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Heliophysics Integrated Modeling: From Sun-Earth to Star-Exoplanet
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Heliophysics Division Next Generation Solar Physics Mission (NGSPM)
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On Clustering of Machine Learning Attempts in Heliophysics: Examples and General Picture
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Heliophysics: Prediction of Radiation Doses Received During Airplane Flights
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Solar Cruiser: Enabling New Vistas for Heliophysics
A poster presentation for the fall 2020 Space Weather Operations and Research Infrastructure Workshop describing the proposed NASA Solar Cruiser mission.
Designing Low-Thrust Enabled Trajectories for a Heliophysics Smallsat Mission to Sun-Earth L5
A small satellite deployed to Sun-Earth L5 could serve as a low-cost platform to observe solar phenomena such as coronal mass ejections. However, the small satellite platform introduces significant challenges in the trajectory design process via limited thrusting capabilities, power and operational constraints, and fixed deployment conditions. To address these challenges, a strategy employing dynamical systems theory is used to design a low-thrust-enabled trajectory for a small satellite to reach the Sun-Earth L5 region. This procedure is demonstrated for a small satellite that launches as a secondary payload with a larger spacecraft destined for a Sun-Earth L2 halo orbit.
SmallSat Forum Presentation: NASA Heliophysics and Astrophysics SmallSat/CubeSats
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NASA Heliophysics GDC/DYNAMIC Overview
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LIKED and DIARieS: Developing the Next Generation Heliophysics Resources
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LIKED and DIARieS: Developing the Next Generation Heliophysics Resources
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Redefining Flux Ropes in Heliophysics
Magnetic flux ropes manifest as twisted bundles of magnetic field lines. They carry significant amounts of solar mass in the heliosphere. This paper underlines the need to advance on the fundamental understanding of heliospheric flux ropes and provides the motivation to significantly improve the status quo of flux rope research through the novel and requisite approaches. It briefly discusses the current understanding of flux rope formation and evolution, and summarizes the strategies that have been undertaken to understand the dynamics of heliospheric structures. The challenges and recommendations put forward to address them are expected to broaden the in-depth knowledge of our nearest star, its dynamics, and its role in its region of influence, the heliosphere.
ISTPNext and the Heliophysics Great Observatories - Motivation, Background, and Current Status
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Introduction to NASA, the Heliophysics Big Year, and Solar Research
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GEOS-MLT: A High-Altitude Atmospheric Model to Bridge Earth System Modeling and Heliophysics Data
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The Lunar Environment Heliophysics X-Ray Imager (LEXI) Mission
The Lunar Environment heliospheric X-ray Imager (LEXI) is a wide field-of-view soft Xray telescope developed to study solar wind-magnetosphere coupling. LEXI is part of the Blue Ghost 1 mission comprised of 10 payloads to be deployed on the lunar surface. LEXI monitors the dayside magnetopause position and shape as a function of time by observing soft X-rays (0.1–2 keV) emitted from solar wind charge-exchange between exospheric neutrals and high charge-state solar wind plasma in the dayside magnetosheath. Measurements of the shape and position of the magnetopause are used to test temporal models of mesoand macro-scale magnetic reconnection. To image the boundary, LEXI employs lobster-eye optics to focus X-rays to a microchannel plate detector with a 9.1◦ × 9.1◦ field of view.
The Lunar Environment Heliophysics X-ray Imager (LEXI) Mission
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ML‐Helio: An Emerging Community at the Intersection Between Heliophysics and Machine Learning
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