Add to ORKGMeasuring energy transfer at colliding streams in solar wind based on data from Explorer 34 and Vela 4B satellite
The radial gradient of long-lived, corotating energetic particle streams was measured using observat...
A multi-institutional, multi-national science team will soon submit a NASA proposal to build a const...
We present a brief review of observations and theory regarding the nature and radial evolution of MH...
Plasma experiments on Explorer 34 satellite to study fluid properties of solar win
Spacecraft observations from the interplanetary medium of our solar system reveal the presence of a ...
The solar wind is a multicomponent plasma consisting of protons, electrons, and smaller amounts of h...
Recent results in interplanetary physics are examined. These include observations of shock waves and...
Using data from the Plasma and Suprathermal Ion Composition (PLASTIC) instruments onboard the Solar ...
Interplanetary acceleration processes are shown as the most plausible explanation for the observed c...
Direct evidence of an inertial-range turbulent energy cascade has been provided by spacecraft observ...
This paper analyzes solar wind power spectra of bulk and thermal speed fluctuations that are compute...
The solar wind is the Sun's exosphere. As the solar atmosphere expands into interplanetary space, it...
A discussion of the solar wind and its interaction with bodies of the solar system is presented. An ...
The solar wind evolves as it moves outward due to interactions with both itself and with the circum-...
The local heating of the solar-wind gas during its expansion represents one of the most intriguing p...
The radial gradient of long-lived, corotating energetic particle streams was measured using observat...
A multi-institutional, multi-national science team will soon submit a NASA proposal to build a const...
We present a brief review of observations and theory regarding the nature and radial evolution of MH...
Plasma experiments on Explorer 34 satellite to study fluid properties of solar win
Spacecraft observations from the interplanetary medium of our solar system reveal the presence of a ...
The solar wind is a multicomponent plasma consisting of protons, electrons, and smaller amounts of h...
Recent results in interplanetary physics are examined. These include observations of shock waves and...
Using data from the Plasma and Suprathermal Ion Composition (PLASTIC) instruments onboard the Solar ...
Interplanetary acceleration processes are shown as the most plausible explanation for the observed c...
Direct evidence of an inertial-range turbulent energy cascade has been provided by spacecraft observ...
This paper analyzes solar wind power spectra of bulk and thermal speed fluctuations that are compute...
The solar wind is the Sun's exosphere. As the solar atmosphere expands into interplanetary space, it...
A discussion of the solar wind and its interaction with bodies of the solar system is presented. An ...
The solar wind evolves as it moves outward due to interactions with both itself and with the circum-...
The local heating of the solar-wind gas during its expansion represents one of the most intriguing p...
The radial gradient of long-lived, corotating energetic particle streams was measured using observat...
A multi-institutional, multi-national science team will soon submit a NASA proposal to build a const...
We present a brief review of observations and theory regarding the nature and radial evolution of MH...