Tor Flå
University of Tromsø
32 Papers
65 Citations
Tor Flå is an academic researcher from University of Tromsø. The author has contributed to research in topics: Modulational instability & Nonlinear system. The author has an hindex of 11, co-authored 30 publications. Previous affiliations of Tor Flå include National Center for Atmospheric Research.
Chat about Author
Papers
Fully adaptive algorithms for multivariate integral equations using the non-standard form and multiwavelets with applications to the Poisson and bound-state Helmholtz kernels in three dimensions
TL;DR: A general formalism for fast numerical solution of time-independent linear partial differential equations as well as integral equations through the application of numerically separable integral operators in d ≥ 1 dimensions using the non-standard (NS) form is developed.
58
DeltaProt : a software toolbox for comparative genomics
TL;DR: The DeltaProt Toolbox is presented, a software toolbox that may be useful in importing, analyzing and visualizing data from multiple alignments of proteins, written in MATLAB™ to provide an easy and user-friendly platform, including a graphical user interface, while ensuring good numerical performance.
18
Dynamical models of mutated chronic myelogenous leukemia cells for a post-imatinib treatment scenario: Response to dasatinib or nilotinib therapy.
TL;DR: This work focuses on modelling the time dependence of imatinib-resistant clones upon subsequent exposure to dasatinib or nilotinib, and implements a new feedback mechanism for regulation of coupling between cycling and non-cycling stem cell reservoirs that depends on total cell populations.
A numerical energy conserving method for the DNLS equation
TL;DR: In this paper, an implicit, numerical energy conserving method for the derivative nonlinear Schrodinger (DNLS) equation for periodic boundary conditions is developed, which is used to follow the nonlinear behavior of the DNLS modulational instability.
8
Alfvén-wave acceleration of the solar wind.
TL;DR: In this article, the increase in mass flux and energy flux from the Sun is calculated for an increasing Alfven-wave amplitude, δv76561 0, in the lower corona and fixed values for the coronal pressure, the Coronal temperature and the interplanetary magnetic field.
6