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Christina Lee
Space Sciences LaboratoryMeeting roles in:
Exploring the Connections Between the Sun, Outer Heliosphere, and Local Interstellar Medium, Including First-Light Results from NASA’s IMAP Mission I Oral
What can 10 years of MAVEN data reveal about electron acceleration in the Martian magnetotail?
IMAP’s Role in Understanding Particle Injection and Energization Throughout the Heliosphere
Exploring the Connections Between the Sun, Outer Heliosphere, and Local Interstellar Medium, Including First-Light Results from NASA’s IMAP Mission II Oral
Radial Dependency of ICME-associated Particle Acceleration Processes: Statistical Multipoint Observations from 2016-2023
Understanding Space Weather for Human and Robotic Exploration to the Moon, Mars, and Beyond I Oral
Understanding Space Weather for Human and Robotic Exploration to the Moon, Mars, and Beyond II Oral
The Solar Energetic Particle Detector on MAVEN: Bonus Science at Mars
Delivering Near Real-Time Space Weather Observations: The I-ALiRT Cloud Architecture and International Ground Station Integration for IMAP
Exploring the Connections Between the Sun, Outer Heliosphere, and Local Interstellar Medium, Including First-Light Results from NASA’s IMAP Mission III Poster
Solar Polar Field Reversal Influences on the Solar Wind at 1 AU
Space Weather Science to Enhance Forecasting with the NASA IMAP Active Link for Real-Time (I-ALiRT) Data System
Understanding Space Weather for Human and Robotic Exploration to the Moon, Mars, and Beyond III Poster
Measuring high energy (10 MeV - 10 GeV) particles at Mars with the MAVEN Solar Energetic Particle detector, with a focus on Galactic Cosmic Ray modulation throughout the solar cycle (2015-2024).
Modeling the 2017 September 10 Solar Energetic Particle Event as Observed on Mars and at 1 au
The Mars Space Weather Collaboration’s Development of Decision-Making Tools to Support Human Exploration
Analysis of Extreme Space Weather Events at Mars with Low Latency Data in Support of Future R2O2R Activities
Recent Multi-Point Measurements of Coronal Mass Ejections: Maximum of Solar Cycle 25
Building a solar energetic particle event catalog for Mars
The Intense Multi-Spacecraft SEP event on 2024 May 20 as a Test of the Main Mechanisms Distributing SEPs in the Inner Heliosphere
Multipoint Observations of Solar Energetic Particle Transport During December 05-10, 2024 Events
Characterizing Bidirectional Solar Energetic Electron Events Near 1 AU
Modeling and Data Analysis of the Solar Energetic Particles during the May 2024 Geostorm Event
Predicting the effects of coronal mass ejections on the lunar exosphere with in-situ observations
A Decade of MAVEN Proton Auroral Observations at Mars: Evaluating the Influence of Seasonal and Solar Cycle Variability
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