Development of a 3D non-kinematic dynamo model for the solar and stellar cycles
Implementing Organization
Indian Institute of Technology (IIT), Varanasi, Uttar Pradesh
Principal Investigator
Dr. Bidya Binay Karak
Indian Institute Of Technology (Bhu), Uttar Pradesh
About
The reversal of the Sun's magnetic field and sun-like stars is a mysterious feature of nature. The amplitude of the magnetic field varies each cycle, suggesting a nonlinear interaction between convective plasma and rotation and magnetic field. Most existing solar dynamo models are kinematic, relying on observations and theoretical models. A proposed project aims to develop a 3D non-kinematic solar dynamo model based on the magnetohydrodynamics model, solving flow and thermodynamic perturbations and using mean flows from observations. This model will be used to study solar and stellar magnetic cycles.
Source
Source
Anusandhan National Research Foundation/Science and Engineering Research Board (SERB), DST 2023-24
Science and Engineering Research Board (SERB), New Delhi
Anusandhan National Research Foundation (ANRF)
Quick Information
Area of Research
Astronomy & Space Sciences
Focus Area
Astrophysics
Start Year
2024
End Year
2027
Sanction Amount
₹ 6.60 L
Status
Ongoing
Contact
karak.phy@iitbhu.ac.in
Output
No. of Research Paper
00
Technologies (If Any)
00
No. of PhD Produced
00
No. of Patents
Filed :00
Grant :00
Disclaimer:
Information available on this portal is sourced from various organizations and is provided for informational purposes only. Users are advised to verify details from the respective official sources.
Please enter your details
Please provide your name and email to continue. Your details are saved in this browser for future use.
Latest Updates
Loading…
⚠️
You are leaving this website
You are about to be redirected to an external website that is not operated by
India Science, Technology & Innovation (ISTI) Portal.
Indian Institute of Technology (IIT), Varanasi, Uttar Pradesh
Acces sibility Controls