HelioWebMausumi Dikpati
flowchart
A[Mausumi Dikpati]
AC["Associated Concepts (25)"]
AW["Authored Works (16)"]
CA["Linked Co-Authors (15)"]
CI["Linked Collaborating Institutions (24)"]
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"]
NI-- ? -->A
A-- ? -->NO
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click NO "#add-outgoing-edge"
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style NO stroke-width:2px,stroke-dasharray: 5 5
- ORCiD
- https://orcid.org/0000-0002-2227-0488
- OpenAlex ID
- https://openalex.org/A5004609547 (API record)
Associated Concepts [?]
- Physics
- Quantum mechanics
- Magnetic field
- Geography
- Astronomy
- Dynamo
- Meteorology
- Astrophysics
- Plasma
- Nuclear physics
- Geology
- Computer science
- Mechanics
- Thermodynamics
- Computer vision
- Stars
- Dynamo theory
- Solar dynamo
- Convection zone
- Convection
- Climatology
- Atmospheric sciences
- Magnetohydrodynamics
- Differential rotation
- Solar wind
Authored Works
sorted by decreasing year, and then by display-name
- Rossby waves in the solar tachocline: nonlinear interactions and instabilities
- Penetration of tachocline Rossby waves through the convection zone to the surface
- Optimal low-dimensional representation of solar tachocline dynamics
- Observations and Simulations of Solar Flows and Their Roles in Magnetic Activity Patterns at the Surface
- Migration of Low Latitude Long Lived Coronal Holes in the McA: An Analysis of Rossby Waves Based on Coronal Hole Drift Speeds
- Magnetohydrodynamics Instabilities of Double Magnetic Bands in a Shallow-water Tachocline Model
- What Deep and Extended Minima Tell us about Magnetism Below the Surface?
- Symmetry-reduced dynamic mode decomposition of solar tachocline dynamics
- Spatio-temporal Drifts of Long-lived Equatorial Coronal Holes: Do they follow the Local Differential Rotation or Rossby Waves?
- Periodic behaviors of white-light faculae
- Origin of Rossby waves observed near the solar surface
- Observational evidence of spot-producing magnetic ring's split during MHD evolution
- Interactions Among Magnetic Bands in Extended Solar Cycles
- Information Horizon of Magnetic Active Regions
- Impact of Time-varying High-latitude Meridional Circulation Cell in Polar Fields
- Global solar flows and their impact on magnetic activity
Linked Co-Authors
- A. A. Norton
- B. Belucz
- Bradley W. Hindman
- Breno Raphaldini
- Ian Hewins
- Krishna M. Jain
- Lisa Upton
- Moritz Linkmann
- R. Erdélyi
- Robert J. Leamon
- S. C. Tripathy
- S. E. Gibson
- Scott W. McIntosh
- Simon Wing
- Subhamoy Chatterjee
Linked Collaborating Institutions
- Aberystwyth University, UK
- Andrews University, Michigan
- Boston College, Massachusetts
- Eotvos Lorand University, Hungary
- Federal University of Minas Gerais, Brazil
- Hungarian Academy of Sciences
- Johns Hopkins University, Applied Physics Laboratory
- Karl Franzens University of Graz, Austria
- Max-Planck-Institute for Solar System Research, Lindau
- NASA HQ
- National Center for Atmospheric Research, Colorado
- National Center for Atmospheric Research, High Altitude Observatory
- National Solar Observatory, Sunspot New Mexico
- New Jersey Institute of Technology
- New York University
- NorthWest Research Associates, Boulder
- Southwest Research Institute, Boulder
- Stanford University, California
- University Corporation for Atmospheric Research, Colorado
- University of Colorado, Boulder
- University of Edinburgh, UK
- University of Sao Paulo, Brazil
- University of Sheffield, UK
- Vellore Institute of Technology, India
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