The Physical Research Laboratory has been engaged in setting up a three-station radio observatory operating at a frequency of 103 MHz in western India for exploration of the heliosphere by the interplanetary scintillation (IPS) technique. The three radio telescopes are separated by about 200 km from each other and are being operated as 'transit' telescopes in correlation interferometer mode with excellent relative time accuracy. IPS observations of scintillating radio sources made over a wide range of their solar elongations permit determination of not only the solar wind velocity at different heliolatitudes and other traveling interplanetary disturbances, but also the structure of the heliosphere up to a distance of about 1.0 AU
We present the first dedicated observations of Interplanetary Scintillation (IPS) with the Murchison...
Small scale turbulence in the solar wind causes radio sources to scintillate and it has been found t...
Purpose: Review of investigations of cosmic sources radioemission scintillations due to interplaneta...
Abstract. Interplanetary scintillation (IPS) remote-sensing observations provide a view of the solar...
The solar wind is a highly supersonic outflow of coronal plasma flowing in a close to radial directi...
519-524Solar wind velocities can be estimated from high signal-to-noise interplanetary scintillation...
Observations of interplanetary scintillation (IPS) allow accurate solar wind velocity measurements t...
The technique of interplanetary scintillation (IPS) is the observation of rapid fluctuations of the ...
The density and velocity structure of the solar wind can be studied by examining the scintillation e...
Interplanetary scintillation (IPS) is a phenomenon that has been known of and used as a measuring te...
We have carried out a program of continuous Interplanetary Scintillation (IPS) monitoring of the int...
International audienceThe present state of solar wind investigations by IPS (interplanetary scintill...
International audiencePurpose: Review of investigations of cosmic sources radioemission scintillatio...
The present state of solar wind investigations by IPS (interplanetary scintillations) observations a...
This dissertation describes the measurement of angular diameters of compact radio sources by the tec...
We present the first dedicated observations of Interplanetary Scintillation (IPS) with the Murchison...
Small scale turbulence in the solar wind causes radio sources to scintillate and it has been found t...
Purpose: Review of investigations of cosmic sources radioemission scintillations due to interplaneta...
Abstract. Interplanetary scintillation (IPS) remote-sensing observations provide a view of the solar...
The solar wind is a highly supersonic outflow of coronal plasma flowing in a close to radial directi...
519-524Solar wind velocities can be estimated from high signal-to-noise interplanetary scintillation...
Observations of interplanetary scintillation (IPS) allow accurate solar wind velocity measurements t...
The technique of interplanetary scintillation (IPS) is the observation of rapid fluctuations of the ...
The density and velocity structure of the solar wind can be studied by examining the scintillation e...
Interplanetary scintillation (IPS) is a phenomenon that has been known of and used as a measuring te...
We have carried out a program of continuous Interplanetary Scintillation (IPS) monitoring of the int...
International audienceThe present state of solar wind investigations by IPS (interplanetary scintill...
International audiencePurpose: Review of investigations of cosmic sources radioemission scintillatio...
The present state of solar wind investigations by IPS (interplanetary scintillations) observations a...
This dissertation describes the measurement of angular diameters of compact radio sources by the tec...
We present the first dedicated observations of Interplanetary Scintillation (IPS) with the Murchison...
Small scale turbulence in the solar wind causes radio sources to scintillate and it has been found t...
Purpose: Review of investigations of cosmic sources radioemission scintillations due to interplaneta...