EISCAT measurements of solar wind velocity and the associated level of interplanetary scintillatio
141 [34] leaves : ill. ; 27 cm.Thesis (Ph.D.) -- University of Adelaide, Dept. of Physics, 197
Single station solar wind velocity measurements using the Ooty Radio Telescope (ORT) in India (opera...
We present results of observations of interplanetary scintillation (IPS) made using the telescopes o...
Observations of interplanetary scintillation (IPS) allow accurate solar wind velocity measurements ...
519-524Solar wind velocities can be estimated from high signal-to-noise interplanetary scintillation...
The solar wind is a highly supersonic outflow of coronal plasma flowing in a close to radial directi...
International audienceA relative scintillation index can be derived from EISCAT observations of Inte...
The solar maximum solar wind is highly structured in latitude, longitude and in time. Coronal me...
The technique of interplanetary scintillation (IPS) is the observation of rapid fluctuations of the ...
International audienceEISCAT observations of interplanetary scintillation have been used to measure ...
Abstract: Interplanetary scintillation measurements can yield estimates of a large number of solar w...
Co-rotating interaction regions (CIRs) between fast and slow streams of plasma are a prominent feat...
Interplanetary scintillation measurements can yield estimates of a large number of solar wind pa...
The density and velocity structure of the solar wind can be studied by examining the scintillation e...
Abstract. Interplanetary scintillation measurements can yield estimates of a large number of solar w...
141 [34] leaves : ill. ; 27 cm.Thesis (Ph.D.) -- University of Adelaide, Dept. of Physics, 197
Single station solar wind velocity measurements using the Ooty Radio Telescope (ORT) in India (opera...
We present results of observations of interplanetary scintillation (IPS) made using the telescopes o...
Observations of interplanetary scintillation (IPS) allow accurate solar wind velocity measurements ...
519-524Solar wind velocities can be estimated from high signal-to-noise interplanetary scintillation...
The solar wind is a highly supersonic outflow of coronal plasma flowing in a close to radial directi...
International audienceA relative scintillation index can be derived from EISCAT observations of Inte...
The solar maximum solar wind is highly structured in latitude, longitude and in time. Coronal me...
The technique of interplanetary scintillation (IPS) is the observation of rapid fluctuations of the ...
International audienceEISCAT observations of interplanetary scintillation have been used to measure ...
Abstract: Interplanetary scintillation measurements can yield estimates of a large number of solar w...
Co-rotating interaction regions (CIRs) between fast and slow streams of plasma are a prominent feat...
Interplanetary scintillation measurements can yield estimates of a large number of solar wind pa...
The density and velocity structure of the solar wind can be studied by examining the scintillation e...
Abstract. Interplanetary scintillation measurements can yield estimates of a large number of solar w...
141 [34] leaves : ill. ; 27 cm.Thesis (Ph.D.) -- University of Adelaide, Dept. of Physics, 197
Single station solar wind velocity measurements using the Ooty Radio Telescope (ORT) in India (opera...
We present results of observations of interplanetary scintillation (IPS) made using the telescopes o...