Add to ORKGThe new Interplanetary scintillation (IPS) observation system which is under construction at the National Astronomical Observatories, CAS (NAOC) is introduced and the principle of the solar wind speed observation by using normalized cross-spectrum of simultaneous dual-frequency IPS measurements is also described in this paper. 1
Abstract. Interplanetary scintillation (IPS) remote-sensing observations provide a view of the solar...
519-524Solar wind velocities can be estimated from high signal-to-noise interplanetary scintillation...
International audienceRapid progress currently takes place in the field of low-frequency radio astro...
The results of observations of interplanetary scintillation (IPS) using the telescopes of EISCAT, in...
The technique of interplanetary scintillation (IPS) is the observation of rapid fluctuations of the ...
Observations of interplanetary scintillation (IPS) allow accurate solar wind velocity measurements ...
Improvements to two of the radio telescopes of European Incoherent SCATter radar (EISCAT) allow meas...
International audienceThe present state of solar wind investigations by IPS (interplanetary scintill...
The Physical Research Laboratory has been engaged in setting up a three-station radio observatory op...
The antennas of EISCAT have been used for interplanetary scintillation (IPS) studies of the solar w...
The solar wind is a highly supersonic outflow of coronal plasma flowing in a close to radial directi...
The present state of solar wind investigations by IPS (interplanetary scintillations) observations a...
We have carried out a program of continuous Interplanetary Scintillation (IPS) monitoring of the int...
Two station IPS observations can be used to measure the solar wind velocity when the velocity is par...
We investigated the propagation of solar wind using the radio signal transmitted by the Mars Reconna...
Abstract. Interplanetary scintillation (IPS) remote-sensing observations provide a view of the solar...
519-524Solar wind velocities can be estimated from high signal-to-noise interplanetary scintillation...
International audienceRapid progress currently takes place in the field of low-frequency radio astro...
The results of observations of interplanetary scintillation (IPS) using the telescopes of EISCAT, in...
The technique of interplanetary scintillation (IPS) is the observation of rapid fluctuations of the ...
Observations of interplanetary scintillation (IPS) allow accurate solar wind velocity measurements ...
Improvements to two of the radio telescopes of European Incoherent SCATter radar (EISCAT) allow meas...
International audienceThe present state of solar wind investigations by IPS (interplanetary scintill...
The Physical Research Laboratory has been engaged in setting up a three-station radio observatory op...
The antennas of EISCAT have been used for interplanetary scintillation (IPS) studies of the solar w...
The solar wind is a highly supersonic outflow of coronal plasma flowing in a close to radial directi...
The present state of solar wind investigations by IPS (interplanetary scintillations) observations a...
We have carried out a program of continuous Interplanetary Scintillation (IPS) monitoring of the int...
Two station IPS observations can be used to measure the solar wind velocity when the velocity is par...
We investigated the propagation of solar wind using the radio signal transmitted by the Mars Reconna...
Abstract. Interplanetary scintillation (IPS) remote-sensing observations provide a view of the solar...
519-524Solar wind velocities can be estimated from high signal-to-noise interplanetary scintillation...
International audienceRapid progress currently takes place in the field of low-frequency radio astro...