1 / 24

QuarkNet 101

QuarkNet 101. Kris Whelan University of Washington. Current Status. Outline Overview Basic Structure Evolution since 1999 Personnel/Responsibilities. Program Context. Reform -based teaching and learning - national standards Scientists as partners in education reform

roden
Download Presentation

QuarkNet 101

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. QuarkNet 101 Kris Whelan University of Washington

  2. Current Status • Outline • Overview • Basic Structure • Evolution since 1999 • Personnel/Responsibilities

  3. Program Context • Reform-based teaching and learning - national standards • Scientists as partners in education reform • Nature of particle physics research • Long-term • Distributed • Best practice professional development • Research appointments • Research-based workshops • Follow-on program

  4. Vision & Goals Building relationships that develop & support a research community of physicists, high school teachers & their students Goal: Engage teachers & their students with scientific investigations. Goal: Confront particle physicists with current issues in science education.

  5. Vision & Goals • Engagement with Scientific Investigations • Enable teachers to teach basic physics concepts in an exciting & rewarding context. • Build a teacher’s confidence to bring current science into the classroom. • Link high school classrooms with frontier experiments. • Attract students to careers in science & technology. • Help develop science literacy.

  6. 5.6 Staff Members 4 PIs Center 60 Typical Center Center 2 Center 1 Center 58 Center 3 Center 59 2 Mentors 2 Lead Teachers 10 Associate Teachers Program Structure Outside Evaluators Advisory Group ProgramSupport Staff Teachers Fellows ---- -----

  7. By the Numbers 537 Teachers & Their Students 97 Mentors 53 Centers 9-11 Experiments 5.6 Staff Members 4 PIs DOE-NSF

  8. Center Profiles Participants • Physicists as mentors & colleagues • Teachers as researchers & facilitators in classrooms • Teachers as professionals • Students as researchers

  9. Physicists as Mentors & Colleagues • Commit for the long term. • Host teachers & students; visit classrooms. • Year I • Participate in orientation. • Recruit 2 lead teachers. • Supervise 7-week research appointments. • Co-plan 3-week research-based institute.

  10. Physicists as Mentors & Colleagues • Year II • Co-recruit 8 associate teachers. • Co-conduct 3-week institute. • Following Years • Co-host 1-week follow-on program. • Involve NSF-funded HS students in summer research.

  11. Mentors Are: • Volunteers • Affiliated with particle particle experiments in the U.S. & overseas • Experimentalists AND Theorists • Entire SMU mentor team is theorists. • Theorists - an integral part of many QuarkNet centers.

  12. Teachers as Researchers • Construct & test detector components. • Analyze data & conduct simulation studies. • Create data sets for their students. • Create scientific investigations for their students. • Build classroom detectors.

  13. Teachers as Professionals • Assume Leadership Roles with Teaching Colleagues • Participate in the Fellows Program: • e-Lab, leadership, LHC, teaching & learning • Develop/Test instructional materials. • Develop/Lead PD activities. • Share/work with colleagues in their schools, districts, centers’ regions, nationally, internationally.

  14. Students as Researchers • Learn fundamental physics by: • Analyzing real data delivered online. • Collaborating with students worldwide. • Participating in inquiry-oriented investigations. • Experimenting using classroom cosmic ray detectors. • Visiting research groups & experiments.

  15. Program Activities • Activities for Participants Teachers Students • Boot Camp at Fermilab - Access to e-Labs • Research appointments -Research appointments • Follow-on activities -Masterclass • Fellows Program • Workshops • Online presence: Web/Web 2.0 (including access to I2U2 e-Labs)

  16. Program Activities • National Project Management • Managing funds • Preparing reports for funding agencies • Collecting data as requested by the outside evaluator • Providing assistance for planning & implementing effective center activities • Creating resources & tools, maintaining the Web presence, & supporting teachers using resources • Supporting QuarkNet fellows • Organizing workshops & special events • Participating in dissemination & broader impact activities

  17. Broader Impacts Examples of Dissemination Activities Cosmic Ray Studies—National & International: Auger, IceCube, + 32 non-QuarkNet institutions IPPOG: QuarkNet program, cosmic ray studies, discovery science and more Masterclasses: CMS international program, astrophysics masterclass Influence on Other Programs: CHEPREO, CMS, COSM, CROP, I2U2, IB, ICAM, ILC, LIGO, MARIACHI, NDeRC, OSG, PARTICLE, SUL, WALTA

  18. Center Program • Staff provides guidance, support, resources for: • Year I - 2 mentors & 2 teachers • Mentors • Orientation Lead Teachers • 1-week orientation workshop (Boot Camp) • 7-week research appointment • Academic year follow-on

  19. Center Program • Staff provides guidance, support, resources for: • Year II - 2 mentors, 2 lead teachers & 8 associate teachers • 3-week research-based institute • Following years - 2 mentors & 10 teachers • 1-week follow-on program • NSF student research program - 1 teacher & 4 students • Additional opportunities for teachers • 1-week Particle Physics Boot Camp • Special Events

  20. Program Evolution • QuarkNet is a dynamic program, responding to formative evaluation data & adjusting to address: • Participants’ needs & interests. • Center strengths. • . . . within available funds.

  21. Program Evolution • Examples of “New” Program Activities • 2001 Cosmic ray detectors • 2001 Run II Discovery • 2004 Student summer research • 2005 Cosmic Ray e-Lab • 2006 Boot Camp model of professional development • 2006 Masterclass • 2008 Fellows • 2008 Instructional design (UbD) • 2010 CMS e-Lab

  22. Program Benefits • A Strong Program Benefits Teachers & Students. • Members of a research community • Working on a team • Sharing ideas • Doing science • Solving problems

  23. Program Benefits • A Strong Program Benefits Teachers & Students. • Members of a learning community • Supporting one another and sharing ideas • Using scientific research in the classroom • Using instructional resources that support student explorations of science • Using particle physics examples in basic physics

  24. Questions? For more information about QuarkNet: Website: quarknet.fnal.gov Kris Whelan kkwhelan@uw.edu

More Related