What is he best known for?
The fields of study he is best known for:
- Astronomy
- Astrophysics
- Photon
Åke Nordlund mostly deals with Astrophysics, Magnetohydrodynamics, Convection, Computational physics and Classical mechanics.
As part of his studies on Astrophysics, Åke Nordlund often connects relevant subjects like Field strength.
His work carried out in the field of Magnetohydrodynamics brings together such families of science as Magnetic flux, Corona and Nanoflares.
The Convection study combines topics in areas such as Radiative transfer and Radiative cooling.
His Computational physics research includes elements of Helioseismology and Interplanetary magnetic field.
His Classical mechanics research is multidisciplinary, incorporating elements of Shock wave and Mechanics.
His most cited work include:
- A grid of MARCS model atmospheres for late-type stars. I. Methods and general properties (1998 citations)
- Dynamo-generated Turbulence and Large-Scale Magnetic Fields in a Keplerian Shear Flow (760 citations)
- Simulations of Solar Granulation. I. General Properties (656 citations)
What are the main themes of his work throughout his whole career to date?
His primary scientific interests are in Astrophysics, Convection, Computational physics, Mechanics and Turbulence.
The various areas that Åke Nordlund examines in his Astrophysics study include Spectral line and Magnetohydrodynamics.
His research integrates issues of Magnetic flux and Corona in his study of Magnetohydrodynamics.
His Convection research focuses on Radiative transfer and how it relates to Opacity.
His Computational physics research is multidisciplinary, relying on both Particle acceleration, Weibel instability and Optics.
His Mechanics study combines topics in areas such as Classical mechanics and Dynamo.
He most often published in these fields:
- Astrophysics (54.32%)
- Convection (35.45%)
- Computational physics (22.50%)
What were the highlights of his more recent work (between 2011-2021)?
- Astrophysics (54.32%)
- Stars (14.77%)
- Molecular cloud (10.45%)
In recent papers he was focusing on the following fields of study:
The scientist’s investigation covers issues in Astrophysics, Stars, Molecular cloud, Turbulence and Computational physics.
The concepts of his Astrophysics study are interwoven with issues in Radiative transfer, Magnetohydrodynamics and Convection.
His Stars research includes themes of Grid and Mass distribution.
His study explores the link between Molecular cloud and topics such as Initial mass function that cross with problems in Brown dwarf.
His work investigates the relationship between Turbulence and topics such as Order of magnitude that intersect with problems in Distribution function.
His studies deal with areas such as Astrophysical jet, Particle acceleration and Jet as well as Computational physics.
Between 2011 and 2021, his most popular works were:
- The absolute chronology and thermal processing of solids in the solar protoplanetary disk. (520 citations)
- SUPERNOVA DRIVING. I. THE ORIGIN OF MOLECULAR CLOUD TURBULENCE (164 citations)
- Supernova Driving. I. The Origin of Molecular Cloud Turbulence (164 citations)
In his most recent research, the most cited papers focused on:
- Astronomy
- Astrophysics
- Photon
Åke Nordlund focuses on Astrophysics, Stars, Molecular cloud, Computational physics and Magnetohydrodynamics.
His Astrophysics research is multidisciplinary, incorporating perspectives in Radiative transfer, Thermal and Dissipation.
Åke Nordlund interconnects Grid and Convection in the investigation of issues within Stars.
His Molecular cloud research integrates issues from Star formation, Protostar, Solar System, Supernova and Mass distribution.
Åke Nordlund has included themes like Stellar structure and Solar flare in his Computational physics study.
His Magnetohydrodynamics study incorporates themes from Magnetic flux, Magnetogram, Magnetic reconnection and Particle acceleration.
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