disk formation from collapsing cloud core

Date	Name	Institute	Reason
5/29/19	David Hendriks <​d.hendriks@surrey.ac.uk>	Astrophysics department Surrey	My planned use for this code is to simulate a binary system where the mass-transfer leads to an accretion disc. I'm interested in the motion of the disc material, and want to investigate eccentric modes within this disc. AstroBear seems to be very extensive and on first sight I think it will suit my needs for my project.
4/16/19	Lydia Heck <​lydia.heck@durham.ac.uk>	Durham University, ICC	Help a user to get the code compiled for her use
4/16/19	Matthew Archer <​ma595@cam.ac.uk>	University of Cambridge	Test on University of Cambridge cluster (Skylakes)
3/8/19	Legg, Cyrus <​j.legg.17@ucl.ac.uk>	UCL London
2/28/19	Antonio Tegon <​antonio.tegon@gmail.com>	Circolo Astrofili "Guido Ruggieri" Marghera-Venezia ( Italy)	Be star disks simulations
2/27/19	Giancarlo Conselvan <​conselvan.giancarlo@gmail.com>	Astrofili Marghera	Magnetic fields of Be stars disk
2/3/19	花輪知幸 Tomoyuki Hanawa <​hanawa@faculty.chiba-u.jp>	IAU CB1	list up public astrophysical simulation codes on our website
8/13/18	Jackson Bates <​jkb1473@rit.edu>	Rochester Institute of Technology	Self-Educational purposes
8/6/18	Alice Allen <​aallen@ascl.net>	Astrophysics Source Code Library/UMD	Testing availability of code
7/16/18	Owain Kenway <​o.kenway@ucl.ac.uk>	UCL London	Central install on our HPC services for users of the clusters.
6/15/18	Ming Xu <​xuming@mail.ustc.edu.cn>	Institute of Applied Physics and Computational Mathematics,Beijing,P.R.China	Simulation of magnetic reconnection
6/7/18	Patrick Mullen <​pmullen2@illinois.edu>	University of Illinois at Urbana-Champaign	I am a 2nd year computational astrophysics student in Prof. C. F. Gammie's research group at UIUC. I am interested in self-gravity with AMR and hope to look further into the test problem of Bonnor-Ebert sphere equilibria.
2/2/18	Edward Edmondson <​eddedmondson+astrobear@gmail.com>	UCL London	Install for researchers.
2/1/18	Florian Kirchschlarger <​f.kirchschlager@ucl.ac.uk>	UCL London	I want to perform MHD calculations for the simulation of shocks impacting a supernova remnant. I am working together with Erica Fogerty.
2/1/18	Franziska Schmidt <​f.schmidt.16@ucl.ac.uk>	UCL London	I want to perform MHD calculations for the simulation of shocks impacting a supernova remnant. I am working together with Erica Fogerty.
12/9/17	Arunachalam B. <​barunva@gmail.com>	NIT Trichy India	use the AstroBear software for my research.
9/19/17	Chris Osborne <​2087801O@student.gla.ac.uk>	University of Glasgow	Evaluation for a PhD project on Alfvenic Heating of the Solar Chromosphere during flaring events
9/15/17	Dhritimaan Gogoi <​dhritimaan.gogoi@outlook.com>	Gauahati University	3d MHD Simulation
5/9/17	Arash Afshar <​afsharph@gmail.com>	Department of Mechanical Engineering UR	I am a PhD student in Department of Mechanical Engineering that work about Magneto hydrodynamics and plasma.
3/21/17	Juan Manzanero <​juan.manzanero@upm.es>	Universidad Politécnica de Madrid	I am a CFD developer, and I am interested to solve the MHD equations.
3/21/17	Xiaoliang Zhang <​zxlgwu@gwmail.gwu.edu>	George Washington University	For our own research work on MHD simulations.
3/6/17	Jose Nandez <​javendan@uwo.ca>	University of Western Ontario	I have performed numerical interactions between RG and BH, as well, as RG + MS using our own distribution of SPH. However, I would like to test your code for angular momentum around the Roche Lobe of a MS + RG, since I want to follow mass flow, I believe another code is required for this task since SPH is good to trace the total amount in the flow, but it is not capable of following mass flows. Also, does your code include a way to add recombination energy in the equation of state?
11/3/16	Jesus Salas<​jesusms@astro.ucla.edu>	University of California - Los Angeles	Hydrodynamical simulations of molecular clouds
10/26/16	Braden Howell <​braden_howell_@hotmail.com>	University of Toronto	I intend to use this code to study stellar winds and accretion disks
9/29/16	Wenshuai Liu<​liuwenshuai2006@126.com>	Nanjing Normal University	Accretion disk
6/28/16	Huchi Li <​hcli@mail.sdu.edu.cn>	Shandong University	Study MHD
6/28/16	Gang Li <​en-super@hotmail.com>	Peking University	Learn computational MHD
3/22/16	Miguel Avillez <​mavillez@uevora.pt>	University of Evora, Portugal	I would like to use learn the ASTROBEAR code and try to implement time-dependent ionisation structure following my previous work. I also would like to use the code in teaching courses on computational astrophysics.
2/23/16	Gustavo <​grsilva@princeton.edu>	Princeton University	Comparison between different codes
12/6/15	Dominik Schleicher <​dschleicher@astro-udec.cl>	Department of Astronomy, Universidad de Concepcion	Modeling of circumbinary disk formation (Master student project)
11/24/15	WeiGang Zeng <​cengwg14@mails.tsinghua.edu.cn>	Tsinghua University	For Fluid Dynamic simulation
10/30/15	Dinh van Trung; ​dvtrung@iop.vast.ac.vn	Institute of Physics, Vietnam Academy of Science and Technology	I plan to simulate star and planet interaction
10/23/15	Mariana Cecere	Instituto de Astronomía Teórica y Experimental CONICET-UNC Argentina	I am studying resistive MHD and would like to try to work with this code
6/1/15	Carmen Tornow	Inst. of Planetary Research	protoplanetary disk evolution
2/2/15	Frank Otto	The Chinese University of Hong Kong	Investigate star formation in molecular clouds
2/2/15	Gustavo Salgado Enriquez	Universidad Complutense de Madrid	Study of wave structures and transport scheme
9/18/14	Manuel	University of Birmingham	Research
9/18/14	Roberto Toscano-Fletes	Dep. Fisica UdeG, Universidad de Guadalajara, México	We try to use astrobear to model magnetohydrodynamic fluids in geophysical environments
6/10/14	Derek Mariscal	UCSD	Plasma jet calculations
5/31/14	Patrick Adams	University of Cape Town	MHD simulation of magnetic fields in astrophysical and cosmological contexts
5/30/14	Bo Chai	Polar Research Institute of China	simulate jet in AGN
5/23/14	Ruslan Gabb	Mexico, UAEH	teaching
5/23/14	Julio Valenzuela	UCSD	2D counter-propagating plasma flows
5/23/14	Dipanjan Mukherjee	Inter-University Centre for Astronomy and Astrophysics	AMR simulations of supernova driven outflows from galactic disks.
5/13/14	Shashi Kanbur	SUNY Oswego
5/8/14	Laurence Sabin	Institute of Astronomy and Meteorology, University of Guadalajara	MHD modelling of evolved stars and comparison to observational data to understand the role played by magnetic fields (e.g. magnetic launching, Alfvén radius…etc).
5/6/14	Lee Youngjun	Chung-Ang University	Plasma Theory and Nonlinear Dynamics Lab., Chung-Ang University, Seoul, Korea. I'm researching on hydrodynamics instability, especially occurs on 'fast ignition scheme'. (more specially, inertial confinement fusion) Although AstroBEAR used on astrophysical area, I think it is suitable on our researching area, studying on Rayleigh-Taylor instability, Kelvin-Helmholtz instability, so on. In this reason, we request AstroBEAR code to improve our researching.
5/6/14	Laura Chajet	York University, Toronto	Modelling of outflows from quasar accretion disc

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