The present state of solar wind investigations by IPS (interplanetary scintillations) observations at decameter wavelengths is discussed. Radio telescopes, equipment and methods which are used in these experiments are shown. We also describe some interesting results devoted to the long term monitoring of the solar wind beyond Earth’s orbit, the detection of the large scale disturbances associated with active processes at the Sun and the reconstructions of the solar wind stream structure. Emphasis is placed on perspectives of low frequency IPS investigations which are particularly connected with the creation of the Giant Ukrainian Radio Telescopes (GURT) and UTR-2 – URAN – GURT – LOFAR collaboration
The technique of interplanetary scintillation (IPS) is the observation of rapid fluctuations of the ...
We present an overview of the recent results in solar observations obtained at decameter radio waves...
Purpose: Review of investigations of cosmic sources radioemission scintillations due to interplaneta...
International audienceThe present state of solar wind investigations by IPS (interplanetary scintill...
International audiencePurpose: Review of investigations of cosmic sources radioemission scintillatio...
The solar wind is a highly supersonic outflow of coronal plasma flowing in a close to radial directi...
Rapid progress currently takes place in the field of low-frequency radio astronomy in the meter–deca...
International audienceWe describe the trends and tasks in the field of lowfrequency studies of radio...
International audienceWith the aim of evaluating the actual possibilities of doing, from the ground,...
International audienceRapid progress currently takes place in the field of low-frequency radio astro...
The density and velocity structure of the solar wind can be studied by examining the scintillation e...
The Physical Research Laboratory has been engaged in setting up a three-station radio observatory op...
International audienceResults of the last observations of solar sporadic radio emission at the UTR-2...
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...
The technique of interplanetary scintillation (IPS) is the observation of rapid fluctuations of the ...
We present an overview of the recent results in solar observations obtained at decameter radio waves...
Purpose: Review of investigations of cosmic sources radioemission scintillations due to interplaneta...
International audienceThe present state of solar wind investigations by IPS (interplanetary scintill...
International audiencePurpose: Review of investigations of cosmic sources radioemission scintillatio...
The solar wind is a highly supersonic outflow of coronal plasma flowing in a close to radial directi...
Rapid progress currently takes place in the field of low-frequency radio astronomy in the meter–deca...
International audienceWe describe the trends and tasks in the field of lowfrequency studies of radio...
International audienceWith the aim of evaluating the actual possibilities of doing, from the ground,...
International audienceRapid progress currently takes place in the field of low-frequency radio astro...
The density and velocity structure of the solar wind can be studied by examining the scintillation e...
The Physical Research Laboratory has been engaged in setting up a three-station radio observatory op...
International audienceResults of the last observations of solar sporadic radio emission at the UTR-2...
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...
The technique of interplanetary scintillation (IPS) is the observation of rapid fluctuations of the ...
We present an overview of the recent results in solar observations obtained at decameter radio waves...
Purpose: Review of investigations of cosmic sources radioemission scintillations due to interplaneta...