Noé Lugaz joined UNH in March 2012 and became a research faculty member with a joint appointment in the Department of Physics and at the Space Science Center of the Institute for the Study of Earth, Oceans, and Space (EOS) in 2013. Starting on 2019 October 1, I am serving as the Editor-in-Chief of the Space Weather journal. From 2019 to 2021, I am serving as the Chair of the steering committee of the Solar-Heliospheric and Interplanetary Environment (SHINE) group.  Before joining UNH, he spent 5 years at the Institute for Astronomy, University of Hawaii, where he was a post-doctoral researcher for 2 years and an Assistant Astronomer for 3 years. He graduated from the University of Michigan with a PhD in Space Science in 2007, and did his undergraduate education in France at ISAE-Supaéro in Aerospace Engineering. From October 2010 to May 2011, he was a short-term JSPS researcher at Kyoto University in Japan.



Dr. Lugaz has over fifteen years of research experience in solar-terrestrial physics, including ten years as a Principal Investigator (PI). His research focuses on the investigation of coronal mass ejections (CMEs), especially series of interacting CMEs, and their consequences. He has been studying CME propagation using numerical magneto-hydrodynamic (MHD) simulations (2004—present), remote observations with STEREO/SECCHI and LASCO (2008—present) and in-situ measurements (2012—present), CME initiation (2007—present), energetic particle acceleration by CME shocks (2013—present) and the effect of CMEs and shocks on Earth’s magnetosphere and radiation belts (2014—present). For his research, he was awarded the 2014 Arne Richter award for Outstanding Young Scientists from the European Geosciences Union (awarded to up to 5 scientists within 7 years of their PhD by the EGU).

He has published over 80 articles, including ~75 in peer-reviewed journals, has received 12 grants as PI or local PI for over 5 M$: 6 grants as PI from the National Science Foundation (NSF), 4 as PI from NASA, and 2 grants as local PI from NSF.  He has conveyed over 10 sessions at the American Geophysical Union Fall Meetings (2009—2019) and 7 sessions at the Solar, Heliospheric and Interplanetary Environment (SHINE) workshop (2010—2014, 2017). From 2013 to 2018, he served as the SHINE workshop coordinator and a member of the SHINE steering committee (250 attendees in 2016).


Selected Publications

  • Reviews

Lugaz, N., Temmer, M., Wang, Y., Farrugia, C. J., The Interaction of Successive Coronal Mass Ejections: A Review, Solar Physics,  292, 64 (2017). 

Manchester, W. B., Kilpua, E., Liu, Y. D., Lugaz, N., Riley, P., Török, T. and Vrsnak, B., The Physical Processes of CME/ICME Evolution, Space Science Reviews, doi:10.1007/s11214- 017-0394-0 (2017). 

Lugaz, N. & Roussev I. I., Numerical Modeling of Interplanetary Coronal Mass Ejections and Comparison with Heliospheric Images, Journal of Atmospheric and Solar-Terrestrial Physics (JASTP)73, 1187-1200 (2011). 

  • Simulations

Schwadron, N. A., Lee, M. A., Gorby, M., Lugaz, N., Spence, H. E. et al., Particle Acceleration at Low Coronal Compression Regions and Shocks, Astrophysical Journal, 81097 (2015).

Lugaz, N., Farrugia, C. J., Manchester, W. B., Schwadron, N. A. The Interaction of Two Coronal Mass Ejections: Influence of Relative Orientation, Astrophysical Journal77820 (2013).

Roussev, I. I., Galsgaard, K., Downs, C., Lugaz, N., Sokolov, I. V., Moise, E., Lin, J., Explaining Fast Ejections of Plasma and Exotic X-Ray Emission from the Solar Corona, Nature Physics8, 845-849 (2012).

Lugaz, N., Downs, C., Shibata, K., Roussev, I. I., Asai, A., Gombosi, T. I., Numerical Investigation of a CME from an Anemone Active Region: Reconnection and Deflection of the 2005 August 22 Eruption, Astrophysical Journal738, 127 (2011).

Lugaz, N., A. Vourlidas, I. I. Roussev, and H. Morgan, Solar-Terrestrial Simulation in the STEREO Era: The January 24-25, 2007 Eruptions, Solar Physics256, 269-284 (2009)

Lugaz, N., W. B. Manchester and T. I. Gombosi, Numerical Simulation of the Interactions of Two Coronal Mass Ejections from Sun to Earth, Astrophysical Journal634651-662 (2005).

  • Satellite Measurements

Lugaz, N., Farrugia, C. J., Winslow, R., Al-Haddad, N., Kilpua, E. K. J., Riley, P., Factors Affecting the Geo-effectiveness of Shocks and Sheaths at 1 AU, Journal of Geophysical Research121,10,861-10,879 (2016). 

Lugaz, N., Farrugia, C. J., Huang, C.-L., Winslow, R. M., Spence, H. E., Schwadron, N. A. Earth’s magnetosphere and outer radiation belt under sub-Alfvénic solar wind, Nature Communications7, 13001 (2016).

Lugaz, N., Farrugia, C. J., Smith, C. W., Paulson, K., Shocks inside CMEs: A survey of properties from 1997 to 2006, Journal of Geophysical Research120, 2409 (2015).

Winslow, R., Lugaz, N., Philpot, L., Schwadron, N. A., Farrugia, C. J., Anderson, B. J., Smith, C. W., Interplanetary coronal mass ejections from MESSENGER orbital observations at Mercury, Journal of Geophysical Research120, 6101 (2015).

  • Satellite Observations

Lugaz, N., C. J. Farrugia, J. A. Davies, et al. The Deflection of the Two Interacting CMEs of 2010 May 24 as Revealed by Combined In-situ Measurements and Heliospheric Imaging, Astrophysical Journal75968 (2012). 

Lugaz, N., Accuracy and Limitations of Fitting and Stereoscopic Methods to Determine the Direction of Coronal Mass Ejections from Heliospheric Imagers Observations, Solar Physics, 267411-429 (2010).