CHROMPHYS

Physics of the Solar Chromosphere

 Coordinatore UNIVERSITETET I OSLO 

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 Nazionalità Coordinatore Norway [NO]
 Totale costo 2˙487˙600 €
 EC contributo 2˙487˙600 €
 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-2011-ADG_20110209
 Funding Scheme ERC-AG
 Anno di inizio 2012
 Periodo (anno-mese-giorno) 2012-01-01   -   2016-12-31

 Partecipanti

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

 Organization address address: Problemveien 5-7
city: OSLO
postcode: 313

contact info
Titolo: Dr.
Nome: Ingse
Cognome: Noremsaune
Email: send email
Telefono: +47 228 55329
Fax: +47 228 54367

NO (OSLO) hostInstitution 2˙487˙600.00
2    UNIVERSITETET I OSLO

 Organization address address: Problemveien 5-7
city: OSLO
postcode: 313

contact info
Titolo: Prof.
Nome: Mats Per-Olof
Cognome: Carlsson
Email: send email
Telefono: +47 228 56536
Fax: +47 228 56505

NO (OSLO) hostInstitution 2˙487˙600.00

Mappa


 Word cloud

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

chromphys    corona    eruptions    space    energy    physics    iris    loading    wind    magnetic    chromosphere    diagnostics    chromospheric    affect    mass    data    solar    simulations   

 Obiettivo del progetto (Objective)

'CHROMPHYS aims at a breakthrough in our understanding of the solar chromosphere by combining the development of sophisticated radiation-magnetohydrodynamic simulations with observations from the upcoming NASA SMEX mission Interface Region Imaging Spectrograph (IRIS).

The enigmatic chromosphere is the transition between the solar surface and the eruptive outer solar atmosphere. The chromosphere harbours and constrains the mass and energy loading processes that define the heating of the corona, the acceleration and the composition of the solar wind, and the energetics and triggering of solar outbursts (filament eruptions, flares, coronal mass ejections) that govern near-Earth space weather and affect mankind's technological environment.

CHROMPHYS targets the following fundamental physics questions about the chromospheric role in the mass and energy loading of the corona:

- Which types of non-thermal energy dominate in the chromosphere and beyond?

- How does the chromosphere regulate mass and energy supply to the corona and the solar wind?

- How do magnetic flux and matter rise through the chromosphere?

- How does the chromosphere affect the free magnetic energy loading that leads to solar eruptions?

CHROMPHYS proposes to answer these by producing a new, physics based vista of the chromosphere through a three-fold effort:

- develop the techniques of high-resolution numerical MHD physics to the level needed to realistically predict and analyse small-scale chromospheric structure and dynamics,

- optimise and calibrate diverse observational diagnostics by synthesizing these in detail from the simulations, and

- obtain and analyse data from IRIS using these diagnostics complemented by data from other space missions and the best solar telescopes on the ground.'

Altri progetti dello stesso programma (FP7-IDEAS-ERC)

VARIOGEO (2011)

The Geometric Calculus of Variations and its Applications

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TADMICAMT (2014)

"Topological, Algebraic, Differential Methods in Classification and Moduli Theory"

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BIOWATER (2014)

"Development of new chemical imaging techniques to understand the function of water in biocompatibility, biodegradation and biofouling"

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