HelioWebHaosheng Lin
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A[Haosheng Lin]
AC["Associated Concepts (25)"]
AW["Authored Works (16)"]
CA["Linked Co-Authors (1)"]
CI["Linked Collaborating Institutions (14)"]
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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- ORCiD
- https://orcid.org/0000-0002-4504-3165
- OpenAlex ID
- https://openalex.org/A5005340549 (API record)
Associated Concepts [?]
- Physics
- Quantum mechanics
- Optics
- Astronomy
- Magnetic field
- Astrophysics
- Geography
- Geology
- Biology
- Computer science
- Remote sensing
- Telescope
- Chemistry
- Solar telescope
- Astrobiology
- Scattering
- Plasma
- Nuclear physics
- Computer vision
- Spectral line
- Solar wind
- Polarimetry
- Materials science
- Meteorology
- Medicine
Authored Works
sorted by decreasing year, and then by display-name
- Tomographic Measurements of Magnetic Free Energy in CME Source Regions
- Retrieving 3D Coronal Magnetic Field from Spectropolarimetry of Coronal Emission Lines.
- 3D Global Coronal Density, Temperature, and Vector Magnetic Field Derived from Coronal Observation.
- The Coronal Solar Magnetism Observatory
- The Coronal Solar Magnetism Observatory (COSMO)
- 3D Coronal Magnetic Field Reconstruction Based on Infrared Polarimetric Observations
- Reconstruction of the 3D Coronal Magnetic Field by Vector Tomography with Infrared Spectropolarimetric Observations from CoMP
- Vector Tomography Inversion for the 3D Coronal Magnetic Field Based on CoMP data
- Testing the vector tomography method for 3D reconstruction of the coronal magnetic field for different coronal field models
- Magnetic Field Measurements at the Photosphere and Coronal Base
- On the reconstructing the coronal magnetic field from Fe XIII 10747 A emission line observations
- The COronal Solar Magnetism Observatory
- The Coronal Solar Magnetic Observatory (COSMO)
- Coronal Magnetic Field Measurements and Comparison with Theoretical Model
- Using Imaging Infrared Coronal Spectropolarimetry to Measure the Near-Sun Plasma
- Measuring Coronal Magnetic Fields with Coronal Emission Line Polarimetry
Linked Co-Authors
Linked Collaborating Institutions
- Catholic University, Department of Physics
- Catholic University, Washington DC
- George Mason University, Virginia
- Max-Planck-Institute for Solar System Research, Lindau
- NASA Goddard Space Flight Center, Maryland
- National Center for Atmospheric Research, Colorado
- National Center for Atmospheric Research, High Altitude Observatory
- National Solar Observatory, Sunspot New Mexico
- Observatoire Mid Pyrenees, France
- Smithsonian Astrophysical Observatory
- University of Hawaii, Manoa
- University of Hawaii, Manoa, Institute for Astronomy
- University of Michigan
- University of Michigan, Department of Atmospheric Oceanic and Space Sciences
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