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*** Heliosphere News Feb. 16, 2016 ***
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Editor: Nathan Schwadron (nschwadron@unh.edu)

Co-Editor: Mihir Desai (mdesai@swri.edu)

Co-Editor: Eric Zirnstein (ezirnstein@swri.edu)

 

If you are interested in posting an announcement (e.g., meeting or workshop information, recent publications, job opportunities etc.,) please send information to Nathan, Mihir or Eric. Posts are limited to ascii text. Newsletters are archived on the following website:

 

http://heliospherenews.unh.edu/



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**ANNOUNCEMENTS
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  1. COSPAR 2016 Deadline Extension
  2. ASTRONUM-2016
  3. New Publications
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*1) COSPAR 2016 ABSTRACTS DUE DATE HAS BEEN EXTENDED TO FEBRUARY 19 at 23:59 UTC14

COSPAR 2016: General Information

COSPAR 41st Scientific Assembly
July 30 - August 7, 2016
Istanbul Congress Center (ICC), Turkey

Website:
http://cospar2016.tubitak.gov.tr/en/default.asp

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*2) ASTRONUM-2016


Monterey, California, USA, 6–10 June, 2016

 

Maison de la Simulation (CEA/CNRS/UPS/UVSQ), France will organize ASTRONUM 2016 – the 11th International Conference on Numerical Modeling of Space Plasma Flows in Monterey, California, USA, on 6–10 June, 2016. The conference web site is

https://www.icnsmeetings.com/conference/astronum2016/index.html

 

The conference will cover the following topics:

 

(1) Advanced numerical methods for space, astrophysical and geophysical flows; (2) Large-scale fluid-based, kinetic, and hybrid simulations;

(3) Turbulence and cosmic ray transport; (4) Magnetohydrodynamics

(5) Software packages for modeling and analyzing plasma flows / Visualisation

 

with the application to

 

(1) Physics of the Sun-Heliosphere-Magnetosphere; 

(2) Interstellar medium and star formation;

(3) Cosmology and galaxy formation; 

(4) Dynamo effect;

(5) Stellar Physics.

 

The purpose of the conference is to bring together leading experts in applied mathematics, space physics, astrophysics, and geophysics to discuss the application of novel numerical algorithms and petascale paral- lelization strategies to computationally challenging problems.

The conference will be structured around invited, 40-minute keynote and 25-minute regular talks, and a limited number of contributed talks, with the attempt to have no parallel sessions. The conference web site icnsmeetings.com will provide the information about the conference venue, registration, and means of transportation. E-mail inquiries about the meeting should be directed to Nikolai.Pogorelov@uah.edu and Edouard.Audit@cea.fr.

 

Program Committee: Tahar Amari (CNRS Ecole Polytechnique), Edouard Audit (CEA, Maison de la Simulation, co-chair), Amitava Bhattacharjee (Princeton Plasma Physics Laboratory), Phillip Colella (Lawrence Berkeley National Laboratory), Anthony Mezzacappa (University of Tennessee, Knoxville),  Ewald Mu¨ller (Max-Planck-Institute for Astrophysics, Garching), Nikolai Pogorelov (University of Alabama in Huntsville, chair), Kazunari Shibata (Kyoto University), James Stone (Princeton University), Jon Linker (Predictive Science Inc.), and Gary P. Zank (University of Alabama in Huntsville).

 

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*3) Zirnstein, E. J., Heerikhuisen, J., Funsten, H. O., Livadiotis, G., McComas, D. J., & Pogorelov, N. V. 2016, ApJL, 818, L18

 “Local Interstellar Magnetic Field Determined from the Interstellar Boundary Explorer Ribbon”

 DOI: http://dx.doi.org/10.3847/2041-8205/818/1/L18


Best regards,


       Mihir

_______________________________________________________________________
Dr. Mihir I Desai  Tel: +1 210 522 6754

Director, Department of Space Research  Cell: +1 210 454 1671

Space Science & Engineering Division  Fax: +1 210 520 9935

Southwest Research Institute  Email: mdesai@swri.edu 
6220 Culebra Road, 

San Antonio TX 78238-5166, USA  

Regular Mail: P.O. Drawer 28510, San Antonio, TX 78228-0510, USA
Overnight deliveries: 9503 W. Commerce, San Antonio, TX  78238-5166, USA
 
Lead Adjoint Professor
Department of Physics and Astronomy
University of Texas, San Antonio
One UTSA Circle, San Antonio, 
Texas 78249-0697, USA

________________________________________________________________________