International audiencePurpose: Review of investigations of cosmic sources radioemission scintillations due to interplanetary plasma irregularities made at the Institute of Radio Astronomy of the National Academy of Sciences of Ukraine, from the first observations in the mid-70s until now. Design/methodology/approach: In the course of preparation of this paper, the authors have reviewed, analyzed and summarized the information being published in the home and foreign publications, and reported at scientific conferences. Findings: The investigations of the interplanetary scintillations carried out at the Institute of Radio Astronomy, NAS Ukraine have been reviewed. A retrospective discussion has been made on how in the course of these research...
This thesis presents several observational studies based on radio variability and interstellar scin...
The solar wind is a highly supersonic outflow of coronal plasma flowing in a close to radial directi...
International audienceThis paper will review the input of 65 years of radio observations to our unde...
International audiencePurpose: Review of investigations of cosmic sources radioemission scintillatio...
Purpose: Review of investigations of cosmic sources radioemission scintillations due to interplaneta...
This dissertation describes the measurement of angular diameters of compact radio sources by the tec...
International audienceThe present state of solar wind investigations by IPS (interplanetary scintill...
The present state of solar wind investigations by IPS (interplanetary scintillations) observations a...
Interplanetary scintillation is the fluctuation produced in the apparent brightness of a radio sourc...
The Physical Research Laboratory has been engaged in setting up a three-station radio observatory op...
The proposal to use ground based radio telescopes for detection of Askaryan radio pulses from partic...
Cosmic ray physics, which ten years ago was a fairly specialized branch of science, has in the cours...
During cosmic ray propagation in interplanetary space there appear characteristic cosmic-ray intensi...
Abstract: Nearly 50 years ago, the first radio signals from cosmic ray air showers were detected. Af...
Abstract: The Mexican Array Radio Telescope (MEXART) consist of a 64x64 (4096) full wavelength dipol...
This thesis presents several observational studies based on radio variability and interstellar scin...
The solar wind is a highly supersonic outflow of coronal plasma flowing in a close to radial directi...
International audienceThis paper will review the input of 65 years of radio observations to our unde...
International audiencePurpose: Review of investigations of cosmic sources radioemission scintillatio...
Purpose: Review of investigations of cosmic sources radioemission scintillations due to interplaneta...
This dissertation describes the measurement of angular diameters of compact radio sources by the tec...
International audienceThe present state of solar wind investigations by IPS (interplanetary scintill...
The present state of solar wind investigations by IPS (interplanetary scintillations) observations a...
Interplanetary scintillation is the fluctuation produced in the apparent brightness of a radio sourc...
The Physical Research Laboratory has been engaged in setting up a three-station radio observatory op...
The proposal to use ground based radio telescopes for detection of Askaryan radio pulses from partic...
Cosmic ray physics, which ten years ago was a fairly specialized branch of science, has in the cours...
During cosmic ray propagation in interplanetary space there appear characteristic cosmic-ray intensi...
Abstract: Nearly 50 years ago, the first radio signals from cosmic ray air showers were detected. Af...
Abstract: The Mexican Array Radio Telescope (MEXART) consist of a 64x64 (4096) full wavelength dipol...
This thesis presents several observational studies based on radio variability and interstellar scin...
The solar wind is a highly supersonic outflow of coronal plasma flowing in a close to radial directi...
International audienceThis paper will review the input of 65 years of radio observations to our unde...