HelioWebB. Gallardo‐Lacourt
flowchart
A[B. Gallardo‐Lacourt]
AC["Associated Concepts (19)"]
AW["Authored Works (16)"]
CA["Linked Co-Authors (35)"]
CI["Linked Collaborating Institutions (18)"]
A== dcterms:relation ==>AC
AW== author ==>A
AW== author ==>CA
AW== affil ==>CI
click AC "#associated-concepts"
click AW "#authored-works"
click CA "#co-authors"
click CI "#collaborating-institutions"
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NO["add outgoing edge"]
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A-- ? -->NO
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- ORCiD
- https://orcid.org/0000-0003-3690-7547
- OpenAlex ID
- https://openalex.org/A5054921715 (API record)
Associated Concepts [?]
- Physics
- Geology
- Quantum mechanics
- Astronomy
- Geography
- Geophysics
- Nuclear physics
- Meteorology
- Magnetic field
- Plasma
- Magnetosphere
- Ionosphere
- Engineering
- Substorm
- Mathematics
- Computer science
- Atmospheric sciences
- Geodesy
- Aerospace engineering
Authored Works
sorted by decreasing year, and then by display-name
- aurora-asi-lib: A User-Friendly Auroral All-Sky Imager Analysis Library
- Utilizing optical flow technique to understand plasma convection
- Systems Understanding of Cross-scale Magnetotail Dynamics
- Resolving the Unique Characteristics of Substorms that Precede Strong Thermal Emission Velocity Enhancement (STEVE) Events using Incoherent Scatter Radar and Spacecraft Observations
- Polar Cap Boundary Identification Using Redline Optical Data and DMSP Satellite Particle Data
- New Insight into the Transition from a SAR Arc to STEVE
- Magnetospheric Observations of Dawnside Storm-time Wedge Current Systems
- Interaction between Subauroral Proton Aurora, SAR Arcs and SAPS Unveiled by Citizen Scientist Photographs
- An examination of magnetosphere-ionosphere-thermosphere coupling during STEVE
- A SAR arc evolving into STEVE during extreme subauroral plasma conditions
- The Association of Relativistic Electron Microbursts with The Aurora
- Signatures of STEVE in SuperDARN HF backscatter data
- Polar Cap Boundary identification using redline optical data and DMSP satellite particle data
- High Latitude Ionospheric Electrodynamics during STEVE and Non-STEVE Substorm Events
- Analyzing plasma convection using optical flow technique: from the aurora to the solar wind
- A review of the physical processes of meso-scale dynamic auroral forms
Linked Co-Authors
- A. J. Halford
- A. S. Reimer
- Alan Dyer
- B. Kunduri
- C. Forsyth
- C. R. Martinis
- D. J. Knudsen
- D. M. Gillies
- E. Spanswick
- G. W. Perry
- H. U. Frey
- J. B. Baker
- J. G. Sample
- J. Liang
- J. M. Ruohoniemi
- J. Wroten
- Kareem Sorathia
- L. Kepko
- L. M. Kilcommons
- L. W. Blum
- Leonardo Regoli
- Lindsay Goodwin
- M. Shumko
- P. J. Erickson
- Pablo Reyes
- R. M. Millan
- S. B. Mende
- S. Ohtani
- Simon Wing
- T. Motoba
- Tomoko Matsuo
- V. G. Merkin
- Vassilis Angelopoulos
- William Archer
- Y. Nishimura
Linked Collaborating Institutions
- Boston University, Massachusetts
- Dartmouth College, New Hampshire
- Haystack Observatory
- Johns Hopkins University, Applied Physics Laboratory
- Los Alamos National Laboratory, New Mexico
- Montana State University, Bozeman
- NASA Goddard Space Flight Center, Maryland
- Nagoya University, Japan
- New Jersey Institute of Technology
- Saint Petersburg State University, Russia
- Stanford Research Institute, California
- University College London, Mullard Space Science Laboratory
- University of Calgary, Canada
- University of California, Berkeley
- University of California, Los Angeles
- University of Colorado, Boulder
- University of Saskatchewan, Canada
- Virginia Polytechnic Institute and State University
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