Opendata, web and dolomites

PROMINENT SIGNED

Solar prominences: unraveling the ultimate condensation catastrophe

Total Cost €

0

EC-Contrib. €

0

Partnership

0

Views

0

 PROMINENT project word cloud

Explore the words cloud of the PROMINENT project. It provides you a very rough idea of what is the project "PROMINENT" about.

radiatively    resolution    eruption    causes    resolve    gravity    cloud    magnetically    physicists    giant    contexts    mediated    spontaneously    adaptive    orbiter    effort    structure    limits    natural    ejections    gigantic    june    shapes    conclusive    grid    answers    initio    generation    barbs    itself    software    forthcoming    mysterious    magnetic    catastrophic    spectacular    pervade    seismologically    mysteries    weight    feet    mass    tornadoes    little    poorly    ultimate    eruptions    size    1946    4th    train    advent    ab    oscillation    gravitationally    intriguing    prominence    heliosphere    million    recorded    surprisingly    riddles    weather    parker    simulations    unravel    dominant    disappearance    frequencies    ejection    instabilities    fundamental    history    cool    body    feasible    found    violent    topology    sizes    formed    structures    inner    thermal    supercomputers    grand    population    form    probe    astrophysical    space    easily    confront    fine    corona    solar    daddy    observations    outweighs    historic    dense    quantify    revolutionary    missions    plasma    predict    degree    condensations    threads    condense    invariably    earth    involve    armed    induce    coronal   

Project "PROMINENT" data sheet

The following table provides information about the project.

Coordinator
KATHOLIEKE UNIVERSITEIT LEUVEN 

Organization address
address: OUDE MARKT 13
city: LEUVEN
postcode: 3000
website: www.kuleuven.be

contact info
title: n.a.
name: n.a.
surname: n.a.
function: n.a.
email: n.a.
telephone: n.a.
fax: n.a.

 Coordinator Country Belgium [BE]
 Total cost 2˙331˙250 €
 EC max contribution 2˙331˙250 € (100%)
 Programme 1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
 Code Call ERC-2018-ADG
 Funding Scheme ERC-ADG
 Starting year 2019
 Duration (year-month-day) from 2019-09-01   to  2024-08-31

 Partnership

Take a look of project's partnership.

# participants  country  role  EC contrib. [€] 
1    KATHOLIEKE UNIVERSITEIT LEUVEN BE (LEUVEN) coordinator 2˙331˙250.00

Map

 Project objective

The most spectacular solar eruptions recorded in history - such as the Grand Daddy Prominence eruption on the 4th of June 1946 - invariably involve the violent ejection of a prominence: a giant, cool and dense plasma cloud that formed spontaneously within the million-degree solar corona. The role of the dominant prominence mass in all magnetically mediated coronal mass ejections is poorly understood, and yet a typical prominence easily outweighs our Earth population in mass (and the Earth itself in size). While they pervade the solar corona in all shapes and sizes, surprisingly little is known on their formation and ultimate disappearance. At the advent of two revolutionary space missions to the inner reaches of our heliosphere (Parker Probe and Solar Orbiter), a dedicated effort on ab initio prominence simulations beyond current resolution limits is needed. This must provide conclusive answers to intriguing riddles: How, where and why does the solar corona spontaneously condense to form these gigantic structures? What is the magnetic field topology throughout the prominence body, and how can it support their weight against solar gravity? What causes the fine structure (so-called threads and barbs) throughout the prominence body, and what is the role of the mysterious solar tornadoes often found at their feet? Can we use their natural oscillation frequencies seismologically? Is it feasible to predict their eruption, and can one quantify their role in space weather contexts? Armed with state-of-the-art, grid-adaptive software to efficiently exploit current and next generation supercomputers, we will resolve these mysteries, confront historic and forthcoming observations, and train a new generation of solar physicists. Along the way, we unravel fundamental processes relevant in many astrophysical contexts: how do radiatively driven, thermal instabilities induce catastrophic, non-gravitationally mediated condensations?

Are you the coordinator (or a participant) of this project? Plaese send me more information about the "PROMINENT" project.

For instance: the website url (it has not provided by EU-opendata yet), the logo, a more detailed description of the project (in plain text as a rtf file or a word file), some pictures (as picture files, not embedded into any word file), twitter account, linkedin page, etc.

Send me an  email (fabio@fabiodisconzi.com) and I put them in your project's page as son as possible.

Thanks. And then put a link of this page into your project's website.

The information about "PROMINENT" are provided by the European Opendata Portal: CORDIS opendata.

More projects from the same programme (H2020-EU.1.1.)

Resonances (2019)

Resonances and Zeta Functions in Smooth Ergodic Theory and Geometry

Read More  

Aware (2019)

Aiding Antibiotic Development with Deep Analysis of Resistance Evolution

Read More  

TAMING CORROSION (2020)

Towards mastering the long-standing challenge of ageing infrastructures in corrosive environments

Read More