Noé Lugaz
University of New Hampshire, University of Hawai'i at Manoa Institute for Astronomy, University of Michigan, ISAE-Supaéro
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Solar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Stellar, planetary, and galactic studies
About
Research Professor working on coronal mass ejections, their initiation, propagation, interaction, and effects on Earth magnetosphere and radiation belts. Former Editor-in-Chief of AGU's Space Weather journal (2019–2025). Chair of the SHINE steering committee (2019–2024). Lead of the IMAP Student Collaboration 3UCubed CubeSat (2020–2025).
At the University of New Hampshire since 2012, as a research faculty since 2013. 2014 Arne Richter award for outstanding young scientist of the European Geosciences Union.
Employment
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University of New Hampshire Research Professor2022 - Present
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University of New Hampshire Research Associate Professor2016 - 2022
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University of New Hampshire Research Assistant Professor2013 - 2016
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University of New Hampshire Research Scientist2012 - 2013
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University of Hawai'i at Manoa Institute for Astronomy Assistant Astronomer (research)2009 - 2012
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University of Hawai'i at Manoa Institute for Astronomy Post-doc2007 - 2009
Education
- 2002 - 2007
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ISAE-Supaéro MEng2000 - 2003
Projects & Funding
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The Sheath and Duration of Coronal Mass Ejections: Multi-Spacecraft Studies National Aeronautics and Space Administration2024 - 2028
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SCIENCE ORGANIZING COMMITTEE MEMBERSHIP FOR THE HELIOPHYSICS 2050 WORKSHOP National Aeronautics and Space Administration2021 - 2022
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How are Magnetospheric Field and Plasmas Impacted by Impulsive Changes in Interplanetary Parameters? National Aeronautics and Space Administration2020 - 2024
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Student Collaboration of the Interstellar Mapping and Acceleration Probe: Phases B to F National Aeronautics and Space Administration2020 - 2025
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The Radial Expansion of Coronal Mass Ejections: Combined Views from Remote and In situ Observations National Aeronautics and Space Administration2020 - 2025
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SUCCESSIVE CORONAL MASS EJECTIONS AND ASSOCIATED SOLAR ENERGETIC PARTICLES National Aeronautics and Space Administration2019 - 2024
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PHYSICAL ORIGINS OF SUPRATHERMAL ION POPULATIONS THROUGHOUT THE HELIOSPHERE National Aeronautics and Space Administration2017 - 2022
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SHINE Workshop Coordination: 2016-2020 National Science Foundation - Directorate for Geosciences2016 - 2021
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Collaborative Research: Reconciliation Between In-situ and Remote Sensing Analyses National Science Foundation - Directorate for Geosciences2015 - 2018
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Collaborative Research: SHINE: Data-constrained Simulations of Coronal Mass Ejection Initiation and Propagation National Science Foundation - Directorate for Geosciences2015 - 2018
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Complex Coronal Mass Ejection Structures and Associated Geo-effectiveness National Science Foundation - Directorate for Geosciences2015 - 2018
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SHINE Workshop Coordination for the Period during January 1, 2010 to December 31, 2014 National Science Foundation2014 - 2016
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NUMERICAL INVESTIGATION OF CME EVOLUTION IN THE CORONA AND INNER HELIOSPHERE AND HOW IT DETERMINES CME PROPERTIES AT IAU National Aeronautics and Space Administration2013 - 2016
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SHINE: The Non-Ideal Evolution of Coronal Mass Ejections: Numerical Studies National Science Foundation2012 - 2012
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SHINE: The Non-Ideal Evolution of Coronal Mass Ejections: Numerical Studies National Science Foundation2012 - 2015
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Collaborative Research: Numerical Investigation of CME-CME Interaction and Associated Effects from the Low Corona to 1 AU National Science Foundation2012 - 2015
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NUMERICAL INVESTIGATION OF CME EVOLUTION IN THE CORONA AND INNER HELIOSPHERE AND HOW IT DETERMINES CME PROPERTIES AT IAU (HAWAII) National Aeronautics and Space Administration2011 - 2014
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NSWP: Numerical Investigation of Coronal Mass Ejection (CME) Cannibalism in the Inner Heliosphere and Its Implications for Space Weather National Science Foundation2008 - 2012
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STUDYING COMPELX EJECTA AT L1 USING REALISTIC MODELS OF CME EVOLUTION AND INTERPLANETARY MAGNETIC FIELD National Aeronautics and Space Administration2008 - 2012
Publications (181)
- Can Alfvénic Fluctuations Affect the Correlation and Complexity of Magnetic Field of Magnetic Ejecta? A Case Study Based on Multi-spacecraft Measurements at 1 au Save
- Commitment to Advance Excellence and Inclusion in the Earth and Space Sciences Scholarly Publications Save
- First Observations of a Geomagnetic Superstorm With a Sub-L1 Monitor Save
- Heliospheric Turbulence: Presidential Budget Request Offers a Bleak Forecast for Space Weather Research Save
- Influence of the Deformation of Coronal Mass Ejections on Their in-Situ Fitting with Circular-Cross-Section Flux Rope Models Save
- Investigating Coronal Mass Ejections through Multispacecraft Measurements: STEREO-A and L1 in 2022-2023 Save
- Space Weather Into the 2030s: The 2024 Solar and Space Physics Decadal Survey Save
- The Magnetic Field Structure of Coronal Mass Ejections: A More Realistic Representation Save
- The Need for a Sub-L1 Space Weather Research Mission: Current Knowledge Gaps on Coronal Mass Ejections Save
- The evolution of CME sheath turbulence from L1 to Earth: Wind and MMS observations of the 2023-04-23 CME Save
- A Survey of Coronal Mass Ejections Measured In Situ by Parker Solar Probe during 2018-2022 Save
- Acceleration and Release of Solar Energetic Particles Associated with a Coronal Shock on 2021 September 28 Observed by Four Spacecraft Save
- Characterization of Small Flux Ropes Using Juno Spacecraft Cruise-phase Data Save
- Combining STEREO heliospheric imagers and Solar Orbiter to investigate the evolution of the 2022 March 10 CME Save
- Discrepancies in the Properties of a Coronal Mass Ejection on Scales of 0.03 au as Revealed by Simultaneous Measurements at Solar Orbiter and Wind: The 2021 November 3–5 Event Save
- Exploring the Impact of the Aging Effect on Inferred Properties of Solar Coronal Mass Ejections Save
- Measurements of Magnetic Cloud Expansion through Multiple Spacecraft in Radial Conjunction Save
- Observation of a Fully-formed Forward-Reverse Shock Pair due to the Interaction between Two Coronal Mass Ejections at 0.5 au Save
- On the Role of Alfvénic Fluctuations as Mediators of Coherence within Interplanetary Coronal Mass Ejections: Investigation of Multi-spacecraft Measurements at 1 au Save
- Thank You to Our Peer Reviewers in 2023 Save