J. T. Steinberg
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View article: Dual-band Ion-scale Waves in the Solar Wind: Statistical Properties and Comparison with Single-band Ion-scale Waves
Dual-band Ion-scale Waves in the Solar Wind: Statistical Properties and Comparison with Single-band Ion-scale Waves Open
We present a comprehensive statistical analysis of ion-scale waves including dual-band ion-scale waves (DBIWs) observed by the Parker Solar Probe in the solar wind. DBIWs are characterized by the simultaneous occurrence of distinct left- a…
View article: Simultaneous Observation of Ion-scale Wave Packets with Opposite Polarizations and Their Implications on the Generation Region in the Inner Heliosphere
Simultaneous Observation of Ion-scale Wave Packets with Opposite Polarizations and Their Implications on the Generation Region in the Inner Heliosphere Open
This paper reports a dispersion analysis of two wave packets simultaneously observed near the local proton gyrofrequency by the Parker Solar Probe. The observed wave event exhibits clear two-banded wave packets both propagating along the m…
View article: Total Ionizing Dose Observations On-Board STPSat-6 in GEO
Total Ionizing Dose Observations On-Board STPSat-6 in GEO Open
The Falcon Solid-state Energetic Electron Detector (SEED) is an energetic charged particle sensor that has been developed at the United States Air Force Academy to monitor electron flux across the energy range of 14 to 145 keV in geosynchr…
View article: Imprint of the Coronal Temperature on Suprathermal Electrons at ACE
Imprint of the Coronal Temperature on Suprathermal Electrons at ACE Open
View article: Presentation - Development of the Experiment for Space Radiation Analysis (ESRA) CubeSat Mission to GTO
Presentation - Development of the Experiment for Space Radiation Analysis (ESRA) CubeSat Mission to GTO Open
View article: The Genesis Mission: Solar Wind Conditions, and Implications for the FIP Fractionation of the Solar Wind.
The Genesis Mission: Solar Wind Conditions, and Implications for the FIP Fractionation of the Solar Wind. Open
The NASA Genesis mission collected solar wind on ultrapure materials between November 30, 2001 and April 1, 2004. The samples were returned to Earth September 8, 2004. Despite the hard landing that resulted from a failure of the avionics t…
View article: HelioSwarm: A Multipoint, Multiscale Mission to Characterize Turbulence
HelioSwarm: A Multipoint, Multiscale Mission to Characterize Turbulence Open
View article: Heavy Ions: A Critical Measurement for Understanding the Solar Wind/Ionosphere/Magnetosphere
Heavy Ions: A Critical Measurement for Understanding the Solar Wind/Ionosphere/Magnetosphere Open
Whitepaper #106 in the Decadal Survey for Solar and Space Physics (Heliophysics) 2024-2033. Main topics: basic research. Additional topics: system science; user-need-driven basic space weather research.
View article: HelioSwarm: A Multipoint, Multiscale Mission to Characterize Turbulence
HelioSwarm: A Multipoint, Multiscale Mission to Characterize Turbulence Open
HelioSwarm (HS) is a NASA Medium-Class Explorer mission of the Heliophysics Division designed to explore the dynamic three-dimensional mechanisms controlling the physics of plasma turbulence, a ubiquitous process occurring in the heliosphe…
View article: Compressible Turbulence in the Near-Sun Solar Wind: Parker Solar Probe’s First Eight Perihelia
Compressible Turbulence in the Near-Sun Solar Wind: Parker Solar Probe’s First Eight Perihelia Open
Many questions remain about the compressibility of solar wind turbulence with respect to its origins and properties. Low plasma beta (ratio of thermal to magnetic pressure) environments allow for the easier generation of compressible turbu…
View article: Compressible Turbulence in the Near-Sun Solar Wind: Parker Solar Probe's First Eight Perihelia
Compressible Turbulence in the Near-Sun Solar Wind: Parker Solar Probe's First Eight Perihelia Open
Many questions remain about the compressibility of solar wind turbulence with respect to its origins and properties. Low plasma beta (ratio of thermal to magnetic pressure) environments allow for the easier generation of compressible turbu…
View article: Nature and Scalings of Density Fluctuations of Compressible Magnetohydrodynamic Turbulence with Applications to the Solar Wind
Nature and Scalings of Density Fluctuations of Compressible Magnetohydrodynamic Turbulence with Applications to the Solar Wind Open
The solar wind is a magnetized and turbulent plasma. Its turbulence is often dominated by Alfvénic fluctuations and often deemed as nearly incompressible far away from the Sun, as shown by in situ measurements near 1 au. However, for solar…
View article: Temperature of Suprathermal Electron Strahl at ACE as an Indicator of Solar Coronal Origin Temperature [Slides]
Temperature of Suprathermal Electron Strahl at ACE as an Indicator of Solar Coronal Origin Temperature [Slides] Open
Determine the effectiveness of using electron strahl temperature to infer coronal source temperature. Suprathermal electron strahl temperature derived from measurements at 1 AU does retain information regarding the coronal source temperatu…
View article: Nature and Scalings of Density Fluctuations of Compressible MHD Turbulence with Applications to the Solar Wind
Nature and Scalings of Density Fluctuations of Compressible MHD Turbulence with Applications to the Solar Wind Open
The solar wind is a magnetized and turbulent plasma. Its turbulence is often dominated by Alfvénic fluctuations and often deemed as nearly incompressible far away from the Sun, as shown by in-situ measurements near 1AU. However, for solar …
View article: Alfvénic velocity spikes and rotational flows in the near-Sun solar wind
Alfvénic velocity spikes and rotational flows in the near-Sun solar wind Open
View article: Low‐Resource Technique for Measurement of H<sup>+</sup> and O<sup>+</sup> in the Terrestrial Magnetosphere
Low‐Resource Technique for Measurement of H<sup>+</sup> and O<sup>+</sup> in the Terrestrial Magnetosphere Open
Measurement of O + in the Earth's magnetosphere is important for monitoring and understanding the initiation and evolution of geomagnetic activity. During active times, O + can be the most abundant ion in the magnetosphere. Furthermore, be…
View article: Data for paper "Low Resource Technique for Measurement of H+ and O+ in the Terrestrial Magnetosphere"
Data for paper "Low Resource Technique for Measurement of H+ and O+ in the Terrestrial Magnetosphere" Open
Data set for paper "Low Resource Technique for Measurement of H+ and O+ in the Terrestrial Magnetosphere" to be published in Journal of Geophysical Research: Space Physics (Technical Methods). Data set is a single Microsoft Excel file cont…
View article: Data for paper "Low Resource Technique for Measurement of H+ and O+ in the Terrestrial Magnetosphere"
Data for paper "Low Resource Technique for Measurement of H+ and O+ in the Terrestrial Magnetosphere" Open
Data set for paper "Low Resource Technique for Measurement of H+ and O+ in the Terrestrial Magnetosphere" to be published in Journal of Geophysical Research: Space Physics (Technical Methods). Data set is a single Microsoft Excel file cont…
View article: [Plasma 2020 Decadal] Multipoint Measurements of the Solar Wind: A\n Proposed Advance for Studying Magnetized Turbulence
[Plasma 2020 Decadal] Multipoint Measurements of the Solar Wind: A\n Proposed Advance for Studying Magnetized Turbulence Open
A multi-institutional, multi-national science team will soon submit a NASA\nproposal to build a constellation of spacecraft to fly into the near-Earth\nsolar wind in a swarm spanning a multitude of scales in order to obtain\ncritically nee…
View article: Multipoint measurements of the solar wind: A proposed advance for studying magnetized turbulence
Multipoint measurements of the solar wind: A proposed advance for studying magnetized turbulence Open
A multi-institutional, multi-national science team will soon submit a NASA proposal to build a constellation of spacecraft to fly into the near-Earth solar wind in a swarm spanning a multitude of scales in order to obtain critically needed…
View article: Solar Wind Electrons Alphas and Protons (SWEAP) Investigation: Design of the Solar Wind and Coronal Plasma Instrument Suite for Solar Probe Plus
Solar Wind Electrons Alphas and Protons (SWEAP) Investigation: Design of the Solar Wind and Coronal Plasma Instrument Suite for Solar Probe Plus Open
View article: Solar Wind Electrons Alphas and Protons (SWEAP) Investigation: Design of the Solar Wind and Coronal Plasma Instrument Suite for Solar Probe Plus
Solar Wind Electrons Alphas and Protons (SWEAP) Investigation: Design of the Solar Wind and Coronal Plasma Instrument Suite for Solar Probe Plus Open