Award Abstract # 1036107
Enabling Breakthrough Kinetic Simulations of the Magnetosphere via Petascale Computing

NSF Org: OAC
Office of Advanced Cyberinfrastructure (OAC)
Recipient: UNIVERSITY OF CALIFORNIA, SAN DIEGO
Initial Amendment Date: November 2, 2010
Latest Amendment Date: November 2, 2010
Award Number: 1036107
Award Instrument: Standard Grant
Program Manager: Irene Qualters
OAC
 Office of Advanced Cyberinfrastructure (OAC)
CSE
 Directorate for Computer and Information Science and Engineering
Start Date: November 1, 2010
End Date: October 31, 2013 (Estimated)
Total Intended Award Amount: $39,900.00
Total Awarded Amount to Date: $39,900.00
Funds Obligated to Date: FY 2011 = $39,900.00
History of Investigator:
  • Homayoun Karimabadi (Principal Investigator)
    homa@ece.ucsd.edu
  • Kevin Quest (Co-Principal Investigator)
  • Amitava Majumdar (Co-Principal Investigator)
Recipient Sponsored Research Office: University of California-San Diego
9500 GILMAN DR
LA JOLLA
CA  US  92093-0021
(858)534-4896
Sponsor Congressional District: 50
Primary Place of Performance: University of California-San Diego
9500 GILMAN DR
LA JOLLA
CA  US  92093-0021
Primary Place of Performance
Congressional District:
50
Unique Entity Identifier (UEI): UYTTZT6G9DT1
Parent UEI:
NSF Program(s): Leadership-Class Computing
Primary Program Source: 01001112DB NSF RESEARCH & RELATED ACTIVIT
Program Reference Code(s): 7781
Program Element Code(s): 778100
Award Agency Code: 4900
Fund Agency Code: 4900
Assistance Listing Number(s): 47.070

ABSTRACT

This award facilitates scientific research using the large new computational resource named Blue Waters being developed by IBM and scheduled to be deployed at the University of Illinois in 2011. It provides travel funds to support technical coordination between the principal investigators, the Blue Waters project team and vendor technical team.

The award will aid researchers in the preparation and development of application codes which will subsequently be used to carry out the most accurate global simulations of the interaction of solar wind with the magnetosphere, far surpassing anything currently available. The accuracy and novelty of the 3D global model derives from its hybrid approach: fluid electrons coupled with kinetic ions. Results of the simulations will be available to the research community, stimulating additional research questions.

Understanding solar wind interaction with the Earth's magnetic field is central to an understanding of space weather. The term "space weather" has been coined to describe the conditions in space that affect the Earth and its technological systems. Space weather affects operations of (i) Global Positioning System satellites, (ii) geosynchronous communication and weather satellites, (iii) large-scale power distribution grids on the ground, and (iv) navigation and communications systems through the ionosphere.

PUBLICATIONS PRODUCED AS A RESULT OF THIS RESEARCH

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Karimabadi, H., J. Dorelli, V. Roytershteyn, W. Daughton, and L. Chacon "Flux pileup in collisionless magnetic reconnection: bursty interaction of large flux ropes" Phys. Rev. Lett , v.107 , 2011 , p.025002
Karimabadi, H., V. Roytershteyn, C.G. Mouikis, L.M. Kistler, W. Daughton "Flushing effect in reconnection: Effects of minority species of oxygen ions" Planetary and Space Science , v.59 , 2011 , p.526
Yi-Hsin Liu, W. Daughton, H. Karimabadi, H. Li, and V. Roytershteyn "Bifurcated Structure of the Electron Diffusion Regionin Three-Dimensional Magnetic Reconnection" Physical Review Letters , v.110 , 2013 , p.265004

PROJECT OUTCOMES REPORT

Disclaimer

This Project Outcomes Report for the General Public is displayed verbatim as submitted by the Principal Investigator (PI) for this award. Any opinions, findings, and conclusions or recommendations expressed in this Report are those of the PI and do not necessarily reflect the views of the National Science Foundation; NSF has not approved or endorsed its content.

Our research involves studies of space plasmas. Aside from its theoretical importance, this area of research has profound implications for life on Earth.  Earth and other planets in the solar system are embedded in the Sun's extended atmosphere.  There are frequent massive electromagnetic storms on the Sun that unleash tons of high energy particles that are spewed out into the solar system.  These energetic particles can wreak havoc on the Earth's electrical systems (e.g., power grids) and have already caused billions of dollars in damage to satellites.  The sience of forecasting of this so-called space weather is still in its infancy.  Space weather was identified as one of nine natural hazards posing the greatest threat to the Nation’s security in Presidential Policy Directive.  A solar storm of the magnitude of the 1859 Solar Superstorm would   cause over $2 trillion in damage today. It can cause catastrophic collapse of power grid over many states that would take months   to bring back on line.  And may satellites would be lost, resulting in no GPS, no cell phones,  and crippling communication worldwide. A severe storm would affect over 130 million people and take out 350 transformers (each takes a year to fix).
This threat is all too real.  Our society narrowly averted on 23-24 July, 2012 – by a margin of  7 days – a geomagnetic storm as large as the 1859 event that caused a catastrophic collapse of the entire power grid in Quebec & widespread blackout along east coast of U.S.  The goal of our research is to develop more accurate forecasting models. We do this through a) development of petascale global simulation codes that include much more physics than the existing global codes, and b) developing a better understanding of key physical processes in space weather.


Last Modified: 01/02/2014
Modified by: Homayoun Karimabadi