215 citations
- Mahidol UniversityTH2 papers
- National Astronomical Research Institute of ThailandTH2 papers
- American Association of Variable Star ObserversUS1 paper
- Bundesdeutsche Arbeitsgemeinschaft für Veränderliche SterneDE1 paper
- California Institute of TechnologyUS1 paper
- Christian-Albrechts-Universität zu KielDE1 paper
- Chulalongkorn UniversityTH1 paper
- Goddard Space Flight CenterUS1 paper
- HeliophysicsUS1 paper
- Instituto de Astrofísica de CanariasES1 paper
- Kasetsart UniversityTH1 paper
- Liverpool John Moores UniversityGB1 paper
5 papers
Magnetic Field Line Separation by Random Ballistic Decorrelation in Transverse Magnetic Turbulence
Chutima Yannawa, Peera Pongkitiwanichakul, David Ruffolo +2
The statistics of the magnetic field line separation provide insight into how a bundle of field lines spreads out and the dispersion of non-thermal particles in a turbulent environ…
Random Walk and Trapping of Interplanetary Magnetic Field Lines: Global Simulation, Magnetic Connectivity, and Implications for Solar Energetic Particles
Rohit Chhiber, David Ruffolo, William H. Matthaeus +4
The random walk of magnetic field lines is an important ingredient in understanding how the connectivity of the magnetic field affects the spatial transport and diffusion of charge…
Photometric Investigation of Novae T Pyx, BT Mon and V574 Pup at Quiescence by using the 2.4 m Thai National Telescope
Ritthichai Thipboon, Metichai Kaewrakmuk, Farung Surina +1
Recurrent novae (RNe) are novae with multiple recorded outbursts powered by a thermonuclear runaway. The outburst occurs on the surface of the white dwarf which accompanies with a…
Evolution of V339 Del (Nova Del 2013) since 0.37 to 75 Days after Discovery
Y. Mueangkon, S. Khamrat, D. Suekong +5
We study the evolution of V339 Del (Nova Del 2013) during 0.37 to 75 days after discovery. Spectra from the Liverpool Telescope were collected and analysed to find velocity of ejec…
A radio pulsing white dwarf binary star
T. R. Marsh, B. T. Gänsicke, S. Hümmerich +23
White dwarfs are compact stars, similar in size to Earth but ~200,000 times more massive. Isolated white dwarfs emit most of their power from ultraviolet to near-infrared wavelengt…