AR
Member Since 2013
Ali Rahmati
Researcher, University of California Berkeley
AGU Research
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Study of Variation Mechanisms of the Martian Diffuse Aurora Based on Monte Carlo Simulations and MAVEN Observations
JOURNAL OF GEOPHYSICAL RESEARCH: SPACE PHYSICS
02 february 2025
Taishin Okiyama, Kanako Seki, Yuki Nakamura, Rober...
Martian diffuse auroras are ultraviolet emissions spread across the nightside of Mars caused by solar energetic particles (SEP), both electrons and...
MAVEN SEP: Turning a Solar Energetic Particle Detector into a Flare Monitor at Mars
SPACE WEATHER AND HUMAN EXPLORATION TO THE MOON, MARS, AND BEYOND II POSTER
spa-solar and heliospheric physics | 12 december 2024
Ali Rahmati, Devon Hartdegen, Davin E. Larson, Chr...
The Solar Energetic Particle (SEP) instrument onboard the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft at Mars is a solid state detector ...
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Temperature Anisotropy and Alpha Abundance Features of Alfvénic Slow Solar Wind Observed by Parker Solar Probe, Helios, and Wind Missions
PARKER SOLAR PROBE’S FURTHEST DESCENT INTO THE SUN’S CORONA V POSTER
spa-solar and heliospheric physics | 11 december 2024
Jia Huang, Davin E. Larson, Tamar Ervin, Oscar Ort...
The slow solar wind is typically characterized as having low Alfvénicity. However, Parker Solar Probe (PSP) has predominantly observed Alfvé...
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Observations of High Energy Proton Events at Mars During Widespread SEP Activity of Solar Cycles 24 to 25
OBSERVATION AND MODELING OF ENERGETIC PARTICLES IN THE HELIOSPHERE I ORAL
spa-solar and heliospheric physics | 11 december 2024
Christina O. Lee, Patrick A. Dunn, Bent Ehresmann,...
Understanding the high-energy particle radiation environment at Mars is important for both scientific and exploration purposes. For example, charged p...
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Kinetic complexities of the near-Sun heliospheric current sheet observed by Parker Solar Probe
PARKER SOLAR PROBE’S FURTHEST DESCENT INTO THE SUN’S CORONA VI POSTER
spa-solar and heliospheric physics | 11 december 2024
Jaye Verniero, Kristoff W. Paulson, Adam Szabo, Ol...
The heliospheric current sheet (HCS), which separates the Suns magnetic field lines of opposite polarity in the solar wind, is a complex structure tha...
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Properties of photoelectrons emitted from antennas: implications on antenna and spacecraft floating potential for Parker Solar Probe
PARKER SOLAR PROBE’S FURTHEST DESCENT INTO THE SUN’S CORONA V POSTER
spa-solar and heliospheric physics | 11 december 2024
Mingzhe Liu, John W. Bonnell, Marc Pulupa, Davin E...
FIELDS instrumentation onboard Parker Solar Probe (PSP) makes use of five voltage probes V1V5 combined to measure three components of the DC and fluct...
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Space Weather Follow On: Developing Imagery and Other Data Products Following the GOES-19 Launch
COMBINING CORONAL AND HELIOSPHERIC IMAGING, IN SITU OBSERVATIONS, AND MODELING TO UNDERSTAND THE YOUNG SOLAR WIND II POSTER
spa-solar and heliospheric physics | 10 december 2024
Dimitrios Vassiliadis, John Carey, Matthew Devaney...
The Space Weather Follow-On (SWFO) program will provide operational solar-coronal images and in situ solar wind measurements to the science community ...
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MAVEN observations during the Perseverance detection of visible auroral emission
SPACE ENVIRONMENTS OF UNMAGNETIZED OR WEAKLY MAGNETIZED SOLAR SYSTEM BODIES AND THE EFFECTS OF SPACE WEATHER ON THESE SYSTEMS I POSTER
planetary sciences | 10 december 2024
Nicholas M. Schneider, Sonal Jain, Julianna Cessna...
Space weather events can bombard Mars with solar energetic particles (SEP's) which engulf the planet in diffuse auroral emissions. Some diffuse aurora...
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