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This study aims to investigate the ambiguous source and the underlying physical processes of the solar type III radio bursts that occurred on April 3, 2019, through the utilization of multiwavelength observations from the LOFAR radio…

太阳与恒星天体物理 · 物理学 2023-12-20 Mohamed Nedal , Kamen Kozarev , Peijin Zhang , Pietro Zucca

Metric type II radio bursts are usually early indicators of CME-driven shocks and other space weather phenomena in the solar corona. This paper presents a detailed investigation of the spectral properties of band-splitting type II radio…

太阳与恒星天体物理 · 物理学 2023-02-28 F. N. Minta , S. Nozawa , K. Kozarev , A. Elsaid , A. Mahrous

Interferometric observations of the Sun with ALMA provide valuable diagnostic tools for studying the small-scale dynamics of the solar atmosphere. Estimations of the observability of the small-scale dynamics as a function of spatial…

太阳与恒星天体物理 · 物理学 2021-12-08 Henrik Eklund , Sven Wedemeyer , Mikołaj Szydlarski , Shahin Jafarzadeh

Based on detailed analysis of radio and X-ray observations of a flare on 2002 April 11 augmented by realistic 3D modeling, we have identified a radio emission component produced directly at the flare acceleration region. This acceleration…

太阳与恒星天体物理 · 物理学 2015-06-15 Gregory D. Fleishman , Eduard P. Kontar , Gelu M. Nita , Dale E. Gary

Photonic methods of radio-frequency waveform generation and processing provide performance and flexibility over electronic methods due to the ultrawide bandwidth offered by the optical carriers. However, they suffer from lack of integration…

Over the last years, radio detection has matured to become a competitive method for the detection of air showers. Arrays of thousands of antennas are now envisioned for the detection of cosmic rays of ultra high energy or neutrinos of…

The Dual-zone Aperture X-ray Solar Spectrometer (DAXSS) was flown on 2018 June18 on the NASA 36.336 sounding rocket flight and obtained the highest resolution to date for solar soft X-ray (SXR) spectra over a broad energy range. This…

太阳与恒星天体物理 · 物理学 2020-11-24 Bennet D. Schwab , Robert H. A. Sewell , Thomas N. Woods , Amir Caspi , James Paul Mason , Christopher Moore

We present observational results from studying the quasi-periodicities in global solar radio flux during periods of enhanced noise storm activity, over durations of ~4 hrs a day ("intra-day" variations), observed at 77.5 MHz with the newly…

天体物理学 · 物理学 2007-05-23 G. A. Shanmugha Sundaram , K. R. Subramanian

Spectrograph slit is conventionally used to enhance the spectral resolution and manage how much light can be allowed to enter spectrograph. A narrower slit provides a higher resolution but sacrifices efficiency of spectrograph and results…

天体物理仪器与方法 · 物理学 2013-06-10 FengFei Wang , HaoTong Zhang , A-Li Luo , ZhongRui Bai , Bing Du , YongHeng Zhao

The solar radiation spectrum is important for renewable energy harvesting, as well as climate and ecological systems analysis. In addition to seasonal/annual and diurnal oscillations, the signal is composed of different frequencies ($f$)…

地球物理 · 物理学 2018-11-01 Golan Bel , Mahesh M. Bandi

For the first time we present simulation results of the focusing effect of the ionospheric plasma density irregularities, namely, Medium Scale Traveling Ionospheric Disturbances (MSTIDs), on solar radio emission by applying a ray-tracing…

太阳与恒星天体物理 · 物理学 2018-12-26 Artem Koval , Yao Chen , Aleksander Stanislavsky , Anton Kashcheyev , Qing-He Zhang

A technique of timescale analysis performed directly in the time domain has been developed recently. We have applied the technique to studying rapid variabilities of hard X-rays from neutron star and black hole binaries, gamma-ray bursts…

天体物理学 · 物理学 2016-01-27 T. P. Li

Solar radio type II bursts are slow-drifting bursts that exhibit various distinct features such as Fundamental (F) and Harmonic (H) emissions, band-splitting, and discrete fine structures in the dynamic spectra. Observationally, it has been…

太阳与恒星天体物理 · 物理学 2025-11-20 Rishikesh G. Jha , K. Sasikumar Raja , R. Ramesh , C. Kathiravan , Christian Monstein

The spatial-frequency coverage of a radio interferometer is increased by combining samples acquired at different times and observing frequencies. However, astrophysical sources often contain complicated spatial structure that varies within…

天体物理仪器与方法 · 物理学 2015-06-11 U. Rau

The dynamic spectrum of a radio pulsar is an in-line digital hologram of the ionised interstellar medium. It has previously been demonstrated that such holograms permit image reconstruction, in the sense that one can determine an…

天体物理学 · 物理学 2009-11-13 Mark Walker , Leon Koopmans , Dan Stinebring , Willem van Straten

We study temporal variations in the amplitudes and widths of high-degree acoustic modes in the quiet and active Sun by applying ring-diagram technique to the GONG+ and MDI Dopplergrams during the declining phase of cycle 23. The increase in…

太阳与恒星天体物理 · 物理学 2015-05-20 Olga Burtseva , S. C. Tripathy , R. Howe , K. Jain , F. Hill , R. Bogart , M. C. Rabello-Soares

The National Laboratory of Space Weather in Mexico (Laboratorio Nacional de ClimaEspacial: LANCE) coordinates instrumentation for monitoring the space-weatherimpact over Mexico. Two of these instruments are the Mexican Array Radio…

Current and future continuum surveys being undertaken by the new generation of radio telescopes are now poised to address many important science questions, ranging from the earliest galaxies, to the physics of nearby AGN, as well as…

天体物理仪器与方法 · 物理学 2016-04-25 Jeremy J. Harwood , Raffaella Morganti

We design an event recognition-analysis system that can automatically detect solar type III radio burst and can mine information of the burst from the dynamic spectra observed by Nancay Decameter Array (NDA). We investigate the frequency…

太阳与恒星天体物理 · 物理学 2018-10-09 Peijin Zhang , Chuan Bing Wang , Lin Ye

Solar neutrinos coming from different nuclear reactions are now detected with a high statistics. Consequently, an accurate spectroscopic analysis of the neutrino fluxes arriving on the Earth's detectors become available, in the context of…

太阳与恒星天体物理 · 物理学 2013-02-13 Ilídio Lopes , Sylvaine Turck-Chièze