Nettsider med emneord «Simulations»
Gene expression is regulated though long-range interactions with enhancer and silencer elements that come into close contact with promoter regions in three-dimensional (3D) space. However, the mechanism is not understood.
The Rosseland Centre for Solar physics continues growing and attracting young, talented researchers. Get to know four new PhD students at the beginning of their scientific ventures.
– I find neutron stars to be some of the coolest and most fascinating objects in the universe, says Jakob Borg new Ph.D. fellow at the Institute of Theoretical Astrophysics.
Paul Shapiro, Department of Astronomy, The University of Texas at Austin (USA).
Luis Teodoro, Centre for Space Sensors and Systems, Faculty of Mathematics and Natural Sciences, University of Oslo.
Rüdiger Pakmor, Max Planck Institute for Astrophysics, Germany.
Cheng-Zong Ruan, Postdoctoral Fellow at Institute of Theoretical Astrophysics, University of Oslo.
Thore Espedal Moe, PhD fellow of Rosseland Centre for Solar Physics (RoCS), University of Oslo.
– I am fascinated about the use of machine learning in different fields and its applications for society in the future, says Dennis Fremstad, new Ph.D. fellow at the Institute of Theoretical Astrophysics.
Lars Frogner, PhD fellow of Rosseland Centre for Solar Physics (RoCS), University of Oslo.
ModelDB provides an accessible location for storing and efficiently retrieving computational neuroscience models.
You find the entry for Neuronify here.
"My research goal? Constraining cosmological and gravitational models and discovering the nature of dark energy".
"I just think galaxies are really, really, cool! I mean have you seen pictures? Who wouldn’t want to know more about those things?", Bendix Hagedorn, new Ph.D. student at the Institute of Theoretical Astrophysics.
"It is really cool to quantitatively describe things in the sky using physical theories developed on earth" - Cheng-Zong Ruan, new postdoc at ITA.
Max Grönke, Max Planck Institute for Astrophysics, Garching (Germany).
The SolarALMA project was funded with a Consolidator Grant by the European Research Council (ERC) and ran from September 2016 to August 2021. The aim was to utilise the first observations of the Sun with the Atacama Large Millimeter/submillimeter Array (ALMA), which promises significant steps towards understanding the outer layers of the solar atmosphere with possible contributions to solving the coronal heating problem.
The project aims to understand the origin of the element, fluorine, in our Galaxy and also advance our knowledge on the dust formation in evolved stars.
Øystein Håvard Færder, Rosseland Centre for Solar Physics, University of Oslo.
Øystein Håvard Færder, Ph.D. student at Rosseland Centre for Solar Physics, University of Oslo.
Simulation is the most important method for verifying correct operation of electronics during the design phase. However, developing and using efficient simulation tools that are both accurate and fast, becomes an increasing challenge as circuits increases from thousands to billions of transistors. A possibility is to have several different types of description of the same module and toggle between these depending on needs. In this way we may toggle between more accurate (and slower) representations, and faster (and less accurate) representations depending on what is our requirements.