SWASTi-SW: Space Weather Adaptive SimulaTion framework for Solar Wind and its relevance to ADITYA-L1 mission
Prateek Mayank, Bhargav Vaidya, D. Chakrabarty

TL;DR
This paper introduces SWASTi-SW, a 3D solar wind simulation framework that integrates coronal and heliospheric models to improve space weather prediction relevant to the upcoming Aditya-L1 mission.
Contribution
It presents a novel integrated 3D solar wind model combining semi-empirical and physics-based approaches for enhanced space weather forecasting.
Findings
Validated with multiple Carrington rotations.
Demonstrated effects of heat ratio variation on solar wind.
Simulated stream interaction regions for Aditya-L1 observations.
Abstract
Solar wind streams, acting as background, govern the propagation of space weather drivers in the heliosphere, which induce geomagnetic storm activities. Therefore, predictions of the solar wind parameters are the core of space weather forecasts. This work presents an indigenous three-dimensional (3D) Solar Wind model (SWASTi-SW). This numerical framework for forecasting the ambient solar wind is based on a well-established scheme that uses a semi-empirical coronal model and a physics-based inner heliospheric model. This study demonstrates a more generalized version of Wang-Sheeley-Arge (WSA) relation, which provides a speed profile input to the heliospheric domain. Line-of-sight observations of GONG and HMI magnetograms are used as inputs for the coronal model, which in turn, provides the solar wind plasma properties at 0.1 AU. These results are then used as an initial boundary…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Ionosphere and magnetosphere dynamics · Geophysics and Gravity Measurements
