{"id":387,"date":"2023-03-12T23:44:56","date_gmt":"2023-03-12T21:44:56","guid":{"rendered":"https:\/\/mosaiics.astro.bas.bg\/?page_id=387"},"modified":"2023-03-20T12:04:42","modified_gmt":"2023-03-20T10:04:42","slug":"machine-learning-and-computer-vision-in-heliophysics-2023","status":"publish","type":"page","link":"https:\/\/mosaiics.astro.bas.bg\/?page_id=387","title":{"rendered":""},"content":{"rendered":"\n<div class=\"wp-block-cover\" style=\"min-height:401px\"><span aria-hidden=\"true\" class=\"wp-block-cover__background has-background-dim-0 has-background-dim\"><\/span><img decoding=\"async\" loading=\"lazy\" width=\"1920\" height=\"1080\" class=\"wp-block-cover__image-background wp-image-223\" alt=\"\" src=\"https:\/\/mosaiics.astro.bas.bg\/wp-content\/uploads\/2022\/11\/MSH2023_1920x1080-2.jpg\" data-object-fit=\"cover\" srcset=\"https:\/\/mosaiics.astro.bas.bg\/wp-content\/uploads\/2022\/11\/MSH2023_1920x1080-2.jpg 1920w, https:\/\/mosaiics.astro.bas.bg\/wp-content\/uploads\/2022\/11\/MSH2023_1920x1080-2-300x169.jpg 300w, https:\/\/mosaiics.astro.bas.bg\/wp-content\/uploads\/2022\/11\/MSH2023_1920x1080-2-1024x576.jpg 1024w, https:\/\/mosaiics.astro.bas.bg\/wp-content\/uploads\/2022\/11\/MSH2023_1920x1080-2-768x432.jpg 768w, https:\/\/mosaiics.astro.bas.bg\/wp-content\/uploads\/2022\/11\/MSH2023_1920x1080-2-1536x864.jpg 1536w\" sizes=\"(max-width: 1920px) 100vw, 1920px\" \/><div class=\"wp-block-cover__inner-container\">\n<p class=\"has-text-align-center has-large-font-size\"><\/p>\n<\/div><\/div>\n\n\n\n<h3 class=\"has-text-align-center\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\">INTERNATIONAL WORKSHOP ON <\/mark><\/strong><br><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\">MACHINE LEARNING AND COMPUTER VISION <\/mark><\/strong><br><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\">IN HELIOPHYSICS<\/mark><\/strong><br><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\">19-21 April, 2023<\/mark><\/strong><br><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\">Sofia, Bulgaria<\/mark><\/strong><br><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\">and online<\/mark><\/strong><\/h3>\n\n\n\n<div class=\"is-layout-flex wp-block-buttons\">\n<div class=\"wp-block-button has-custom-font-size has-small-font-size\"><a class=\"wp-block-button__link has-black-color has-pale-cyan-blue-background-color has-text-color has-background wp-element-button\" href=\"https:\/\/mosaiics.astro.bas.bg\/?page_id=165\" style=\"border-radius:20px\">Back<\/a><\/div>\n<\/div>\n\n\n\n<div style=\"height:28px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<h4 class=\"has-text-align-center has-medium-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\">Wednesday, April 19, 2023<\/mark><\/strong><\/h4>\n\n\n\n<h4 class=\"has-medium-font-size\"><strong>8:30 \u2013 9:00 Registration and Introduction<\/strong><\/h4>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>09:00 \u2013 09:40<\/strong> <strong>(Invited) <\/strong>Michele Piana \u2013 <em>Artificial intelligence for space weather forecasting: data-driven and physics-informed approaches in research and operational settings<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\">Session 1 \u2013 Machine Learning \/ Computer Vision Techniques<\/mark><\/strong><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>09:40 \u2013 10:00 <\/strong>Vanessa Mercea \u2013 <em>A Machine Learning Enhanced Approach for Automated Sunquake Detection in Acoustic Emission Maps<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>10:00 \u2013 10:20 <\/strong>Francesco Pio Ramunno \u2013 <em>Modeling Solar Images from SDO\/AIA with Denoising Diffusion Models<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>10:20 \u2013 10:40<\/strong> Manuel Luna \u2013 <em>Towards a technique for automatic detection and characterisation of oscillations in solar filaments<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\">10:40 \u2013 11:20 Coffee Break<\/mark><\/strong><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>11:20 \u2013 11:40 <\/strong>Connor O&#8217;Brien \u2013 <em>Non-Deterministic Models of Solar Wind Propagation from L1 to the Earth<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>11:40 \u2013 12:00<\/strong> Jeremiah Scully \u2013 <em>Mitigation of Radio Frequency Interference in Solar Radio observations using Generative Adversarial Networks<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>12:00 \u2013 12:20<\/strong> Matthew Lennard \u2013 <em>Fast Feature Recovery for Flux Emergence Forecasting in the Photosphere using Neural Networks<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>12:20 \u2013 12:40<\/strong> Juan Esteban Agudelo Ortiz \u2013 <em>Deep Learning techniques implementation for the generation of stokes parameters and atmospheric parameters in the solar context<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\">12:40 \u2013 14:20 Lunch<\/mark><\/strong><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>14:20 \u2013 14:40<\/strong> Talha Siddique \u2013 <em>A Cluster of Machine Learning Enabled Magnetometer System For Online Training And Prediction of Geomagnetic Disturbances<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>14:40 \u2013 15:00 <\/strong>Gonzalo Cucho-Padin \u2013 <em>Three-dimensional reconstruction of ion flux in the Earth\u2019s northern cusp based on artificial neural networks<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>15:00 \u2013 15:20 <\/strong>Daniel Carpenter \u2013 <em>A Customized Distance Metric for Explainable In-Situ Solar Wind Clustering<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>15:20 \u2013 15:40<\/strong> Andong Hu \u2013 <em>Multi-Hour-Ahead Geoelectric Fields Forecast Using Multi-fidelity Machine Learning Method<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>15:40 \u2013 16:20<\/strong> <strong>Coffee Break<\/strong><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>16:20 \u2013 17:00 (Invited) <\/strong>Enrico Camporeale \u2013<strong> <\/strong><em>Data-Driven Discovery of Fokker-Planck Equation for the Earth&#8217;s Radiation Belts Electrons Using Physics-Informed Neural Networks<\/em><\/mark>\u00a0<\/p>\n\n\n\n<p class=\"has-medium-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\">Session 2 \u2013 Machine Learning \/ Computer Vision Applications in Heliophysics<\/mark><\/strong><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>17:00 \u2013 17:20 <\/strong>Spyros Kasapis \u2013 <em>Turning Noise into Data: Characterization of the Van Allen Radiation Belt Using SDO Spikes Data<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>17:20 \u2013 17:40<\/strong> Ricardo Gafeira \u2013 <em>PCA-NN model for TEC with space weather parameters as predictors: tuning of NN algorithms and input parameters<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>17:40 \u2013 18:00<\/strong> Benoit Tremblay \u2013 <em>SuNeRFs: The Sun as a (fully-resolved) Star<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\">18:00 \u2013 20:00 Reception&nbsp;<\/mark><\/strong><\/p>\n\n\n\n<h4 class=\"has-text-align-center has-medium-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\">Thursday April 20, 2023<\/mark><\/strong><\/h4>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\">Session 2 \u2013 Machine Learning \/ Computer Vision Applications in Heliophysics<\/mark><\/strong><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>9:00 \u2013 9:40 (Invited) <\/strong>Athanasios Papaioannou \u2013 <em>Predicting Solar Activity (flares, CMEs &amp; SEPs) using Machine-Learning<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>9:40 \u2013 10:00 <\/strong>Hanne Baeke \u2013 <em>Classification of Solar Flares using Data Analysis and Clustering of Active Regions<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>10:00 \u2013 10:20<\/strong> Hemapriya Raju \u2013 <em>Dynamic time based eruptive flare prediction using machine learning<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>10:20 \u2013 10:40 <\/strong>Mohamed Nedal \u2013 <em>Predicting the Solar Energetic Proton Integral Flux with Deep Learning Models<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\">10:40 \u2013 11:20 Coffee Break<\/mark><\/strong><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>11:20 \u2013 11:40 <\/strong>Suhaila Binti M Buhari \u2013 <em>Equatorial Plasma Bubble Prediction Model Using Satellite Data<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>11:40 \u2013 12:00 <\/strong>Philippe Garnier \u2013 <em>Martian bow shock detection with machine learning<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>12:00 \u2013 12:20 <\/strong>Pearse Murphy \u2013<em> Automatic recognition of solar radio bursts in NenuFAR observations<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>12:20 \u2013 12:40 <\/strong>Akhil Gunessee \u2013 <em>Can a deep learning approach of detecting solar radio bursts perform better than the interquartile range threshold outlier detection method?<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\">12:40 \u2013 14:20 Lunch<\/mark><\/strong><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>14:20 \u2013 14:40 <\/strong>Mario Fernandez \u2013 <em>deARCE solar burst detection system applied to unlabeled e-Callisto data<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>14:40 \u2013 15:00<\/strong> Andrea Diercke \u2013 <em>A Universal Method for Solar Filament Detection from H-alpha Observations using Semi-supervised Deep Learning<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>15:00 \u2013 15:20<\/strong> Aparna Venkataramanasastry \u2013 <em>Applying machine learning to find Filament Chirality<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-medium-font-size\"><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\"><strong>15:20 \u2013 15:40<\/strong> Alin Paraschiv \u2013 <em>Predicting the Geoeffectiveness of CMEs Using Machine Learning<\/em><\/mark><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>15:40 \u2013 16:00 Coffee Break<\/strong><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>16:00 \u2013 18:30 Poster Session<\/strong><br>James Wanliss &#8211; <em>Forecasting Space Weather with Physics-Based Input and Temporal Convolutional Neural Networks<\/em><br>Milo Buitrago-Casas &#8211; <em>A real-time solar flare alert system for early flare physics studies: Exploratory data analysis<\/em><br>Gr\u00e9goire Francisco &#8211; <em>Insight on Flare Forecast with Explainable Deep Learning<\/em><br>Christoph Schirninger &#8211; <em>Deep learning image-burst stacking for post-processing of high-resolution ground-based solar observations<\/em><br>Adeline Paiement &#8211; <em>Removing cloud shadows from ground-based solar imagery<\/em><br>Niels Sayez &#8211; <em>Segmentation, grouping and classification of sunspots from ground-based observations using deep learning methods<\/em><br>Iaroslav Gorbachev &#8211; <em>Application of Deep Learning techniques for Stokes inversions using the Milne-Eddington approximation based on GRIS data<\/em><br>Susan Palacio Salcedo &#8211; <em>Automatic classification of Range-Time-Intensity maps of Equatorial Spread-F<\/em><br>Julio Hernandez Camero &#8211; <em>Building a Coronal Mass Ejection source region catalogue for Machine Learning based space weather forecasting<\/em><br>Maike Bauer &#8211; <em>Automated CME detection and tracking in HI<\/em><br>Valeria Sieyra &#8211; <em>Understanding CME deflections<\/em><br>Saida Milena D\u00edaz Castillo &#8211; <em>Exploring U-net + LSTM networks for classification and segmentation of evolving granular structures<\/em><br>Daniel Collin &#8211; <em>Forecasting solar wind speed from solar EUV images<\/em><br>Aatiya Ali &#8211; <em>Understanding Predictability of Solar Proton Events from GOES statistical features and MHD coronal models.<\/em><br>Kamen Kozarev &#8211; <em>Improving LOFAR Solar Radio Imaging Observations With Machine Learning<\/em><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>19:00 \u2013 21:00 Conference Dinner<\/strong><\/p>\n\n\n\n<p class=\"has-text-align-center has-black-color has-text-color has-medium-font-size\"><strong>Friday April 21, 2023<\/strong><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>Session 2 \u2013 Machine Learning- and Computer Vision-Based Tools<\/strong><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>9:00 \u2013 9:40 (Invited) <\/strong>Robert Jarolim \u2013 <em>Physics informed neural networks and application to solar magnetic field simulations<\/em><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>9:40 \u2013 10:00 <\/strong>Senthamizh Pavai Valliappan <em>\u2013 Performance analysis of AI generated solar farside magnetograms in EUHFORIA<\/em><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>10:00 \u2013 10:20 <\/strong>Jorge Amaya \u2013 <em>Parametrization of solar active regions using Variational Autoencoders<\/em><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>10:20 \u2013 10:40<\/strong> Hannah T. R\u00fcdisser \u2013 <em>Automatic Detection of Interplanetary Coronal Mass Ejections<\/em><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>10:40 \u2013 11:20 Coffee Break<\/strong><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>11:20 \u2013 11:40<\/strong> Felix Nakotey Minta \u2013 <em>Forecasting the Transit Time of Earth-directed Halo CMEs Using Artificial Neural Network: A case study application of GCS forward-modelling technique<\/em><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>11:40 \u2013 12:00<\/strong><em> <\/em>Harshita Gandhi \u2013 <em>Probing the True Nature of CMEs using GCS-based Large Statistics of Multi-viewpoint Observations<\/em><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>12:00 \u2013 12:20<\/strong><em> <\/em>Henrik Eklund \u2013 <em>Artificial neural network based spatio-temporal deconvolver for refinement of solar images<\/em><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>12:20 \u2013 12:40<\/strong><em> <\/em>Slava Bourgeois \u2013 <em>Machine Learning\/Mathematical Morphology coupling for solar features detection<\/em><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>12:40 \u2013 14:20 Lunch<\/strong><br><br><strong><mark style=\"background-color:rgba(0, 0, 0, 0)\" class=\"has-inline-color has-black-color\">Session 4 \u2013 Machine Learning- and Computer Vision-Based Tools<\/mark><\/strong><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>14:20 \u2013 15:00<\/strong> <strong>(Invited)<\/strong> Alexander Engell \u2013 <em>SPRINTS: A machine learning ecosystem for forecasting solar-driven events and scientific event crowd-sourcing<\/em><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>15:00 \u2013 15:20<\/strong> Manolis Georgoulis \u2013 <em>Benchmark Datasets for Solar Weather Forecasting Applications<\/em><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>15:20 \u2013 15:40<\/strong> Oleg Stepanyuk \u2013 <em>Advanced Multi-Instrument Image Processing and Feature Tracking for Remote CME Characterization with Convolutional Neural Network<\/em><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>15:40 \u2013 16:20 Coffee Break<\/strong><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>16:20 \u2013 16:40<\/strong> Mattia Mancini \u2013 <em>Making LOFAR Data Accessible to the Solar and Space Weather Community<\/em><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>16:40 \u2013 17:00 <\/strong>Shane Maloney \u2013 <em>ARCAFF Project Early Results<\/em><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>17:00 \u2013 17:20 <\/strong>Christopher Prior \u2013 <em>ARTop: a program to calculate novel topology-based predictive metrics of active region magnetic field structure.<\/em><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>17:20 \u2013 17:40 <\/strong>Simon Mackovjak \u2013 <em>Feasibility study of data-driven Autonomous Service for Prediction of Ionospheric Scintillations (ASPIS)<\/em><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><strong>17:40 \u2013 18:00 <\/strong>Katya Verner \u2013 <em>The Very First NASA AI\/ML Crowdsourcing Challenge Results Using SOHO\/LASCO Data<\/em><br><br><strong>18:00 \u2013 18:30 Discussion and Farewell<\/strong><\/p>\n\n\n\n<p class=\"has-black-color has-text-color has-medium-font-size\"><\/p>\n","protected":false},"excerpt":{"rendered":"<p>INTERNATIONAL WORKSHOP ON MACHINE LEARNING AND COMPUTER VISION IN HELIOPHYSICS19-21 April, 2023Sofia, Bulgariaand online Wednesday, April 19, 2023 8:30 \u2013 9:00 Registration and Introduction 09:00 \u2013 09:40 (Invited) Michele Piana \u2013 Artificial intelligence for space weather forecasting: data-driven and physics-informed approaches in research and operational settings Session 1 \u2013 Machine Learning \/ Computer Vision Techniques<\/p>\n<p class=\"more-link\"><a href=\"https:\/\/mosaiics.astro.bas.bg\/?page_id=387\" class=\"themebutton\">Read More<\/a><\/p>\n","protected":false},"author":2,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":[],"_links":{"self":[{"href":"https:\/\/mosaiics.astro.bas.bg\/index.php?rest_route=\/wp\/v2\/pages\/387"}],"collection":[{"href":"https:\/\/mosaiics.astro.bas.bg\/index.php?rest_route=\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/mosaiics.astro.bas.bg\/index.php?rest_route=\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/mosaiics.astro.bas.bg\/index.php?rest_route=\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/mosaiics.astro.bas.bg\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=387"}],"version-history":[{"count":15,"href":"https:\/\/mosaiics.astro.bas.bg\/index.php?rest_route=\/wp\/v2\/pages\/387\/revisions"}],"predecessor-version":[{"id":438,"href":"https:\/\/mosaiics.astro.bas.bg\/index.php?rest_route=\/wp\/v2\/pages\/387\/revisions\/438"}],"wp:attachment":[{"href":"https:\/\/mosaiics.astro.bas.bg\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=387"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}