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相关论文: Sub-THz radiation mechanisms in solar flares

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Recent solar flare observations in the sub-THz range have provided evidence of a new spectral component with fluxes increasing for larger frequencies, separated from the well-known microwave emission that maximizes in the GHz range.…

太阳与恒星天体物理 · 物理学 2015-06-22 J. Michael Klopf , Pierre Kaufmann , Jean-Pierre Raulin , Sérgio Szpigel

Observations of solar flares at sub-THz frequencies (mm and sub-mm wavelengths) over the last two decades often show a spectral component rising with frequency. Unlike a typical gyrosynchrotron spectrum decreasing with frequency, or a weak…

太阳与恒星天体物理 · 物理学 2018-12-05 E. P. Kontar , G. G. Motorina , N. L. S. Jeffrey , Y. T. Tsap , G. D. Fleishman , A. V. Stepanov

The sub-THz event observed on the 4 July 2012 with the Bauman Moscow State Technical University Radio Telescope RT-7.5 at 93 and 140~GHz as well as Kislovodsk and Mets\"ahovi radio telescopes, Radio Solar Telescope Network (RSTN), GOES,…

The presence of a solar burst spectral component with flux density increasing with frequency in the sub-terahertz range, spectrally separated from the well-known microwave spectral component, bring new possibilities to explore the flaring…

Incoherent solar radio radiation comes from the free-free, gyroresonance, and gyrosynchrotron emission mechanisms. Free-free is primarily produced from Coulomb collisions between thermal electrons and ions. Gyroresonance and gyrosynchrotron…

太阳与恒星天体物理 · 物理学 2020-07-30 A. Nindos

Solar observations at sub-THz frequencies detected a new flare spectral component peaking in the THz range, simultaneously with the well known microwaves component, bringing challenging constraints for interpretation. Higher THz frequencies…

Recent advancements in spintronics have opened a new avenue in terahertz (THz) radiation sources that may outperform the traditional contact-based metallic counterparts. Inspired by the generation of broadband spintronic THz signals at the…

介观与纳米尺度物理 · 物理学 2025-04-25 Abbas Ghaffari , Malek Abdelsamei , Puja Thapa , Seiji Mita , Ramón Collazo , Kenan Gundogdu , Dali Sun , Qing Gu

In spintronic terahertz emitters, THz radiation is generated by exciting an ultrafast spin current through femtosecond laser excitation of a ferromagnetic-nonmagnetic metallic heterostructure. Although an extensive phenomenological…

材料科学 · 物理学 2024-11-22 Francesco Foggetti , Peter M. Oppeneer

A new solar burst emission spectral component has been found showing sub-THz fluxes increasing with frequency, spectrally separated from the well known microwave component. Rapid pulsations are found present in all events observed at the…

We derive simple formulas to explain terahertz (THz) emission from semiconductor surfaces excited by a femtosecond (fs) laser. Femtosecond optical pulses with energies larger than the bandgap create photocarriers which travel and generate…

应用物理 · 物理学 2020-09-01 Masayoshi Tonouchi

Properties of the solar radio spectrum, as well as the temporal profiles of flare emission, indicate the thermal nature of the sub-terahertz (sub-THz) component observed as the growth of radio emission in the frequency range of 100-1000…

太阳与恒星天体物理 · 物理学 2023-11-07 G. G. Motorina , Yu. T. Tsap , V. V. Smirnova , A. S. Morgachev , A. D. Shramko , A. S. Motorin

Solar observations in the infrared domain can bring important clues on the response of the low solar atmosphere to primary energy released during flares. At present the infrared continuum has been detected at 30 THz (10 $\mu$m) in only a…

太阳与恒星天体物理 · 物理学 2015-11-04 G. Trottet , J. -P. Raulin , A. MacKinnon , G. Giménez de Castro , P. J. A. Simões , D. Cabezas , V. de La Luz , M. Luoni , P. Kaufmann

The quiet Sun, i.e. in its non-flaring state or non-flaring regions, emits thermal radiation from radio to ultraviolet. The quiet Sun produces also non-thermal radiation observed in gamma rays due to interactions of Galactic Cosmic Rays…

高能天体物理现象 · 物理学 2023-02-15 Elena Orlando , Vahe' Petrosian , Andrew Strong

Ground- and space-based observations of solar flares from radio wavelengths to gamma-rays have produced considerable insights but raised several unsolved controversies. The last unexplored wavelength frontier for solar flares is in the…

Solar flares observed in the 200-400 GHz radio domain may exhibit a slowly varying and time-extended component which follows a short (few minutes) impulsive phase and which lasts for a few tens of minutes to more than one hour. The few…

太阳与恒星天体物理 · 物理学 2011-11-21 G. Trottet , J. -P. Raulin , G. Giménez de Castro , T. Lüthi , A. Caspi , C. H. Mandrini , M. L. Luoni , P. Kaufmann

Microwave emission of solar flares is formed primarily by incoherent gyrosynchrotron radiation generated by accelerated electrons in coronal magnetic loops. The resulting emission depends on many factors, including pitch-angle distribution…

太阳与恒星天体物理 · 物理学 2015-05-30 Alexey A. Kuznetsov , Gelu M. Nita , Gregory D. Fleishman

We develop a model for a possible origin of hard very high energy spectra from a distant blazar. In the model, both the primary photons produced in the source and secondary photons produced outside the source contribute to the observed high…

高能天体物理现象 · 物理学 2016-09-30 Y. G. Zheng , T. Kang

We report on terahertz (THz) radiation under electrical pumping from a degenerate semiconductor possessing an electron accumulation layer. In InN, the random grating formed by topographical defects provides high-efficiency coupling of…

材料科学 · 物理学 2015-05-19 T. V. Shubina , N. A. Gippius , V. A. Shalygin , A. V. Andrianov , S. V. Ivanov

The spectrum of gyrosynchrotron emission from solar flares generally peaks in the microwave range. Its optically-thin, high-frequency component, above the spectral peak, is often used for diagnostics of the nonthermal electrons and the…

太阳与恒星天体物理 · 物理学 2018-11-07 Gregory D. Fleishman , Maria A. Loukitcheva , Varvara Yu. Kopnina , Gelu M. Nita , Dale E. Gary

Based on a structure consisting of a single graphene layer situated on a periodic dielectric grating, we show theoretically that intense terahertz (THz) radiations can be generated by an electron bunch moving atop the graphene layer. The…

介观与纳米尺度物理 · 物理学 2015-06-18 T. R. Zhan , D. Z. Han , X. H. Hu , X. H. Liu , S. T. Chui , J. Zi
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