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Jul 22, 2014

Electron Cyclotron Maser Emission in Coronal Arches and Solar Radio Type V Bursts

According to the close association of type V solar bursts with type III bursts, we propose that solar radio type V bursts are excited by the electron cyclotron maser instability. The work by J. F. Tang, D. J. Wu and C. M. Tan has been pu...
Nov 25, 2013

Particle Simulations Reveal Small-Scale Energy Dissipation of Solar Storm

Because the transportation of energy from a solar storm is a large scale problem, in the long term, the Magnetohydrodynamics (MHD) method can better resolve processes related to transportation of the solar wind in the heliosphere.However...
Nov 20, 2013

XAO Developed the OTF Observation Model to Improve Observing Efficiency

OTF model is an observation method which controls the telescope moving uniformly, in the same time, recording the spectrum line data in a high sample rate, to finish a map of specifically region. OTF model can highly improve the efficien...
Oct 01, 2013

XAO Signed MOU with NRAO to Enhance Scientific Cooperation

Xinjiang Astronomical Observatory (XAO) and the National Radio Astronomy Observatory (NRAO) signed the “Memorandum of Agreement for Scientific and Technical Consultation on the Planned Qi-Tai Radio Telescope (QTT) Astronomical Radio Tel...
Sep 30, 2013

Pulsar Group of XAO Found Nine glitches in the Crab pulsar

Nine glitches in the Crab pulsar have been observed by pulsar group of Xinjiang Astronomical Observatory, including the largest glitch for this pulsar. Pulsar glitches are characterized by the sudden increases in pulse frequency. Glitche...
Sep 17, 2013

Professor Christian Henkel from Max Planck Institute had visited XAO

From June 24th to 26th, 2013, Professor Christian Henkel from Max Planck Institute for Radio Astronomy had visited XAO. During this visit, Professor Henkel gave a presentation entitled "New Masers, Physical Constants, Densities and Tempe...

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