Документ взят из кэша поисковой машины. Адрес оригинального документа : http://hea-www.harvard.edu/~deluca/DeLuca_Resume_2012_onepage.pdf Дата изменения: Thu Jan 5 01:15:13 2012 Дата индексирования: Mon Oct 1 22:07:05 2012 Кодировка: Поисковые слова: п п п п п п п п п п п п п п п п п п п п п

EDWARD DELUCA

M S 58 60 Garden St. Cambridge, MA 02138 T 617-496-7725 F 617-496-7577 edeluca@cfa.har vard.edu

EDUCATION

Ph.D. Astrophysics, 1986, University of Colorado, Boulder, CO B.A. Astronomy, 1979, Wesleyan University, Middletown, CT

APPOINTMENT Smithsonian Astrophysical Observatory, Cambridge, MA

Senior Astrophysicist
PREVIOUS APPOINTMENTS

2012 - present

SAO, Cambridge, MA - Supervisory Astrophysicist SAO, Cambridge, MA - Astrophysicist IfA, University of Hawaii, Honolulu, HI - Astronomer Dept. of Astronomy, University of Chicago, Chicago, IL - Postdoc ASP, NCAR, Boulder, CO - Postdoctoral Hinode Science Working Group LWS Targeted Research & Technology Steering Committee Solar-C International Sub-Working Group Co-Chair for NGXT NASA Advisory Council Heliophysics Sub-Committee American Astronomical Society Solar Physics Division Chair NASA Sun-Earth Connection Roadmap Team Compton Lecturer, University of Chicago

2006 1993 1990 1987 1986 2005 2010 2009 2006 2003 2002 Sprin

-

2012 2006 1993 1990 1987 present 2011 2011 2010 2006

COMMITTEES & HONORS

g 1989

RESEARCH INTERESTS

Theory of magnetic field generation in the Sun and stars; coronal heating via magnetic reconnection and MHD turbulence; magnetic flux emergence in the Sun and stars; the nature and origin of coronal fine structure; state-of-the-art X-Ray and EUV instrumentation.

MANAGEMENT EXPERIENCE

US PI Hinode X-Ray Telescope (XRT). Hinode is a strategic solar mission in low earth orbit. It is an international collaboration between the US, Japan, UK and Norway. The XRT team includes scientists from nine different institutions in the US and Japan. Co-I, Project Scientist pre-launch, Solar Dynamics Observatory (SDO) Atmospheric Imaging Array (AIA), NASA strategic mission. SDO launched in February 2010. Responsible for developing the testing program for entrance filters, SAO representative to the science working group, helped define the fundamental science questions that would be addressed by the mission. Helped to secure the SAO archive of SDO data. Co-I, Project Scientist Interface Region Imaging Spectrograph, NASA Small Explorer. SAO has built the UV telescope feed for the spectrograph. Will help define the science goals for this mission. Will help develop the Mission Operations and Data Analysis (MODA) plans. Will organize the SAO contributions to science and operations. Co-I SAO Project Scientist, Transition Region and Coronal Explorer, NASA Small Explorer. Responsible for entrance filter testing and installation, helped define the science goals for the missions, trained and organized the telescope operators, helped lead the science working group. TRACE images are still highest resolution images ever made of the solar corona.

RESEARCH GRANTS

PI & Team Leader Living with a Start Focus Science Topic - Jets & Plumes in the Solar Atmosphere. A four year research effort starting Fall 2011. NASA HQ requested that I lead a group of five independently funded groups to study physical processes that form jets and plumes in the chromosphere and corona. (2011 - 2015) PI Non-Potential Structure of Active Regions, NASA Grant. A four year research effort has resulted in the most accurate magnetic models of active regions. (2007 - 2010) PI Influence of Coronal Abundance Variations, NASA Grant. A three year research project exploring the relationship between the variable solar coronal abundances and imaging in narrow EUV and broad X-Ray passbands. (2005 2009)