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FASR ScienceFASR Science• Nature & Evolution of Coronal Magnetic Fields Measurement of coronal magnetic fields
Temporal & spatial evolution of fieldsRole of electric currents in corona
• Coronal Mass EjectionsBirth; Acceleration
B, T, nnt, nth
Prominence eruptions
• FlaresEnergy releasePlasma heatingElectron acceleration and transport
• Nature & Evolution of Coronal Magnetic Fields Measurement of coronal magnetic fields
Temporal & spatial evolution of fieldsRole of electric currents in corona
• Coronal Mass EjectionsBirth; Acceleration
B, T, nnt, nth
Prominence eruptions
• FlaresEnergy releasePlasma heatingElectron acceleration and transport
FASR SpecificationsFASR SpecificationsFrequency range ~0.1 – 30 GHz
Frequency resolution 1%, 0.1 – 3 GHz3%, 3 – 30 GHz
Time resolution <0.01 s, 0.1 – 3 GHz<0.1 s, 3 – 30 GHz
Number antennas ~100 (5000 baselines)
Size antennas D = 2 – 6 m
Polarization 0.1 - 3 GHz, full3 – 30 GHz, dual
Angular resolution 20/n9 arcsec
Field of View 19/(Dn9) deg
Timeline For FASRTimeline For FASR2002-3: Design Study (NSF/ATI)• International Science Definition Workshop (May 23-
25, 2002)
• Configuration; Software architecture; Site Surveys
• Design options; Costing (Current estimate $30 M)
2004-5: Design and Development• Prototype Major Elements
• Prototype Array (< 10 elements)
• Refine Hardware and Software Design
2005-8: Construction
2002-3: Design Study (NSF/ATI)• International Science Definition Workshop (May 23-
25, 2002)
• Configuration; Software architecture; Site Surveys
• Design options; Costing (Current estimate $30 M)
2004-5: Design and Development• Prototype Major Elements
• Prototype Array (< 10 elements)
• Refine Hardware and Software Design
2005-8: Construction
Principal Institutions and People
Principal Institutions and People
NJIT D. E. Gary, P. Goode, J. Lee
NRAO T. S. Bastian, J. Webber
UMd S. M. White, A. Harris
Berkeley G. J. Hurford
Lucent L. J. Lanzerotti
NSO C. Keller
<your institution><your name here>
NJIT D. E. Gary, P. Goode, J. Lee
NRAO T. S. Bastian, J. Webber
UMd S. M. White, A. Harris
Berkeley G. J. Hurford
Lucent L. J. Lanzerotti
NSO C. Keller
<your institution><your name here>