Optimization of Curvi-Linear Tracing Applied to Solar Physics and Biophysics
arXiv:1307.5046 · doi:10.3390/e15083007
Abstract
We developed an automated pattern recognition code that is particularly well suited to extract one-dimensional curvi-linear features from two-dimensional digital images. A former version of this {\sl Oriented Coronal CUrved Loop Tracing (OCCULT)} code was applied to spacecraft images of magnetic loops in the solar corona, recorded with the NASA spacecraft {\sl Transition Region And Coronal Explorer (TRACE)} in extreme ultra-violet wavelengths. Here we apply an advanced version of this code ({\sl OCCULT-2}) also to similar images from the {\sl Solar Dynamics Observatory (SDO)}, to chromospheric H- images obtained with the {\sl Swedish Solar Telescope (SST)}, and to microscopy images of microtubule filaments in live cells in biophysics. We provide a full analytical description of the code, optimize the control parameters, and compare the automated tracing with visual/manual methods. The traced structures differ by up to 16 orders of magnitude in size, which demonstrates the universality of the tracing algorithm.
Entropy, Special Issue on Advanced Signal Processing in Heliospheric Physics, (in press)
Cited by in corpus (17)
- Global Energetics of Solar Flares: I. Magnetic Energies
- The Width Distribution of Loops and Strands in the Solar Corona -- Are we Hitting Rock Bottom ?
- The Magnetic Field of Active Region 11158 During the 2011 February 12-17 Flares : Differences between Photospheric Extrapolation and Coronal Forward-Fitting Methods
- The Vertical Current Approximation Nonlinear Force-Free Field Code - Description, Performance Tests, and Measurements of Magnetic Energies Dissipated in Solar Flares
- Driving Solar Spicules and Jets with Magnetohydrodynamic Turbulence: Testing a Persistent Idea
- Tracing the Chromospheric and Coronal Magnetic Field with AIA, IRIS, IBIS, and ROSA Data
- Comparison of Two Coronal Magnetic Field Models for Reconstructing a Sigmoidal Solar Active Region With Coronal Loops
- Statistical Relation between Solar Flares and Coronal Mass Ejections with Respect to Sigmoidal Structures in Active Regions
- Automated Spatiotemporal Analysis of Fibrils and Coronal Rain using the Rolling Hough Transform
- Magnetic Energy Dissipation during the 2014 March 29 Solar Flares
- The Magnetic Properties of Heating Events on High-Temperature Active Region Loops
- Towards a Quantitative Comparison of Magnetic Field Extrapolations and Observed Coronal Loops
- Blind Stereoscopy of the Coronal Magnetic Field
- Chromospheric magnetic field: A comparison of He I 10830 A observations with nonlinear force-free field extrapolation
- Helical Twisting Number and Braiding Linkage Number of Solar Coronal Loops
- Torsional Alfvénic Oscillations Discovered in the Magnetic Free Energy During Solar Flares
- Searching for signatures of H spicule-like features in the solar transition region