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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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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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Future Exploration of the Outer Heliosphere and the Very Local Interstellar Medium
THE PAST, PRESENT, AND FUTURE OF HELIOPHYSICS THROUGH IN SITU OBSERVATIONS OF THE OUTER HELIOSPHERE AND THE INTERSTELLAR MEDIUM I POSTER
spa-solar and heliospheric physics | 14 december 2023
Pontus C. Brandt, Ralph L. McNutt, Merav Opher, Li...
Our solar system has evolved through accretion of dust and gas as the Sun and its protective magnetic bubble the heliosphere - have plowed through in...
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Heating of Energetic Pickup Ions in the Supersonic Solar Wind Region by Shock Waves: Observations and Modeling
THE PAST, PRESENT, AND FUTURE OF HELIOPHYSICS THROUGH IN SITU OBSERVATIONS OF THE OUTER HELIOSPHERE AND THE INTERSTELLAR MEDIUM I POSTER
spa-solar and heliospheric physics | 14 december 2023
Parisa Mostafavi, Gary P. Zank, Matthew E. Hill, M...
The outer heliosphere is a highly dynamic region that is profoundly influenced by the presence of nonthermal energetic pickup ions (PUIs). These PUIs,...
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Looking for Signatures of Magnetic Reconnection in the Heliosheath and at the Heliopause with Voyager Data
THE PAST, PRESENT, AND FUTURE OF HELIOPHYSICS THROUGH IN SITU OBSERVATIONS OF THE OUTER HELIOSPHERE AND THE INTERSTELLAR MEDIUM I POSTER
spa-solar and heliospheric physics | 14 december 2023
Benoit Lavraud, Drew L. Turner, Baptiste Bernard, ...
Magnetic reconnection has been proposed as an important process in the heliosheath and at the heliopause. Yet, apart from some suprathermal particle s...
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investigating the collisional shock structures in the VLISM using Braginskii type fluid models
THE PAST, PRESENT, AND FUTURE OF HELIOPHYSICS THROUGH IN SITU OBSERVATIONS OF THE OUTER HELIOSPHERE AND THE INTERSTELLAR MEDIUM I POSTER
spa-solar and heliospheric physics | 14 december 2023
Keyvan Ghanbari, Gary P. Zank, Parisa Mostafavi
The Voyager spacecraft have detected shocks in the very local interstellar medium (VLISM), which have different properties than shocks in the inner he...
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Parker Solar Probe Observations and Hybrid Models of High Mach Number Oblique Shock
PROCESSES ACROSS SHOCK WAVES IN COLLISIONLESS PLASMAS II ORAL
spa-solar and heliospheric physics | 12 december 2023
Leon Ofman, Scott A. Boardsen, Jonathan Ng, Lynn B...
On September 5, 2022, the Parker Solar Probe (PSP) detected a high Mach number oblique shock for the first time in the inner heliosphere close to the ...
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Observing the Earliest Stage of Non-thermal Charged Particle Acceleration in Interplanetary Space: the September 5, 2022 “Labor Day” Event at Parker Solar Probe
PARKER SOLAR PROBE’S CONTINUED EXPLORATION OF THE SUN’S LOWER CORONA I ORAL
spa-solar and heliospheric physics | 11 december 2023
Matthew E. Hill, Joe Giacalone, John Mitchell, Chr...
During solar flare episodes and eruptions of solar material, known as coronal mass ejections (CMEs), free electrons and ions are accelerated to high e...
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