JH
J. Todd Hoeksema
Also known as: Todd Hoeksema, J. T. Hoeksema
Stanford University, Calvin University
Research areas: Physics and Astronomy · Astronomy and Astrophysics · Solar and Space Plasma Dynamics · Stellar, planetary, and galactic studies · Ionosphere and magnetosphere dynamics
Employment
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Stanford University Professor of Physics (Research)1984 - Present
Education
- ? - 1984
- ? - 1978
Projects & Funding
Projects & funding information is unavailable.
Publications (136)
- Synoptic Maps of Solar Magnetic Field and Open Magnetic Flux Save
- Stray Light Correction for the Helioseismic and Magnetic Imager Save
- Toward a Consensus for Multi-Sourced Photospheric Line-of-Sight Magnetic Field Cross-Calibration Save
- Three Years of Making COFFIES Save
- Ensemble Kalman Filter Data Assimilation into the Surface Flux Transport Model to Infer Surface Flows: An Observing System Simulation Experiment Save
- The Dependence of Joy’s Law and Mean Tilt as a Function of Flux Emergence Phase Save
- MHD Parameters of Solar Active Regions for Solar Flare Forecasting Save
- SuperSynthIA: Physics-ready Full-disk Vector Magnetograms from HMI, Hinode, and Machine Learning Save
- The Relationship between Kinetic and Magnetic Helicity in Solar Active Regions Save
- The Sun’s Large-Scale Flows I: Measurements of Differential Rotation & Torsional Oscillation Save
- Vol. 55, Issue 3 (Heliophysics 2024 Decadal Whitepapers) Save
- Vol. 55, Issue 3 (Heliophysics 2024 Decadal Whitepapers) Save
- Vol. 55, Issue 3 (Heliophysics 2024 Decadal Whitepapers) Save
- Vol. 55, Issue 3 (Heliophysics 2024 Decadal Whitepapers) Save
- Vol. 55, Issue 3 (Heliophysics 2024 Decadal Whitepapers) Save
- Vol. 55, Issue 3 (Heliophysics 2024 Decadal Whitepapers) Save
- Large-scale Spatial Cross-calibration of Hinode/SOT-SP and SDO/HMI Save
- Editorial: Connecting solar flows and fields to understand surface magnetism Save
- Solaris: A Focused Solar Polar Discovery-class Mission to achieve the Highest Priority Heliophysics Science Now Save
- The Dependence of Joy’s Law as a Function of Flux Emergence Phase Save