OSFair2017 Workshop | OpenAIRE services and activities for training, support/helpdesk, community engagement

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Iryna Kuchma presents OpenAIRE services and community engagement | OSFair2017 Workshop Workshop title: National and European e-infrastructure cooparation for Open Science Workshop overview: This collaborative workshop comes in the context of coordinating EOSC related activities across large European infrastructures at European and national level. The workshop will offer an opportunity for cross-pollination on issues ranging from open scholarship to technical service provision, training, community engagement and support. OpenAIRE NOADs, EGI NGIs, GEANT NRENs and other national e-Infrastructure representatives will discuss gaps, synergies, coordination and service integration opportunities. DAY 3 - PARALLEL SESSION 6 & 7

Sciences

@openaire_eu
OpenAIREservicesandactivitiesfortraining,
support/helpdesk,communityengagement
IrynaKuchma
EIFL

EGI GEANT OpenAIRE Workshop 2
OpenAIRE fosters the social and technical links
that enable Open Science in Europe and beyond
Human
Network
Digital
Network
50 Partners from every EU country, and beyond
Data centers, universities, libraries, repositories, legal experts

Ourkeystakeholders
EGI GEANT OpenAIRE Workshop

Howdoweengage?
EGI GEANT OpenAIRE Workshop
Network Helpdesk
Services
Direct outreach
Global alignment
Tenders

Research is global, support is
local
EGI GEANT OpenAIRE Workshop 5

Humaninfrastructure
EGI GEANT OpenAIRE Workshop 6
Human support network
• 33 expert nodes all
over Europe helping
with:
• OA training and
support
• OA policy alignment
(PASTEUR4OA)
• Technical assistance

EGI GEANT OpenAIRE Workshop 7
National
Workshops

Support and training
EGI GEANT OpenAIRE Workshop 8

EGI GEANT OpenAIRE Workshop 9
Guides &
Factsheets
FAQs

EGI GEANT OpenAIRE Workshop 10
Workshops

Building partnerships
Global
alignment
EGI GEANT OpenAIRE Workshop 12

Building bridges with the
international community
13
“bloor viaduct”, https://www.flickr.com/photos/43021516@N06/, CC BY-SA 2.0
Synergies with COAR,
CLARA, WDS, …

Attracting SMEs & young
investigators
Tenders
EGI GEANT OpenAIRE Workshop 14

Tenders
Innovative scholarly communication models and/or services
Services targeting repository platforms (e.g., ResourceSync, new
protocols)
SME's services basedon opendata/open publications
OpenAIRE-Advance: adedicated taskon"open innovation"
EGI GEANT OpenAIRE Workshop 15

Collaborations
Joint webinars and other training events
Co-creation of materials
Joint train-the-trainers events
EGI GEANT OpenAIRE Workshop 16

Thank you!
https://www.openaire.eu
@OpenAIRE_eu

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Botany 4th semester file By Sumit Kumar yadav.pdf

Sumit Kumar yadav

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Lokesh Kothari

Understanding circumstellar disks is of prime importance in astrophysics, however, their birth process remains poorly constrained due to observational and numerical challenges. Recent numerical works have shown that the small-scale physics, often wrapped into a sub-grid model, play a crucial role in disk formation and evolution. This calls for a combined approach in which both the protostar and circumstellar disk are studied in concert. Aims. We aim to elucidate the small scale physics and constrain sub-grid parameters commonly chosen in the literature by resolving the star-disk interaction. Methods. We carry out a set of very high resolution 3D radiative-hydrodynamics simulations that self-consistently describe the collapse of a turbulent dense molecular cloud core to stellar densities. We study the birth of the protostar, the circumstellar disk, and its early evolution (< 6 yr after protostellar formation). Results. Following the second gravitational collapse, the nascent protostar quickly reaches breakup velocity and sheds its surface material, thus forming a hot (∼ 103 K), dense, and highly flared circumstellar disk. The protostar is embedded within the disk, such that material can flow without crossing any shock fronts. The circumstellar disk mass quickly exceeds that of the protostar, and its kinematics are dominated by self-gravity. Accretion onto the disk is highly anisotropic, and accretion onto the protostar mainly occurs through material that slides on the disk surface. The polar mass flux is negligible in comparison. The radiative behavior also displays a strong anisotropy, as the polar accretion shock is shown to be supercritical whereas its equatorial counterpart is subcritical. We also f ind a remarkable convergence of our results with respect to initial conditions. Conclusions. These results reveal the structure and kinematics in the smallest spatial scales relevant to protostellar and circumstellar disk evolution. They can be used to describe accretion onto regions commonly described by sub-grid models in simulations studying larger scale physics.

Formation of low mass protostars and their circumstellar disks

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Formation of low mass protostars and their circumstellar disks

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