TGF-MEPPA

Terrestrial Gamma Flashes-the Most Energetic Photon Phenomenon in our Atmosphere

 Coordinatore UNIVERSITETET I BERGEN 

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 Nazionalità Coordinatore Norway [NO]
 Totale costo 2˙492˙811 €
 EC contributo 2˙492˙811 €
 Programma FP7-IDEAS-ERC
Specific programme: "Ideas" implementing the Seventh Framework Programme of the European Community for research, technological development and demonstration activities (2007 to 2013)
 Code Call ERC-2012-ADG_20120216
 Funding Scheme ERC-AG
 Anno di inizio 2013
 Periodo (anno-mese-giorno) 2013-03-01   -   2018-02-28

 Partecipanti

# participant  country  role  EC contrib. [€] 
1    UNIVERSITETET I BERGEN

 Organization address address: Museplassen 1
city: BERGEN
postcode: 5007

contact info
Titolo: Ms.
Nome: Liv-Grethe
Cognome: Gudmundsen
Email: send email
Telefono: 4755584965
Fax: 4755584991

NO (BERGEN) hostInstitution 2˙492˙811.00
2    UNIVERSITETET I BERGEN

 Organization address address: Museplassen 1
city: BERGEN
postcode: 5007

contact info
Titolo: Prof.
Nome: Nikolai
Cognome: østgaard
Email: send email
Telefono: +47 55582794
Fax: +47 55589440

NO (BERGEN) hostInstitution 2˙492˙811.00

Mappa


 Word cloud

Esplora la "nuvola delle parole (Word Cloud) per avere un'idea di massima del progetto.

implications    related    electric    ray    mev    lightning    atmosphere    gamma    flashes    thunderstorm    photon    energies    questions    tgf    relativistic    electrical    electrons    space    gt    km    energetic    phenomenon    tgfs    earth    circuit   

 Obiettivo del progetto (Objective)

'Only 20 years after the discovery of Cosmic Gamma-ray Bursts from the universe another completely unknown phenomenon involving gamma-rays was discovered by coincidence the BATSE instrument on the Compton Gamma-Ray Observatory. Short-lived (~1 ms) and very energetic photon emissions (>1 MeV and later: >40 MeV) were found to originate from the Earth’s atmosphere and were named Terrestrial Gamma Flashes (TGFs). These flashes are the most energetic natural photon phenomenon that is known to exist on Earth, in which also anti-matter is produced. Based on the few datasets available to date we believe that TGFs are related to electric discharges in thunderstorm systems and that electrons accelerated to relativistic energies are involved to produce bremsstrahlung of such high energies. However, it is not known how frequent TGFs are, the altitude range and the spatial extent of their source region, to what kind of thunderstorms and lightning they are related or the implications of relativistic electrons and positrons ejected into space. There is no consensus on how TGFs are produced. All these questions need to be answered before we understand how important they are and how they may affect the Earth’s electrical circuit and atmosphere.

The goal of the TGF-MEPPA project is to attack these questions by combining modelling of electron acceleration in thunderstorm electric fields, X- and gamma-ray production and propagation, lightning development with unprecedented measurements of TGFs from three different altitudes: 350 km, 30 km and 20 km to obtain the most comprehensive and detailed dataset needed to make significant advances in the TGF research. I will also perform electric discharge experiments in the laboratory. The goal is to establish a consistent model for the TGF-production and answer the question ‘How common are TGFs?’ to determine their implications for the Earth’s electrical circuit, atmosphere and outer space.'

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