PROJECT

Ventspils University of Applied Sciences` International Cooperation and Innovation for the Development of Latvia’s Smart Specialisation

Project title: “Ventspils University of Applied Sciences` International Cooperation and Innovation for the Development of Latvia’s Smart Specialisation”

 

Project No: 1.1.1.5/3/25/I/012

 

Project implementor: Ventspils University of Applied Sciences

 

Project duration: 01.06.2025. – 30.11.2029.

 

Total Budget: 568,000.00 euro: European Regional Development Fund (85,00%) – 482,800.00 euro and State Budget Funding (15%)– 85,200.00 euro.

 

The project aims to promote Latvia’s participation in international research initiatives and increase the competitiveness and global visibility of Latvian scientific institutions. In cooperation with ERIC consortia (JIV ERIC and LOFAR ERIC), it is planned to strengthen scientific capacity and excellence in radio astronomy, astrophysics, information technologies, data processing methods, and the development of new technologies.


To achieve these goals, existing research infrastructure and resources will be improved, new scientific methods and technologies will be developed, and knowledge transfer and integration of young researchers into the international scientific community will be promoted. Within the project framework, 16 international cooperation projects that exceed the quality threshold are planned for development.


Main activities:

  1. Support for the preparation of project applications submitted and evaluated above the quality threshold in the Horizon Europe programme and the 10th IP sub-programme competitions (at least 16 project applications).
  2. Ensuring participation in ERIC consortia and ESFRI platforms, including:
  • foreign and domestic business trips and service trips,
  • creation of communication materials,
  • organisation of conferences and seminars.

 

Contact information: Santa Kalvāne, santa.kalvane@venta.lv

PROJECT NEWS

By Martina Bertāne September 3, 2025
We are pleased to invite you to participate in the VIRAC Summer School on Pulsar Observations at Centimetre and Metre Wavelengths: Ventspils, Latvia |September 8–19, 2025 This intensive and inspiring summer school is designed for Master’s students, PhD candidates, and early-career researchers in astronomy and astrophysics. The event is hosted by Ventspils University of Applied Sciences. Key Topics: Pulsar observations with the LOFAR telescope Pulsar astronomy fundamentals Observation planning Pulsar data processing and analysis Venue: Engineering Research Institute – Ventspils International Radio Astronomy Centre, Ventspils University of Applied Sciences, Room 407
By Rota Rulle August 22, 2025
On August 18, 2025, Dr. Evanthia Hatziminaoglou from the European Southern Observatory (ESO) and the Instituto de Astrofísica de Canarias (IAC) delivered an insightful invited talk at the University of Latvia. The presentation provided a comprehensive overview of cutting-edge astronomical research and advancements, focusing on ESO's contributions, the ALMA telescope, the Atacama Large Aperture Submillimetre Telescope (AtLAST), and the study of quasars. Dr. Hatziminaoglou highlighted ESO's role as the leading intergovernmental astronomy organization, encompassing 16 member states and strategic partnerships with Chile and Australia. The talk showcased ESO's groundbreaking facilities, including the Very Large Telescope (VLT) at Paranal and the upcoming Extremely Large Telescope (ELT), set to be the largest optical/infrared telescope in the world. The presentation also delved into ALMA's capabilities, emphasizing its precision in resolving small details and its ongoing upgrades to enhance sensitivity. Dr. Hatziminaoglou discussed the AtLAST concept, a next-generation 50-meter single-dish observatory powered by renewable energy, designed to bridge gaps in angular scales, sensitivity, and mapping speed in submillimeter astronomy. A significant portion of the talk focused on the study of quasars, exploring their environments, star formation rates, and the triggers of extreme star formation in quasar hosts. Dr. Hatziminaoglou shared findings on multiplicities around SDSS quasars, revealing how submillimeter counterparts and redshift influence star formation rates and environments. In addition to the scientific presentation, there was a lively discussion on potential collaboration between the University of Latvia, Riga Technical University, and Ventspils University of Applied Sciences. The discussion emphasized creating pathways for Latvian researchers and students to engage with ESO and ALMA facilities, opening new opportunities for joint projects, training, and integration into international astronomy networks. This engaging presentation underscored the synergy between ESO's facilities, ALMA, and AtLAST, paving the way for future discoveries in astronomy. Dr. Hatziminaoglou's talk was an inspiring showcase of the collaborative efforts driving innovation in the field and inspiring the next generation of astronomers. Dr. Hatziminaoglou's talk was an inspiring showcase of the collaborative efforts driving innovation in the field and inspiring the next generation of astronomers. The seminar was organized within the framework of the project “Ventspils University of Applied Sciences` International Cooperation and Innovation for the Development of Latvia’s Smart Specialisation” (No. 1.1.1.5/3/25/I/012), co-financed by the European Regional Development Fund.
By Rota Rulle June 25, 2025
You are kindly invited to attend a scientific seminar that will take place on June 27, 2025 , at Room D407, VeA IZI VSRC . Seminar Programme 10:00 – 11:00 Prof. Valery M. Nakariakov , University of Warwick, UK "A Plasma Orchestra, or Magnetohydrodynamic Waves in the Solar Corona" 11:00 – 12:00 Lunch break 12:00 – 15:00 Scientific seminar “Magnetohydrodynamic Waves in the Solar Corona” as part of the JIV-ERIC National Node Scientific Seminar Series Please confirm your participation by marking your name in the Excel sheet: Participation Sheet You can join in person or online via Google Meet . Google Meet link --- A Plasma Orchestra, or Magnetohydrodynamic Waves in the Solar Corona Valery M Nakariakov (University of Warwick, United Kingdom) The corona of the Sun is the outermost part of the solar atmosphere. The corona is a very hot, fully ionised plasma dominated by the magnetic field. The corona is the birthplace of extreme events of space weather, and a natural laboratory for plasma physics. One of the most fascinated discoveries made with recent high-precision spaceborne imaging telescopes operating in the extreme UV band is the ubiquitous dynamics of the corona in a form of various large-scale wave motions. An example of such an instrument is the Extreme UV imager on the recently launched Solar Orbiter spacecraft. Typical oscillation periods are several minutes, typical wavelengths are tens to hundred thousand kilometres, and typical speeds are from several tens to several thousand kilometres per second, which make the solar coronal waves the largest electromagnetic wave motions resolved simultaneously in time and space, detected in the Universe. The observed waves are confidently interpreted in terms of the magnetohydrodynamic theory. Various plasma structures of the corona support different types of wave modes, allowing for the use of the waves for the plasma diagnostics via the method of magnetohydrodynamic seismology.