P. H. Scherrer
- ORCiD
- https://orcid.org/0000-0002-6937-6968
- OpenAlex ID
- https://openalex.org/A5090533607 (API record)
Associated Concepts [?]
- Physics
- Quantum mechanics
- Astronomy
- Magnetic field
- Astrophysics
- Geology
- Geography
- Computer science
- Mathematics
- Nuclear physics
- Plasma
- Biology
- Optics
- Solar wind
- Meteorology
- Chemistry
- Engineering
- Sunspot
- Coronal mass ejection
- Computer vision
- Solar cycle
- Atmospheric sciences
Authored Works
sorted by decreasing year, and then by display-name
- Measuring the Large-scale Solar Magnetic Field
- The Olsen Rotating Dipole, Revisited
- Achieving Consistent Vector Magnetic Field Measurements from SDO/HMI
- The Sun From the Perspective of an Observer
- The height of flare emissions in white light and in hard X-rays
- Approach to Integrate Global-Sun Models of Magnetic Flux Emergence and Transport for Space Weather Studies
- Far-side seismic maps with HMI
- Estimating the Energy Flux of Acoustic-Gravity Waves in the Solar Atmosphere from SDO/HMI Data
- Access to Solar Dynamics Observatory HMI and AIA Data via the Joint Science Operations Center (JSOC)
- Quantitative Study of Solar Farside Observations to Predict Active Regions
- Data Management Techniques and Global Acess for the Space Weather Monitor Project of the IHY
- VLF Remote Sensing of the Lower Ionosphere: Solar Flares, Electron Precipitation, Sudden Ionospheric Disturbances, Sprites, Gravity Waves and Gamma-ray Flares
- The Sun-Earth Connection: How Ionospheric Monitoring can Engage and Inspire Students in Science and Engineering.
- Space Weather Monitors -- A Global Education and Small Instruments Program for the IHY 2007
- Characteristics of the Sun's polar magnetic flux from 1996-2005 using SOHO/MDI observations
- The Effect of the Differential Rotation of Photospheric Magnetic Features on Synoptic Frames of the Photospheric Magnetic Field
- The Stanford Solar Observatory Group E/PO Program
- Vector Magnetic Field Measurement Capabiliity of the Helioseismic and Magnetic Imager on SDO
- The Helioseismic and Magnetic Imager for the Solar Dynamics Observatory
- The Largest Active Region of the Solar Cycle
- Solar Coronal Structures in Extreme Ultraviolet and Soft X-rays and Their Relation to Magnetic Flux
- "All About the Sun" A Webcast With Audience Participation
Linked Co-Authors
Linked Collaborating Institutions
- Goddard Space Flight Center, Astrophysics Division
- Kirtland Air Force Research Laboratory, New Mexico
- Lockheed Martin, Palo Alto
- Los Alamos National Laboratory, New Mexico
- Michigan State University
- NASA Ames Research Center
- 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
- NorthWest Research Associates, Boulder
- Stanford University, California
- Stanford University, Department of Astronomy
- Stanford University, Department of Electrical Engineering
- Stanford University, Department of Physics
- University of California, Berkeley, Space Sciences Laboratory
- University of Cambridge, UK
- University of Hawaii, Manoa
- University of Michigan
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