Skip to content

QUICK FIELD:

Search Database

SoFT: Detecting and tracking magnetic structures in the solar photosphere

Authors

Berretti, M.;
RefereedArticle

Abstract

In this work, we present Solar Feature Tracking, a novel feature-tracking tool developed in Python and designed to detect, identify, and track magnetic elements in the solar atmosphere. It relies on a watershed segmentation algorithm to effectively detect magnetic clumps within magnetograms, which are then associated across successive frames to follow the motion of magnetic structures in the photosphere. Here, we study its reliability in detecting and tracking features under different noise conditions starting with real-world data observed with SDO/HMI and followed with simulation data obtained from the Bifrost numerical code to better replicate the movements and shape of actual magnetic structures observed in the Sun's atmosphere within a controlled noise environment.

Details

© The SAO Astrophysics Data System

help[at]scixplorer.org

SciX is a project created by the Astrophysics Data System (ADS), which is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative Agreement 80NSSC21M0056.

Version: v0.46.4

*The material contained in this document is based upon work supported by a National Aeronautics and Space Administration (NASA) grant or cooperative agreement. Any opinions, findings, conclusions or recommendations expressed in this material are those of the author and do not necessarily reflect the views of NASA.

RESOURCES

About SciXGive FeedbackSciX HelpSystem StatusCareers@SciXAccessibility Conformance ReportWeb Accessibility PolicyNASA Science Discovery Engine