Solar corona during the 2 July 2019 total solar eclipse, observed from La Silla, Chile

Universidad de Santiago de Chile — Department of Physics

Heliophysics and Space Weather

We study the Earth's magnetosphere, radiation belts, and solar wind coupling using satellite data and ground-based observations. Our group develops machine learning tools for space weather prediction and contributes to developing a pilot space weather monitoring platform for Chile.

Credit: ESA/CESAR

Research

Research lines

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Schematic illustration: Earth, dipole field lines, and the inner and outer radiation belts

Space physics

Radiation belt dynamics

Energization, transport, and decay of relativistic electrons in the Van Allen belts. Enhancement and dropout events during geomagnetic storms. Formation and evolution of ultrarelativistic remnant belts. Adiabatic and non-adiabatic processes in the outer radiation belt.

Schematic illustration: an oscillating magnetic field line and a ULF wave train

Space physics

ULF waves and magnetospheric turbulence

Role of electromagnetic ULF waves in trapped particle dynamics. Magnetospheric turbulence and total pressure balance during storms and substorms. Eddy diffusion in the plasma sheet. Wave-particle interactions.

Schematic illustration: neural network and a time series with a forecast and its uncertainty band

Data science

Space weather prediction with ML

Prediction of ground magnetic perturbations and geomagnetically induced currents (GIC). Probabilistic forecasting using deep learning (LSTM, CNN). ML model explainability for operational space weather. Plasmapause location with machine learning.

Schematic illustration: solar wind deflected by Earth's bow shock and magnetopause

Space physics

Solar wind — magnetosphere coupling

Solar wind dynamic pressure effects on magnetospheric turbulence. Foreshock transients and magnetospheric perturbations. Expanding plasma systems: solar and stellar winds. Adiabatic invariants and non-adiabatic mechanisms in solar wind expansion.

Projects

Active projects

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Schematic illustration of a neural-network forecast

FONDEF IDEA I+D 2025 · FONDEF/ANID

Chilean Space Weather Platform

Pilot platform for real-time space weather monitoring and early warnings in Chile, with deep-learning forecasting models. Led by Universidad Adventista de Chile, with USACH as partner institution.

  • Real-time monitoring
  • DL forecasting
  • GIC prediction

Director: M. Bravo (Universidad Adventista de Chile) · Principal investigator (USACH): Dr. Victor Pinto · 2025-2027

Schematic illustration of a ULF wave in the magnetosphere

FONDECYT Initiation 2025 · ANID

ULF waves and trapped particles

The role of electromagnetic ULF waves in the dynamics of charged particles trapped in Earth's radiation belts.

  • Van Allen Probes
  • THEMIS
  • GOES

PI: Dr. Victor Pinto · 2025-2028

Schematic illustration of the solar wind interacting with the magnetosphere

FONDECYT Regular 2025 · ANID

Turbulence and pressure balance in the magnetosphere

Turbulence and total pressure balance in the interconnected dynamic magnetosphere during storms and substorms.

  • Magnetospheric turbulence
  • Pressure balance
  • Storm dynamics

PI: Prof. Marina Stepanova · Co-I: Dr. Victor Pinto · 2025-2029

Team

Our team

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Dr. Victor A. Pinto Abarzúa

Assistant Professor
Department of Physics, USACH · Associate Chair for Teaching

Prof. Marina Stepanova

Professor
Department of Physics, USACH

Dr. Bea Zenteno Quinteros

Postdoctoral researcher (FONDECYT Postdoctoral grant), USACH

Space plasma physics: waves, instabilities, and relativistic electron losses

Dr. Matilde Coello

Postdoctoral researcher (DICYT Postdoctoral grant), USACH

Expansion, instabilities, and thermodynamics of the young solar wind

Dafhne Muñoz Reyes

Astrophysics Engineering, USACH

ML model for plasmapause location (Van Allen Probes)

Camila Peña Cifuentes

Physics Engineering, USACH

Deep Learning prediction of relativistic electron flux

Paula Reyes

M.Sc. in Physics, Universidad de Chile (co-advised)

Geomagnetic storms and their relation with solar cycle phases

Publications

Recent publications

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  1. 2026

    Comparative performance analysis of five magnetometers for geomagnetic monitoring

    Caro, G., Carrasco, E., Diaz Peña, J., Urra, B., Rojo, E., Castro, L., Bravo, M., Pinto, V., Stepanova, M., Godoy, A., Ovalle, E., Denardini, C.M., Su Chen, S.

    Sensors, 26, 4700 · DOI

  2. 2026

    The effect of expansion and instabilities in the thermodynamic regulation of the young solar wind plasma

    Coello-Guzmán, M., Pinto, V.A., Navarro, R.E., Moya, P.S.

    Astronomy & Astrophysics · in press

  3. 2026

    The role of auroral phenomena in the dynamics of the outer radiation belt during the 1 June 2013 geomagnetic storm

    Inostroza, A.M., Díaz Peña, J., Coello-Guzmán, M., Stepanova, M., Pinto, V.A., Navarro, R.E., Espinoza, J.M., Kolomiytseva, E.A., Antonova, E.E.

    JGR: Space Physics · DOI

  4. 2026

    On the effects of the solar wind structure in the global distribution of dBH/dt spikes during geomagnetic storms

    Marchezi, J.P., Keesee, A., Coughlan, M., Mukundan, R., Pinto, V., Da Silva, L.A., Alves, L.R., Connor, H., Hampton, D.

    JGR: Space Physics · DOI

  5. 2026

    Role of the solar wind dynamic pressure in the development of magnetospheric turbulence

    Stepanova, M., Pinto, V.A., Espinoza, C.M., Ovchinnikov, I.L., Antonova, E.E.

    Physica Scripta, 101, 095603 · DOI

Infrastructure

Infrastructure and data

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High-performance computing (HPC) cluster

Computing platform at the Department of Physics, funded by FONDEQUIP (2023) and directed by Dr. Victor Pinto. Used to train machine learning models, process large satellite datasets, and run numerical simulations.

Pilot space weather platform (FONDEF IDEA)

Project led by Universidad Adventista de Chile, with USACH as partner institution (2025-2027). It develops a pilot system for real-time space weather monitoring and early warnings in Chile, with deep-learning forecasting models.

Magnetometry

Performance evaluation of magnetometers for geomagnetic monitoring, in collaboration with Universidad Adventista de Chile, and analysis of ground magnetometer network data to study geomagnetic disturbances and geomagnetically induced currents (GIC).

Contact

Open positions

We are looking for undergraduate and master's students to work on relativistic electron dynamics, geomagnetic storm prediction with deep learning, geomagnetically induced currents (GIC), satellite data processing, and magnetospheric turbulence. If you study physics, astrophysics, or a related field, write to us.

We welcome collaborations, thesis projects, and press inquiries about heliophysics and space weather.

Dr. Victor A. Pinto

Group co-lead

Department of Physics, Universidad de Santiago de Chile