HelioWebDaniel B. Seaton
flowchart
A[Daniel B. Seaton]
AC["Associated Concepts (24)"]
AW["Authored Works (24)"]
CA["Linked Co-Authors (64)"]
CI["Linked Collaborating Institutions (46)"]
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click AW "#authored-works"
click CA "#co-authors"
click CI "#collaborating-institutions"
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- ORCiD
- https://orcid.org/0000-0002-0494-2025
- OpenAlex ID
- https://openalex.org/A5012320864 (API record)
Associated Concepts [?]
- Physics
- Quantum mechanics
- Astronomy
- Astrophysics
- Magnetic field
- Plasma
- Nuclear physics
- Biology
- Solar wind
- Engineering
- Coronal mass ejection
- Geology
- Computer science
- Astrobiology
- Geography
- Optics
- Venus
- Corona (planetary geology)
- Aerospace engineering
- Mathematics
- Materials science
- Meteorology
- Solar flare
- Computer vision
Authored Works
sorted by decreasing year, and then by display-name
- The COMPLETE mission concept for comprehensive 3D understanding of coronal magnetic energy storage and release
- Strategies for Modern, Multi-dimensional Data: Case Studies from PUNCH, CubIXSS, ECCCO, SunCET, & COMPLETE
- Single and Multiple Vantage Point 3D Coronal Reconstruction with the CROBAR Method
- Resolving CME Characteristics with Polarized PUNCH Data
- Real-Time Operational Measurements of the Thermospheric State: Recent Advances and Future Possibilities
- Prominence Eruption Observed in He II 304 Å up to >6 Solar Radii by EUI/FSI Aboard Solar Orbiter
- Preparing for the 2024 Total Solar Eclipse with Citizen CATE
- Pathfinding Solar Tomography for Future Missions via Model Data Reconstruction
- Magnetic Field Reconnection as the Source of the Solar wind
- Leveraging the Citizen CATE 2017 Eclipse Experience to Build CATE 2024
- Following a prominence eruption from the Sun to Parker Solar Probe with multi-spacecraft observations
- ECCCO: The EUV CME and Coronal Connectivity Observatory
- A New Universal Polarization Resolving Software Package for Solar Coronal and Heliospheric Observations
- Understanding the coronal origins of global heliospheric phenomena through 3D measurements with COMPLETE
- Understanding Solar Eruptions, Solar Wind Formation, and how the Sun Connects to the Heliosphere through a Polar Perspective
- Tracing the Drivers of Slow Solar Wind in the Middle Corona
- Towards a Coherent View of the Sun/Corona/Heliosphere: Combining Remote Sensing Data Products with PSP In Situ Measurements
- The Multiview Observatory for Solar Terrestrial Science (MOST)
- The COMPLETE mission concept for the Heliophysics Decadal Survey
- Small-Scale Solar Activity and its effect on the coronal environment
- SWAP and the Middle Corona
- Polarimeter to Unify the Corona and Heliosphere (PUNCH) Science Operations Center (SOC) Design and Data Products
- Exploring the middle corona: new instrumentation to address science questions critical to understanding the thermal structure and dynamic evolution of the middle corona
- Direct First PSP Observation Of The Interaction Of Two Successive Interplanetary Coronal Mass Ejections On November 2020
Linked Co-Authors
- A. K. Higginson
- A. N. Zhukov
- A. W. Case
- Albert Y. Shih
- Ali Rahmati
- Amir Caspi
- Ayris Narock
- B. J. Thompson
- Brian E. Wood
- C. A. Madsen
- Chris Lowder
- Christopher Moore
- Cooper Downs
- D. E. McKenzie
- D. Lario
- David B. Wexler
- Donald M. Hassler
- E. A. Jensen
- E. E. DeLuca
- E. K. Sutton
- E. Thiemann
- Erika Palmerio
- J. C. Kasper
- J. F. Drake
- J. Marcus Hughes
- Jason Kooi
- Jeffrey Newmark
- Jia Huang
- K. E. Korreck
- K. W. Paulson
- Krishna M. Jain
- L. F. Guedes dos Santos
- L. Golub
- L. P. Chitta
- M. I. Desai
- M. L. Mays
- Marc L. DeRosa
- Marie Dominique
- Matthew J. West
- N. E. Raouafi
- N. Gopalswamy
- N. M. Viall
- Nathalia Alzate
- Nishu Karna
- Pete Riley
- Phillip Hess
- Qian Gong
- S. C. Tripathy
- S. D. Bale
- S. E. Gibson
- S. F. Fung
- S. Parenti
- S. Tomczyk
- S. Yashiro
- Sabrina Savage
- Sarah A. Kovac
- Silvina Guidoni
- Simone Di Matteo
- T. A. Kucera
- T. N. Woods
- Tatiana Niembro
- Teresa Nieves‐Chinchilla
- V. M. Uritsky
- Yeimy Rivera
Linked Collaborating Institutions
- Aberystwyth University, UK
- Academy of Sciences of the Czech Republic, Astronomical Institute
- Atmospheric & Space Technology Research Associates (ASTRA)
- Catholic University, Washington DC
- George Mason University, Virginia
- Imperial College, London
- Institut d'Astrophysique Spatiale
- Institut d'Astrophysique de Paris
- Jet Propulsion Laboratory
- Johns Hopkins University, Applied Physics Laboratory
- Johns Hopkins University, Maryland
- Lockheed Martin, Palo Alto
- Max-Planck-Institute for Solar System Research, Lindau
- NASA Goddard Space Flight Center, Maryland
- NASA HQ
- NASA Marshall Space Flight Center
- National Autonomous University of Mexico
- National Center for Atmospheric Research, Colorado
- National Centers for Environmental Information
- National Solar Observatory, Sunspot New Mexico
- New Jersey Institute of Technology
- New Mexico State University
- Planetary Science Institute, Arizona
- Predictive Science Inc., California
- Royal Observatory of Belgium
- Royal Observatory of Belgium, Department of Solar Physics
- Smithsonian Astrophysical Observatory
- Southwest Research Institute, Boulder
- Southwest Research Institute, Texas
- Stanford University, California
- U.S. Department of the Navy, Naval Research Laboratory, Washington DC
- University College London, UK
- University of Alcala, Spain
- University of California, Berkeley
- University of California, Berkeley, Space Sciences Laboratory
- University of California, Los Angeles, Institute of Geophysics and Planetary Physics
- University of Cambridge, UK
- University of Colorado, Boulder
- University of Colorado, Boulder, Laboratory for Atmospheric and Space Physics
- University of Florence, Italy
- University of Ljubljana, Slovenia
- University of Maryland, College Park
- University of Michigan
- University of Minnesota, Twin Cities
- University of Northern Colorado
- University of Paris-Saclay, France
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