AM
Amaal Mohamed
National Research Institute of Astronomy and Geophysics, NASA Goddard Space Flight Center and The Catholic University of America, The University of Sydney, Cairo University
Employment
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National Research Institute of Astronomy and Geophysics Researcher2016 - Present
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National Research Institute of Astronomy and Geophysics Research Associate2013 - Present
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NASA Goddard Space Flight Center and The Catholic University of America Research Associate2013 - 2013
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NASA Goddard Space Flight Center and The Catholic University of America Research Associate2011 - 2011
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NASA Goddard Space Flight Center and The Catholic University of America Research Assistant2008 - 2011
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National Research Institute of Astronomy and Geophysics Lecturer Assistant2007 - 2008
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The University of Sydney Ph.D. Student2005 - 2006
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National Research Institute of Astronomy and Geophysics Lecturer Assistant2000 - 2005
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National Research Institute of Astronomy and Geophysics Assistant Lecturer1994 - 2000
Education
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The University of Sydney Ph.D.2005 - 2011
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Cairo University M.Sc.1996 - 2000
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Cairo University Pre-Master1992 - 1993
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Cairo University B.Sc.1987 - 1992
Projects & Funding
Projects & funding information is unavailable.
Publications (8)
- Evaluation of seismic hazard at the northwestern part of Egypt Save
- Near-field broadband ground-motion simulation using a hybrid approach Save
- Coronal Hole Influence on the Observed Structure of Interplanetary CMEs Save
- Coronal Hole Influence on the Observed Structure of Interplanetary CMEs Save
- The relation between coronal holes and coronal mass ejections during the rise, maximum, and declining phases of Solar Cycle 23 Save
- Informational analysis of seismic sequences by applying the Fisher Information Measure and the Shannon entropy: An application to the 20042010 seismicity of Aswan area (Egypt) Save
- The relation between coronal holes and coronal mass ejections during the rise, maximum, and declining phases of Solar Cycle 23 Save
- Prediction of background levels for the Wind WAVES instrument and implications for the galactic background radiation Save