Track and maintain observing requirements driven by the Science Objectives. Organize and lead the PUNCH Science Team and interface between the Science Team and the PI. Karen Harvey Prize, for outstanding early career contributions PUNCH Role NRC Postdoctoral Fellow, NASA GSFC,1996-1998 Awards NSF-NATO Postdoctoral Fellow, University of Cambridge, 1999-2000 Research Assistant Professor The Catholic University of America, 1998-1999 2000-2001 in Physics, Stanford University, 1989 Professional Background in Astrophysics, University of Colorado-Boulder, 1993ī.S. in Astrophysics, University of Colorado-Boulder, 1995 2001: Polar Plume Lifetime and Coronal Hole Expansion, APJ 560, 490 2001: Observation of Polar Plumes at High … Altitudes, APJ 546, 569ĭeForest, C.E. 2011: Detailed Structure in the Solar Wind. 2012: Inner Heliospheric Flux Rope Evolution via Imaging of Coronal Mass Ejections, APJ 746, 64ĭeForest, C.E. 2012: Disconnecting Solar Magnetic Flux, APJ 745, 36 III: Tracking Features in 3D, APJ 765, 45ĭeForest, C.E. Howard, T.A., Tappin, S.J., Odstrcil, D., & DeForest, C.E. 2013: Tracking Features from the Low Corona to Earth, APJ 769, 43 2014: Inbound waves … Alfvén surface location, APJ 787, 124ĭeForest, C.E. 2015: Feasibility of Heliospheric Imaging from Near Earth, APJ 804, 126ĭeForest, C.E. 2015: Turbulence…Solar Wind.Comet Tail Test Particles, APJ 812, 108ĭeForest, C.E. 2016: The utility of polarized heliospheric imaging for space weather monitoring, Sp. 2016: Fading coronal structure and the…young solar wind, APJ 828, 66ĭeForest, C.E. 2017: 3D Polarized Imaging of CMEs: Chirality of a CME, APJ 850, 130ĭeForest, C.E. 2018: The Highly Structured Outer Solar Corona, APJ 862, 18ĭeForest, C.E. Selected Publications Relevant to PUNCHĭeForest, C.E. Of CME chirality, via 3D polarized imaging (2018) discovery of very highly structured fine detail in the outer solar corona usingĭeep-field campaign data from STEREO/COR2. Outer solar corona using 2-D velocity filtration (2015) measurement of solar wind turbulence via comet tail tracking (2016)ĭetection of the breakup of coronal structure and transition to solar wind flow, 0.2 AU from the Sun (2017) remote measurement Single CME, and demonstration of the solar origin of CME plasma at Earth (2014) sensitive detection of inbound features in the LASCO field of view (2009) demonstration that the EUV corona is more spatially variable than previously thought (2011) firstīackground-subtracted heliospheric images useful for feature photometry (2012) first complete tracking from Sun to Earth of a Include: (1997) first detection of traveling waves in the solar corona (2001) imaging of faint polar plumes to the limits of the He developed the analysis tools that enabled theĬurrent era of photometric heliospheric imaging, and has exploited them with a series of groundbreaking papers. Fromġ999-2016, was Press Officer for the AAS/SPD, after which he stepped down to lead PUNCH.ĭeForest is well known for his expertise in solar data analysis and reduction. Ground-based demonstration heliospheric imaging observatory), and SSIPP (a balloon-borne miniature solar observatory). He led several ground and suborbital instrument development efforts including SHAZAM (a novel high-speed magnetograph), DASH (a He was Resident Observer (at NASA/GSFC) for the Michelson Doppler Imager experiment on the SOHO mission from 1995-1999 ĭuring this time he explored dynamics of the corona and the limits of solar observing in the faint outer corona. (1989-1995) centered on the Multi-Spectral Solar telescope Array, a sounding rocket that helped pioneer EUV imaging of the solarĬorona. His graduate studies at Stanford University He holds an adjunct professorship at theĭeForest has studied the Sun, its corona, and the solar wind for over 30 years. Professional Background and Supporting ExperienceĬraig DeForest is Southwest Research Institute’s Program Director for solar astrophysics, and the Vice-Chair of theĪmerican Astronomical Society’s Solar Physics Division (AAS/SPD). Success in all aspects of the PUNCH mission. Leads the PUNCH team and is responsible for ensuring programmatic, technical, and scientific in Physics, Reed College, 1989 PUNCH Role in Applied Physics, Stanford University, 1996ī.A.
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