Search Results - "Rouillard, P."
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Modeling the Formation and Evolution of Solar Wind Microstreams: From Coronal Plumes to Propagating Alfvénic Velocity Spikes
Published in The Astrophysical journal (01-12-2023)“…Abstract We investigate the origin of mesoscale structures in the solar wind called microstreams, defined as enhancements in the solar wind speed and…”
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A Multiple Flux-tube Solar Wind Model
Published in The Astrophysical journal (01-04-2017)“…We present a new model, MULTI-VP, which computes the three-dimensional structure of the solar wind and includes the chromosphere, the transition region, and…”
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Evidence for a Coronal Shock Wave Origin for Relativistic Protons Producing Solar Gamma-Rays and Observed by Neutron Monitors at Earth
Published in The Astrophysical journal (01-04-2020)“…We study the solar eruptive event on 2017 September 10 that produced long-lasting >100 MeV γ-ray emission and a ground level enhancement (GLE72). The origin of…”
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DERIVING THE PROPERTIES OF CORONAL PRESSURE FRONTS IN 3D: APPLICATION TO THE 2012 MAY 17 GROUND LEVEL ENHANCEMENT
Published in The Astrophysical journal (10-12-2016)“…ABSTRACT We study the link between an expanding coronal shock and the energetic particles measured near Earth during the ground level enhancement of 2012 May…”
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Near-Sun observations of an F-corona decrease and K-corona fine structure
Published in Nature (London) (12-12-2019)“…Remote observations of the solar photospheric light scattered by electrons (the K-corona) and dust (the F-corona or zodiacal light) have been made from the…”
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Magnetized Winds of M-type Stars and Star–Planet Magnetic Interactions: Uncertainties and Modeling Strategy
Published in The Astrophysical journal (01-11-2024)“…Abstract M-type stars are the most common stars in the Universe. They are ideal hosts for the search of exoplanets in the habitable zone (HZ), as their small…”
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Extended 3He-rich Time Periods Observed by Solar Orbiter: Magnetic Connectivity and Sources
Published in The Astrophysical journal (01-10-2023)“…Observations of Solar Energetic Particles (SEPs) using the Suprathermal Ion Spectrograph (SIS), which is part of the Energetic Particle Detector suite on the…”
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Multispacecraft observation of magnetic cloud erosion by magnetic reconnection during propagation
Published in Journal of Geophysical Research (01-09-2012)“…During propagation, Magnetic Clouds (MC) interact with their environment and, in particular, may reconnect with the solar wind around it, eroding away part of…”
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Statistical study of magnetic cloud erosion by magnetic reconnection
Published in Journal of geophysical research. Space physics (01-01-2015)“…Several recent studies suggest that magnetic reconnection is able to erode substantial amounts of the outer magnetic flux of interplanetary magnetic clouds…”
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Spatial and temporal variation in New Hampshire bat diets
Published in Scientific reports (22-08-2022)“…Insectivorous bats consume a diverse array of arthropod prey, with diets varying by bat species, sampling location, and season. North American bat diets remain…”
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The Rise and Fall of Open Solar Flux During the Current Grand Solar Maximum
Published in The Astrophysical journal (01-08-2009)Get full text
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The very slow solar wind: Properties, origin and variability
Published in Journal of geophysical research. Space physics (01-04-2016)“…Solar wind slower than 300 km/s, hereafter termed very slow solar wind (VSSW), is seldom observed at 1 AU. It was, however, commonly measured inside 0.7 AU by…”
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First imaging of corotating interaction regions using the STEREO spacecraft
Published in Geophysical research letters (01-05-2008)“…Plasma parcels are observed propagating from the Sun out to the large coronal heights monitored by the Heliospheric Imagers (HI) instruments onboard the NASA…”
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THE LONGITUDINAL PROPERTIES OF A SOLAR ENERGETIC PARTICLE EVENT INVESTIGATED USING MODERN SOLAR IMAGING
Published in The Astrophysical journal (10-06-2012)“…We use combined high-cadence, high-resolution, and multi-point imaging by the Solar-Terrestrial Relations Observatory (STEREO) and the Solar and Heliospheric…”
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CMEs in the Heliosphere: I. A Statistical Analysis of the Observational Properties of CMEs Detected in the Heliosphere from 2007 to 2017 by STEREO/HI-1
Published in Solar physics (01-05-2018)“…We present a statistical analysis of coronal mass ejections (CMEs) imaged by the Heliospheric Imager (HI) instruments on board NASA’s twin-spacecraft STEREO…”
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Stereoscopic imaging of an Earth‐impacting solar coronal mass ejection: A major milestone for the STEREO mission
Published in Geophysical research letters (01-04-2009)“…We present stereoscopic images of an Earth‐impacting Coronal Mass Ejection (CME). The CME was imaged by the Heliospheric Imagers onboard the twin STEREO…”
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A synoptic view of solar transient evolution in the inner heliosphere using the Heliospheric Imagers on STEREO
Published in Geophysical research letters (01-01-2009)“…By exploiting data from the STEREO/heliospheric imagers (HI) we extend a well‐established technique developed for coronal analysis by producing time‐elongation…”
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Excess open solar magnetic flux from satellite data: 2. A survey of kinematic effects
Published in Journal of Geophysical Research. A. Space Physics (01-11-2009)“…We investigate the “flux excess” effect, whereby open solar flux estimates from spacecraft increase with increasing heliocentric distance. We analyze the…”
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Interpreting the Properties of Solar Energetic Particle Events by Using Combined Imaging and Modeling of Interplanetary Shocks
Published in The Astrophysical journal (01-07-2011)“…Images of the solar corona obtained by the Solar-Terrestrial Relations Observatory (STEREO) provide high-cadence, high-resolution observations of a compression…”
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Effects of solar wind magnetosphere coupling recorded at different geomagnetic latitudes: Separation of directly-driven and storage/release systems
Published in Geophysical research letters (01-11-2008)“…The effect on geomagnetic activity of solar wind speed, compared with that of the strength of the interplanetary magnetic field, differs with geomagnetic…”
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