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Related papers: A Two Year Survey for VLF Emission from Fireballs

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Blazars are a subclass of active galactic nuclei (AGN) having relativistic jets aligned within a few degrees of our line-of-sight and form the majority of the AGN detected in the TeV regime. The Fermi-Large Area Telescope (LAT) is a…

High Energy Astrophysical Phenomena · Physics 2023-07-04 Atreya Acharyya , Alberto C. Sadun

We analyze here two very bright fireballs produced by the ablation in the atmosphere of two large meteoroids in 2009 and 2010. These slow-moving and deep-penetrating events were observed over Spain in the framework of our Spanish Fireball…

Earth and Planetary Astrophysics · Physics 2015-06-22 Jose M. Madiedo , Josep M. Trigo-Rodriguez , Jose L. Ortiz , Alberto J. Castro-Tirado , Jesus Cabrera-Caño

On 25 October 2012 the Reuven Ramaty High Energy Solar Spectroscope Imager (RHESSI) and the Tropical Rainfall Measuring Mission (TRMM) satellites passed over a thunderstorm on the coast of Sri Lanka. RHESSI observed a terrestrial gamma ray…

Space Physics · Physics 2017-08-25 Thomas Gjesteland , Nikolai Østgaard , Phillip Bitzer , Hugh J. Christian

We present multi-epoch astrometric observations of the M9 ultra-cool dwarf TVLM513-46546 that is placed at the brown dwarf boundary. The new observations have been performed with the European VLBI Network (EVN) at 6cm band. The target has…

Solar and Stellar Astrophysics · Physics 2017-01-18 Marcin P. Gawronski , Krzysztof Gozdziewski , Krzysztof Katarzynski

This paper presents the results of a nearly two year long campaign to detect and analyze meteor persistent trains (PTs) - self-emitting phenomena which can linger up to an hour after their parent meteor. The modern understanding of PTs has…

Earth and Planetary Astrophysics · Physics 2024-07-29 L. E. Cordonnier , K. S. Obenberger , J. M. Holmes , G. B. Taylor , D. Vida

Context. The existence of meteor clusters has long since been a subject of speculation and so far only seven events have been reported, among which two involve less than five meteors, and three were seen during the Leonid storms. Aims. The…

Terrestrial Gamma ray Flashes (TGFs) -- very short, intense bursts of electrons, positrons, and energetic photons originating from terrestrial thunderstorms -- have been detected with satellite instruments. TETRA, an array of NaI(Tl)…

High Energy Astrophysical Phenomena · Physics 2013-12-20 Rebecca Ringuette , Gary L. Case , Michael L. Cherry , Douglas Granger , T. Gregory Guzik , Michael Stewart , John P. Wefel

Superfireballs are rare phenomena for which the reports are scarce and the estimation of their abundance has a huge margin of uncertainty. As a citizen science project we have gathered >500 reports from newspapers in the 1850-2000 period.…

Earth and Planetary Astrophysics · Physics 2015-12-22 Sandra Zamora , Fancisco Ocaña , Alejandro Sánchez de Miguel , Maruška Mole

The atmospheric aerosol monitoring system of the Pierre Auger Observatory has been operating smoothly since 2004. Two laser facilities (Central Laser Facility, CLF and eXtreme Laser Facility, XLF) fire sets of 50 shots four times per hour…

Instrumentation and Methods for Astrophysics · Physics 2019-06-12 Laura Valore

Terrestrial gamma-ray flashes (TGFs) are the most energetic photon phenomenon occurring naturally on Earth. An outstanding question is as follows: Are these flashes just a rare exotic phenomenon or are they an intrinsic part of lightning…

Space Physics · Physics 2016-05-19 N. Østgaard , K. H. Albrechtsen , T. Gjesteland , A. Collier

Experiments that observe coherent radio emission from extensive air showers induced by ultra-high energy cosmic rays are designed for a detailed study of the development of the electromagnetic part of air showers. Radio detectors can…

Instrumentation and Detectors · Physics 2019-08-21 Zbigniew Szadkowski

In this paper, we present the first high-speed video observation of a cloud-to-ground lightning flash and its associated downward-directed Terrestrial Gamma-ray Flash (TGF). The optical emission of the event was observed by a high-speed…

Atmospheric and Oceanic Physics · Physics 2023-08-11 R. U. Abbasi , M. M. F. Saba , J. W. Belz , P. R. Krehbiel , W. Rison , N. Kieu , D. R. da Silva , Dan Rodeheffer , M. A. Stanley , J. Remington , J. Mazich , R. LeVon , K. Smout , A. Petrizze , T. Abu-Zayyad , M. Allen , Y. Arai , R. Arimura , E. Barcikowski , D. R. Bergman , S. A. Blake , I. Buckland , B. G. Cheon , M. Chikawa , T. Fujii , K. Fujisue , K. Fujita , R. Fujiwara , M. Fukushima , G. Furlich , N. Globus , R. Gonzalez , W. Hanlon , N. Hayashida , H. He , K. Hibino , R. Higuchi , K. Honda , D. Ikeda , N. Inoue , T. Ishii , H. Ito , D. Ivanov , H. Iwakura , A. Iwasaki , H. M. Jeong , S. Jeong , C. C. H. Jui , K. Kadota , F. Kakimoto , O. Kalashev , K. Kasahara , S. Kasami , S. Kawakami , K. Kawata , I. Kharuk , E. Kido , H. B. Kim , J. H. Kim , J. H. Kim , S. W. Kim , Y. Kimura , I. Komae , Y. Kubota , V. Kuzmin , M. Kuznetsov , Y. J. Kwon , K. H. Lee , B. Lubsandorzhiev , J. P. Lundquist , H. Matsumiya , T. Matsuyama , J. N. Matthews , R. Mayta , I. Myers , S. Nagataki , K. Nakai , R. Nakamura , T. Nakamura , T. Nakamura , Y. Nakamura , A. Nakazawa , E. Nishio , T. Nonaka , H. Oda , S. Ogio , M. Ohnishi , H. Ohoka , Y. Oku , T. Okuda , Y. Omura , M. Ono , A. Oshima , S. Ozawa , I. H. Park , M. Potts , M. S. Pshirkov , J. Remington , D. C. Rodriguez , C. Rott , G. I. Rubtsov , D. Ryu , H. Sagawa , N. Sakaki , T. Sako , N. Sakurai , K. Sato , T. Seki , K. Sekino , P. D. Shah , Y. Shibasaki , N. Shibata , T. Shibata , J. Shikita , H. Shimodaira , B. K. Shin , H. S. Shin , D. Shinto , J. D. Smith , P. Sokolsky , B. T. Stokes , T. A. Stroman , K. Takahashi , M. Takamura , M. Takeda , R. Takeishi , A. Taketa , M. Takita , Y. Tameda , K. Tanaka , M. Tanaka , Y. Tanoue , S. B. Thomas , G. B. Thomson , P. Tinyakov , I. Tkachev , H. Tokuno , T. Tomida , S. Troitsky , R. Tsuda , Y. Tsunesada , S. Udo , T. Uehama , F. Urban , D. Warren , T. Wong , M. Yamamoto , K. Yamazaki , K. Yashiro , F. Yoshida , Y. Zhezher , Z. Zundel

Given the possible repetitive nature of fast radio bursts (FRBs), their cosmological origin, and their high occurrence, detection of strongly lensed sources due to intervening galaxy lenses is possible with forthcoming radio surveys. We…

High Energy Astrophysical Phenomena · Physics 2017-09-27 Liang Dai , Wenbin Lu

The origin and phenomenology of the Fast Radio Burst (FRB) remains unknown despite more than a decade of efforts. Though several models have been proposed to explain the observed data, none is able to explain alone the variety of events so…

High Energy Astrophysical Phenomena · Physics 2021-03-26 Luciano Nicastro , Cristiano Guidorzi , Eliana Palazzi , Luca Zampieri , Massimo Turatto , Angela Gardini

We present the analysis of the atmospheric trajectory and orbital data of four bright bolides observed over Spain, one of which is a potential meteorite dropping event. Their absolute magnitude ranges from -10 to -11. Two of these are of…

Earth and Planetary Astrophysics · Physics 2015-06-16 J. M. Madiedo , J. M. Trigo-Rodriguez , J. L. Ortiz , A. J. Castro-Tirado , S. Pastor , J. A. de los Reyes , J. Cabrera-Cano

The total energy of a fireball is commonly obtained from optical measurements with an assumed value for luminous efficiency. Acoustic energy measurements offer an independent means of energy estimation. Here we combine optical and acoustic…

Earth and Planetary Astrophysics · Physics 2024-08-09 Luke McFadden , Peter Brown , Denis Vida

We report results of a novel high-energy follow-up observation of a potential Fast Radio Burst. The radio burst was detected by VLA/realfast and followed-up by the Neil Gehrels Swift Observatory in very low latency utilizing new operational…

We describe the arrival time measurements and timing modeling of the periodic radio flares and optical brightness variations of the M9 ultracool dwarf, TVLM 513-46546. We confirm the stability of the observed period and determine its…

Solar and Stellar Astrophysics · Physics 2015-06-19 A. Wolszczan , M. Route

Bright optical transients (i.e. transients typically visible with the naked eye) are populated mainly by novae eruptions plus a few supernovae (among which the SN1987a event). One bright nova happen every two years, either in the North ot…

Solar and Stellar Astrophysics · Physics 2014-07-22 Florentin Millour , Olivier Chesneau , Anthony Meilland , Nicolas Nardetto

Fast Radio Bursts (FRBs) are extremely energetic pulses of millisecond duration and unknown origin. In order to understand the phenomenon that emits these pulses, targeted and untargeted searches have been performed for multi-wavelength…