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2025 CAP Congress / Congrès de l'ACP 2025

8–13 Jun 2025
America/Regina timezone
Welcome to the 2025 CAP Congress Program website! / Bienvenue au siteweb du programme du Congrès de l'ACP 2025!

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Session

(DASP) M2-2 General Topics: Planetary Physics and Astronomy | Thèmes généraux: Physique et astronomie planétaires (DPAE)

M2-2
9 Jun 2025, 14:15

Conveners

(DASP) M2-2 General Topics: Planetary Physics and Astronomy | Thèmes généraux: Physique et astronomie planétaires (DPAE)

  • David Themens (University of New Brunswick)
  • Giacomo Radaelli

Presentation materials

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  1. 102. A Virtual Solar Wind Monitor at Mars to Enable Statistical and Comparative Magnetospheric Studies
    Dr Abigail Azari (University of Alberta, Alberta Machine Intelligence Institute)
    09/06/2025, 14:15
    Atmospheric and Space Physics / Physique atmosphérique et spatiale (DASP/DPAE)
    Invited Speaker / Conférencier(ère) invité(e)

    Unlike Earth, Mars does not possess an upstream solar wind monitor. This lack of continuous solar wind observations has fundamentally limited scientific studies that investigate solar wind impacts on the Mars space environment. This lack of a dedicated upstream monitor has also limited emerging operational tasks for predicting space weather throughout our solar system. Previous estimates of...

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  2. 107. Simulation-Based Evaluation of Crosslink Radio Occultation for Lunar Ionosphere Observations
    Giacomo Radaelli
    09/06/2025, 14:45
    Atmospheric and Space Physics / Physique atmosphérique et spatiale (DASP/DPAE)
    Oral Competition (Graduate Student) / Compétition orale (Étudiant(e) du 2e ou 3e cycle)

    The lunar ionosphere is a ∼100 km thick layer of plasma surrounding the Moon. Despite knowledge of its existence for decades, the structure and dynamics of the lunar plasma remain a mystery due to lack of consistent observational capacity. An enhanced observational picture of the lunar ionosphere and improved understanding of its formation/loss mechanisms is critical for understanding the...

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  3. 321. Learning to See: Applying Inverse Recurrent Inference Machines to See through Refractive Scattering
    Mr Arvin Kouroshnia (University of Waterloo)
    09/06/2025, 15:00
    Atmospheric and Space Physics / Physique atmosphérique et spatiale (DASP/DPAE)
    Oral Competition (Undergraduate Student) / Compétition orale (Étudiant(e) du 1er cycle)

    The Event Horizon Telescope (EHT) has captured images resolving the horizon of Sagittarius A (Sgr A∗), unveiling a new window into understanding strong gravity and cosmology. Scattering from the turbulent plasma of the interstellar medium distort the appearance of Sgr A, limiting the practical angular resolution of Sgr A*. We utilized a recurrent neural network trained on samples ignorant to...

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  4. 320. Moving to Learn to See
    Kenny Nguyen (University of Waterloo)
    09/06/2025, 15:15
    Atmospheric and Space Physics / Physique atmosphérique et spatiale (DASP/DPAE)
    Oral Competition (Undergraduate Student) / Compétition orale (Étudiant(e) du 1er cycle)

    The Event Horizon Telescope (EHT) is a very long baseline interferometry (VLBI) array that has the capacity to resolve images of supermassive black holes such as Sagittarius A and M87. Turbulence in the interstellar medium distorts images of objects near the galactic center, e.g., Sagittarius A*. This reduces the angular resolution that could be resolved. The scattering screen changes on...

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