Member Since 1984
Lynn M. Kistler
Professor, University of New Hampshire Main Campus
AGU Research
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Energy Dispersed Oxygen Beams in the Magnetotail During Storms
AGU 2024
spa-magnetospheric physics | 13 december 2024
Lynn M. Kistler, Milla Kalliokoski, Yoshizumi Miyo...
Because of its off-equatorial orbit, the Arase satellite is well-placed to observe the plasma sheet boundary layer (PSBL) at apogee on the nightside. ...
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Statistical study of the warm plasma cloak
AGU 2024
spa-magnetospheric physics | 12 december 2024
Jing Liao, Lynn M. Kistler, Christopher Mouikis, T...
The warm plasma cloak (a few eV- 1 keV) is a population that drapes around the outer edge of the plasmasphere and spreads out to higher L regions from...
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Differences in Ionospheric O+ and H+ Outflow during Storms with and without Sawtooth Oscillations
AGU 2024
spa-magnetospheric physics | 12 december 2024
Niloufar Nowrouzi, Lynn M. Kistler, Kai Zhao, Eric...
Previous simulations have suggested that O+ outflow plays a role in driving the sawtooth oscillations. This study investigates the role of O+ by ident...
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The Storm‐Time Ring Current Response to CIRs and CMEs driven magnetic storms: Arase Observations
AGU 2024
spa-magnetospheric physics | 12 december 2024
Sandeep Kumar, Yoshizumi Miyoshi, Vania K. Jordano...
Geomagnetic storms are caused by corotating interaction regions (CIRs) associated with high-speed solar wind streamers (HSSs), and coronal mass ejecti...
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Analysis of Pickup Ions Observed by SWA-HIS during the Solar Orbiter Encounter with Comet Leonard
AGU 2024
planetary sciences | 11 december 2024
Kevin Delano, Timothy J. Stubbs, Ryan M. Dewey, An...
Comet Leonard was the brightest comet of 2021, and shortly before it disintegrated the Solar Orbiter spacecraft passed through its tail, providing a u...
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Variations in the He+ Pickup Ion Distributions inside 1 AU
AGU 2024
spa-solar and heliospheric physics | 11 december 2024
Antoinette B. Galvin, Lynn M. Kistler, Lorna Ellis...
Pickup ions (PUI) are generated when a neutral in the heliosphere is ionized and then is picked up by the local magnetic field . The single charge sta...
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Suprathermal Ion Observations from Solar Orbiter: Status of Intercalibration between the Heavy Ion Sensor and Suprathermal Ion Spectrograph
AGU 2024
spa-solar and heliospheric physics | 11 december 2024
Benjamin L. Alterman, Robert C. Allen, Ryan M. Dew...
Suprathermal ions occupy the energy range of a few keV to MeV between the thermal solar wind and energetic particles that suffuse the interplanetary s...
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The Ion Mass Spectrometer On-board the Plasma Observatory Mother Spacecraft
AGU 2024
spa-magnetospheric physics | 10 december 2024
Maria Federica Marcucci, Lynn M. Kistler, Benoit L...
Plasma Observatory (PO) is the first multiscale mission tailored to study plasma energization and energy transport in the Earth's Magnetospheric Syste...
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