous Statistical Approach to Determine Solar Wind Composition from ACE/SWICS Data, and New Ne/O Ratios
- Solar Wind Abundances From Ulysses-SWICS
- GIADA On-Board Rosetta: Early Dust Grain Detections and Dust Coma Characterization of Comet 67P/C-G
- Solar Corona/Wind Composition and Origins of the Solar Wind
- Temporal evolution of the snow density near the surface at Dome C on Antarctica Plateau
- The role of the heliosphere for interstellar dust trajectories - revisited
- Tracking the direction of the interstellar wind over a full solar cycle using pickup ions detected by ACE SWICS
- Coma dust environment observed by GIADA during the Perihelion of 67P/Churyumov-Gerasimenko.
- New insights in the interstellar dust properties and its interaction with the heliosphere from data, simulations and experiments
- Slow Solar Wind: Observable Characteristics for Constraining Modelling
- Total Land Water Storage Change over 2003-2013 Estimated from a Global Mass Budget Approach
- Variations in Solar Wind Fractionation as Seen by ACE/SWICS Over a Full Solar Cycle and the Implications for Genesis Mission Results
- Fundamental Physics of the Slow Solar Wind - What do we Know?
- Solar Metallicity Derived from In-Situ Solar Wind Composition
- Influence of the surface permeability on the GRACE water mass variations. Case of the Lake Chad basin.
- Observing pre-earthquake features in the Earth atmosphere-ionosphere environment associated with 2017 Tehuantepec and Puebla earthquakes in Mexico
- Porosity Gradient at the Surface of Comet 67P/Churyumov-Gerasimenko
- Migrating Scarps in the Hapi Region on Comet 67P/Churyumov-Gerasimenko
- Small Satellites for Space Science (4S) COSPAR Roadmap
- Migrating Scarps as a Significant Driver for Cometary Mass Loss
- The Heat Flow and Physical Properties Package HP<SUP>3</SUP> on InSight: Status and First Results
- The VALKYRIE Payload for Probing the Martian Subsurface
- Interannual variability in the rate of the global mean sea level rise
- Properties of the top Forty Centimeters of the Martian soil From HP3 Mole Penetration and Thermal Conductivity Measurements
- Sea-level fingerprints due to ongoing land ice melting in altimetry-based sea-level data
- A 6-7 year cycle in the Earth System
- Land/Ocean Surface Diversity on Earth-like (Exo)planets: Implications for Habitability