Explore the words cloud of the new-ppd-environments project. It provides you a very rough idea of what is the project "new-ppd-environments" about.
The following table provides information about the project.
LEIBNIZ-INSTITUT FUR ASTROPHYSIK POTSDAM (AIP)
|Coordinator Country||Germany [DE]|
|Total cost||1˙392˙763 €|
|EC max contribution||1˙392˙763 € (100%)|
1. H2020-EU.1.1. (EXCELLENT SCIENCE - European Research Council (ERC))
|Duration (year-month-day)||from 2015-06-01 to 2020-05-31|
Take a look of project's partnership.
|1||LEIBNIZ-INSTITUT FUR ASTROPHYSIK POTSDAM (AIP)||DE (POTSDAM)||coordinator||323˙319.00|
|2||KOBENHAVNS UNIVERSITET||DK (KOBENHAVN)||participant||1˙069˙443.00|
The aim of this ambitious research project is to produce the most realistic computer simulations of gaseous protoplanetary accretion discs to date, and thereby define in an assertive way the environment that shapes the assembly and early evolution of planetary systems. In their role as planet nurseries, protoplanetary discs are of key interest to planet formation theory. Their dynamical, radiative and thermodynamic properties critically define the environment for embedded solids: dust grains, pebbles and planetesimals. In short, the building blocks of planet formation. The discs’ dynamics and structure in turn depend critically on the influence of magnetic fields that couple to tenuously ionised and low-density regions. Being comparatively cold and dense, the ionisation state of the disc plasma is dominated by external far-UV, X-Ray, and cosmic-ray radiation, leading to a layered vertical structure – with turbulent, magnetised surface layers and a magnetically-decoupled midplane. This classic ‘dead-zone’ picture is now turned upside-down by previously ignored micro-physical effects. For instance, ambipolar diffusion is predicted to dominate in the tenuous hot corona of the disc. It is expected that parts of the disc will thus be stabilised and a magneto-centrifugal wind will be launched. This has so far only been studied in very simplified local models that are affected by fundamental limitations. Our understanding of the structure of protoplanetary discs is about to undergo a dramatic shift, and my proposed research is at the forefront of this development. My recent successful work at the interface between MHD dynamics and planet formation theory makes me ideally skilled to lead a research group in this endeavour and to communicate advancements to a wide audience of theoreticians in planet formation. Our ambitious global simulations will furthermore provide realistic templates to interpret new observations made with the ALMA telescope array.
|year||authors and title||journal||last update|
Toward realistic simulations of magneto-thermal winds from weakly-ionized protoplanetary disks
published pages: , ISSN: , DOI:
|Proceedings, 11th International Conference on Numerical Modeling of Space Plasma Flows (ASTRONUM-2016)||2019-05-28|
Karin I. Ã–berg, Viviana V. GuzmÃ¡n, Christopher J. Merchantz, Chunhua Qi, Sean M. Andrews, L. Ilsedore Cleeves, Jane Huang, Ryan A. Loomis, David J. Wilner, Christian Brinch, Michiel Hogerheijde
H 2 CO Distribution and Formation in the TW HYA Disk
published pages: 43, ISSN: 1538-4357, DOI: 10.3847/1538-4357/aa689a
|The Astrophysical Journal 839/1||2019-05-28|
Colin P. McNally, Richard P. Nelson, Sijme-Jan Paardekooper, Oliver Gressel, Wladimir Lyra
Low mass planet migration in magnetically torqued dead zones â€“ I. Static migration torque
published pages: 1565-1575, ISSN: 0035-8711, DOI: 10.1093/mnras/stx2136
|Monthly Notices of the Royal Astronomical Society 472/2||2019-05-28|
O. M. Umurhan, R. P. Nelson, O. Gressel
Linear analysis of the vertical shear instability: outstanding issues and improved solutions
published pages: A33, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201526494
|Astronomy & Astrophysics 586||2019-05-28|
Pablo BenÃtez-Llambay, Martin E. Pessah
Torques Induced by Scattered Pebble-flow in Protoplanetary Disks
published pages: L28, ISSN: 2041-8213, DOI: 10.3847/2041-8213/aab2ae
|The Astrophysical Journal 855/2||2019-05-28|
Yuri I. Fujii, Hiroshi Kobayashi, Sanemichi Z. Takahashi, Oliver Gressel
Orbital Evolution of Moons in Weakly Accreting Circumplanetary Disks
published pages: 194, ISSN: 1538-3881, DOI: 10.3847/1538-3881/aa647d
|The Astronomical Journal 153/4||2019-05-28|
Lee Hartmann, Fred Ciesla, Oliver Gressel, Richard Alexander
Disk Evolution and the Fate of Water
published pages: 813-834, ISSN: 0038-6308, DOI: 10.1007/s11214-017-0406-0
|Space Science Reviews 212/1-2||2019-05-28|
Philipp Weber, Pablo BenÃtez-Llambay, Oliver Gressel, Leonardo Krapp, Martin E. Pessah
Characterizing the Variable Dust Permeability of Planet-induced Gaps
published pages: 153, ISSN: 1538-4357, DOI: 10.3847/1538-4357/aaab63
|The Astrophysical Journal 854/2||2019-05-28|
Christian Brinch, Jes K. JÃ¸rgensen, Michiel R. Hogerheijde, Richard P. Nelson, Oliver Gressel
MISALIGNED DISKS IN THE BINARY PROTOSTAR IRS 43
published pages: L16, ISSN: 2041-8213, DOI: 10.3847/2041-8205/830/1/L16
|The Astrophysical Journal 830/1||2019-05-28|
P. Bjerkeli, J. K. JÃ¸rgensen, C. Brinch
A young bipolar outflow from IRASâ€‰15398-3359
published pages: A145, ISSN: 0004-6361, DOI: 10.1051/0004-6361/201527310
|Astronomy & Astrophysics 587||2019-05-28|
Krapp, Leonardo; Gressel, Oliver; BenÃtez-Llambay, Pablo; Downes, Turlough P.; Mohandas, Gopakumar; Pessah, Martin E.
Dust segregation in Hall-dominated turbulent protoplanetary disks
published pages: 105, ISSN: 1538-4357, DOI:
|The Astrophysical Journal 865||2019-03-18|
Are you the coordinator (or a participant) of this project? Plaese send me more information about the "NEW-PPD-ENVIRONMENTS" 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 (email@example.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 "NEW-PPD-ENVIRONMENTS" are provided by the European Opendata Portal: CORDIS opendata.