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Member Since 2015
Parisa Mostafavi
Senior Professional Staff I , Johns Hopkins University Applied Physics Laboratory
AGU Research
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Study of Ion Velocity Distributions and Kinetic Wave Activity Observed in the Acceleration Region of the Solar Wind by the Parker Solar Probe
AGU 2024
spa-solar and heliospheric physics | 13 december 2024
Leon Ofman, Scott A. Boardsen, Lan Jian, Yogesh .,...
The Parker Solar Probe (PSP), launched in August, 2018 is expected to reach the closest approach in December 2024 to about 0.04 AU (about 9Rs). The PS...
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Investigation of the ion-cyclotron waves and proton beams during PSP encounter 17
AGU 2024
spa-solar and heliospheric physics | 13 december 2024
Yogesh ., Leon Ofman, Scott A. Boardsen, Viachesla...
Recent in situ observations from the Parker Solar Probe (PSP) mission in the inner heliosphere near perihelia reveal evidence of ion beams, temperatur...
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Understanding Extreme Solar Energetic Particle Pressures and Shock Structures within 1 AU
AGU 2024
spa-solar and heliospheric physics | 12 december 2024
Parisa Mostafavi, David Lario, Athanasios Kouloumv...
Large solar energetic particle (SEP) events are typically associated with strong coronal and interplanetary shocks driven by coronal mass ejections (C...
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A “Valley” in Heliospheric Energetic Particle Intensities and Implications for a New Horizons Encounter with the Solar Wind Termination Shock
AGU 2024
spa-solar and heliospheric physics | 11 december 2024
Romina Nikoukar, Matthew E. Hill, Robert B. Decker...
Launched in 2006, the New Horizons (NH) spacecraft is currently at 59 au from the Sun and expected to observe the solar wind termination shock (TS) as...
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Preparing for the Termination Shock Encounter with New Horizons
AGU 2024
spa-solar and heliospheric physics | 11 december 2024
Pontus C. Brandt, Matthew E. Hill, Heather A. Elli...
Across the Termination Shock (TS) the solar wind was expected to transition from supersonic to subsonic and heat by two orders of magnitude. Voyager 2...
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Coronal Jet, Hard X-ray, Type III, and Electron Beam-Associated 3He-rich Event April 1, 2024 at 25 Solar Radii
AGU 2024
spa-solar and heliospheric physics | 09 december 2024
Donald G. Mitchell, David Lario, Nour E. Raouafi, ...
Parker Solar Probe (PSP) observations of a small dispersive event on April 1, 2024 reveal highly enriched 3He abundance in the low suprathermal energy...
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Globally distributed flux of ENAs at energies below 2 keV
CONNECTING FUNDAMENTAL PLASMA PROCESSES AT 1 AU TO IMAGING NEUTRAL ATOMS FROM THE OUTER HELIOSPHERE: IBEX AND IMAP PERSPECTIVES I ELIGHTNING
spa-solar and heliospheric physics | 15 december 2023
Justyna M. Sokol, Stephen A. Fuselier, André Galli...
IBEX-Lo collects neutral atoms of energies below 2 keV. At energies less than 0.1 keV, a signal from the interstellar neutral gas and its secondary po...
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Bridging the Energy Gap: Solar Wind Data from PEPSSI and SWAP on New Horizons
THE PAST, PRESENT, AND FUTURE OF HELIOPHYSICS THROUGH IN SITU OBSERVATIONS OF THE OUTER HELIOSPHERE AND THE INTERSTELLAR MEDIUM II ORAL
spa-solar and heliospheric physics | 15 december 2023
Ralph L. McNutt, David J. McComas, Matthew E. Hill...
The New Horizons spacecraft, launched in 2006, continues to return unprecedented charged particle data from the outer heliosphere. The Pluto Energetic...
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