Modified from Workshop Proposal

Establishing a Digital Library To Support Education In

Earth and Space Science:

A Proposal To Conduct A Community-Wide Meeting

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1. INTRODUCTION

We propose to conduct a national meeting of key leaders and educators in Earth and Space Science. The meeting participants will be charged to develop an action plan for the establishment of a national digital library to support undergraduate education in Earth and Space Science. (In this proposal, we use the term "national digital library" to refer to both a collection of electronic materials, and the community based organization that manages the collection, develops new software tools, and provides consulting and training services to library users.) This national digital library is recognized as the central organizing tool for dissemination and coordination of curricular materials and instructional methods, and for developing interfaces with primary data needed for effective inquiry based study of the Earth System.

 

1.1 Goal for the Meeting  [back to the letter]

The goal for the proposed meeting to is develop an action plan that

  • articulates the need for a digital national library (as recommended in Shaping the Future, New Expectations for Undergraduate Education in Science, Mathematics, Engineering, and Technology, National Science Foundation, 1996 (hereafter NSF96) supporting education in Earth and Space Science,

  • states a vision for the state of this library in 2010,

  • makes recommendations regarding

  • the library`s initial scope, structure, and operating procedures, and

  • a community based consortium to operate the library.

Recommendations developed at the meeting and through subsequent community wide discussion via the World Wide Web will be documented in a meeting report. This report will be formulated as a plan of action for establishment of a national digital library supporting Earth and Space Science education and operated by an open consortium with broad community support. The establishment of such a consortium is a key recommendation of Shaping the Future of Undergraduate Earth Science Education (Ireton et al., 1996; hereafter STF); the relevant section is reproduced in Appendix 1.

Copies of the meeting report will be provided to the sponsoring agencies, meeting attendees, and professional and scientific organizations with interest in the Earth and Space Sciences, and disseminated broadly through the Earth and Space Science education community.

1.2 Motivation - Why Call Such a Meeting?[back to the letter]

Over the past eight years, the Earth and Space Science education community has identified as high priority needs: 1) instruction of a much larger generation of Earth Science teachers as required for implementation of the National Science Education Standards (National Research Council, 1996; hereafter NRC96); 2) preparation of the next generation of Earth and space scientists for success in both traditional and emerging geoscience careers; and 3) use of Earth and Space Science as a vehicle for enhanced science education for all students (Scrutiny of Undergraduate Geoscience Education, 1994; STF). It has also been recognized that satisfying these needs requires that two obstacles be overcome. First, the Earth and Space Science community overcome its traditional fragmentation -- based both on the parts of the Earth traditionally studied by different groups of people and on institutional goals, size, and student body -- and work together to foster in students the development of understanding of the whole Earth System (STF, pg. 14). Second, instructors must employ best teaching practices including building inquiry and discovery into all courses and providing experience with the processes of science (STF, pg. 25).

The proposed meeting aims to establish a "national digital library" to support the Earth and Space Science educational community. The process of establishing this library, in and of itself, will be an important step in reducing fragmentation between the various parts of this community. Furthermore, it is recognized that the emergence of the "Earth System" concept as a unifying theme in Earth and Space Science education requires new tools for teaching. Rapid dissemination of high quality instructional tools to the entire community must be a priority at this time. Finally, two of the most powerful tools for integrating inquiry, discovery, and the process of science into Earth Science courses are 1) the use of real time atmospheric, oceanographic, and seismic data (STF, pg. 27), and 2) the use of Geographic Information Systems and image analysis techniques to assimilate and explore spatial data sets (including remote sensing data). Collection and maintenance of these data sets is a community effort carried largely in support of the research enterprise. A parallel community effort is needed to provide an effective and stable interface with these data sets for educational purposes. These community needs coincide with advancements in digital communications and information science that make it is possible to establish a national digital library (National Research Council, 1988 (hereafter NRC98); National Science Foundation, 1998 (hereafter NSF98); NRC, report in progress).

Thus we believe that a community meeting to formulate an action plan for establishing a national digital library supporting education in Earth and Space Science is the appropriate next step in implementing the agenda set forth in Shaping the Future of Undergraduate Earth Science Education. This plan will provide a community vision to guide respondents to the current request for proposals on "Applications of Digital Libraries to Undergraduate Earth Systems Education" (National Science Foundation, 1999 (hereafter NSF99)) and future efforts to build national digital libraries for other disciplines.

1.3. The Challenge - Establishing A National Digital Library To Support Earth and Space Science Education

We envision the key aspect of the digital library to be access to 1) instructional materials (e.g., exercises for discovery and inquiry in large classrooms, laboratory exercises, summary papers to assist in preparation of instruction on particular topics, etc); 2) data sets and software tools to allow students to explore major aspects of the Earth System; and 3) materials and training that will assist faculty in implementing the most effective methods for instructing students.

A national digital library is the best tool for providing such access because it can 1) provide convenient, stable cross-platform access to instructional materials, 2) establish standards and foster the development by the community of software tools for accessing, manipulating, displaying, and interpreting archived and real-time data sets, 3) provide a structure for review, organization, and dissemination of instructional materials, and 4) providing training and assistance to faculty nationwide.

In establishing such a facility there are four key areas that must be addressed:

  • Collecting materials. This potentially includes materials of vastly different types, e.g., from big, fairly concentrated data sets (weather and climate data) to small, widely distributed materials such as laboratory exercises developed by individual faculty.

  • Organizing materials. This leads to questions of how the library will be structured to facilitate easy access, and includes information science issues such as indexing, annotating, reviewing, and preserving the collection. Related questions include searching across sub-collections, using standard or controlled vocabularies, and establishing appropriate standards for metadata and interoperability.

  • Evaluating materials. Faculty have repeatedly called for easy access to high-quality instructional material (STF, p. 27; UCAR, 1998). Thus we envision that the library will necessarily include a rigorous system for evaluation of materials. This will likely include not only peer review and user comments, but also a significant component based on measures of student learning. Instruments to measure the effectiveness of materials and methods will need to be developed to fully implement such and evaluation system. Evaluation data, reviews, and users' comments could be part of the metadata associated with material stored in the library. Ideally, admittance of one's work into the library will come to have the prestige of a traditional journal publication. Community involvement in designing and implementing the evaluation system is required.

  • Obtaining and Maintaining User/Community Buy-In. If the library is to become highly used and self-supporting, it is essential that it be community-owned and -maintained. The facility will have to evolve to respond to formative evaluation, as well as to meet changing community needs. Establishment of such a facility, even if much of it is distributed, will be expensive. Further, given the rate of turnover of hardware and software, routine operating costs and periodic upgrades to maintain currency will be costly. To be successful, the community must value the library sufficiently to pay for its services in some way (user fees, decreased budgets for other projects at funding agencies, etc.) Thus, a fundamental priority is establishing community ownership at the outset.

 

2. PLANNING THE MEETING AND OTHER PRE-MEETING ACTIVITIES

2.1 Organizing Committee 3. CONDUCT OF THE MEETING back to the letter

 

2.1 Organizing Committee

An organizing committee with approximately ten members will be formed to plan and conduct the meeting. This organizing committee will 1) have the broad range of technical and organizational expertise needed to design and conduct the meeting; 2) have the range of disciplinary and institutional representation needed to establish this as a community project from the beginning; and 3) be composed of individuals that can bring all the major portions of the Earth and Space Science education community to the table.

It is anticipated that the organizing committee will work closely with interested individuals from agencies such as the National Science Foundation, National Aeronautics and Space Administration, National Oceanic and Atmospheric Administration, and the United States Geological Survey.

The organizing committee will meet May 24/25 at the National Science Foundation.

The organizing committee will be charged with…

    • Ensuring that a broad range of sub-disciplines from the Earth and Space Sciences is represented at the meeting.

    • Ensuring that there are representatives from the full specturm of American higher education at the meeting (two- and four-year institutions; comprehensive national research institutions; institutions focused on serving African, Hispanic, and Native American students; etc…)

    • Selecting a meeting site.

    • Selecting a format and preparing an agenda for the meeting.

    • Preparing a formal charge to be given to the meeting participants. This will stress the need for the development of an action plan that will enjoy support from the Earth and Space Science community.

    • Preparing a series of well-posed questions that will lead the participants in the meeting to produce a coherent, comprehensive action plan enjoying broad-based "community ownership". Sample questions are given in Appendix 2.

    • Identifying an appropriate, succinct collection of "read ahead" materials to add participants in preparing for the meeting.

    • Identifying appropriate presenters for the meeting.

    • Prior to and during the meeting, leading and/or facilitating discussions, and serving as reporters.

    • After the meeting, preparing summaries of the discussions and assisting in the preparation of a final report.

    • Making extensive use of the World Wide Web both before and after the meeting to keep participants and the broader community advised of plans and progress, and to solicit community input.

2.2 Selecting Participants

The organizing committee will invite ~40 individuals to be participants in the meeting. This will give a total meeting attendance of ~50 individuals. The organizing committee will insure that the ~40 participants include 1) key Earth and Space Science educators, 2) Earth and Space Science community leaders (from the director, dean, and university vice-presidential level), and 3) individuals knowledge in the technical aspects of digital libraries.

2.3 Meeting Site on the World Wide Web

Immediately following the May meeting of the organizing committee, a web site devoted to the August meeting will be established on the World Wide Web. It will announce the meeting, indicating its purpose and goals, and display the questions to be addressed. Community comment will be solicited by advertising the site through such list servers as geo-ed@arbuckle.geo.utulsa.edu, the Keck Consortium list server, the PKAL Earth and Planetary Science server, and the NASA/USRA Earth System Science Education server.

 

3. CONDUCT OF THE MEETING[back to the letter]

The meeting will be conducted Monday/Tuesday, 9/10 May 1999, with the participants traveling the day before (Sunday) and the day after the meeting (Wednesday). The meeting will take place at Coolfont, WV.

As was the case with the highly successful Spheres of Influence meeting that produced the STF report, this is to be a "working meeting", with only a limited number of formal presentations. The majority of the meeting time devoted to discussion and writing by participants. The organizing committee will decide the format of the meeting. Devices such as discussions and writing in small groups, plenaries with group reports and open discussion, poster sessions with "post-it" comments, and emissaries between groups will be used to insure that consensus is developed on a plan of action for establishing and maintaining the library.

To prepare for the meeting, list-servers will be established. The organizing committee will foster electronic discussion of the meeting goals and the questions to be addressed. Electronic discussions in advance of the Spheres of Influence meeting allowed participants to introduce themselves, clarify their assignments, share initial ideas, and in one case, to produce a draft document that served as a basis for discussion at the meeting.

A possible agenda for the meeting is as follows:

Day 1 - Travel day

Welcoming Reception

Day 2 - 1st Meeting Day

Opening Plenary

Charge to the Participants

Responding to the "charge" -- process to formulate and reach a consensus on recommendations

Presenter 1: Earth System Science and Global Change Education- a review of our priorities

Presenter 2: Digital Libraries - what are they and why are they important?

Presenter 3: Demonstration of a digital library and its use as an educational tool.

Hands-on experience - exploring representative digital libraries (12-seat high-end computer laboratory available on a round-robin basis)

Lunch

Work sessions in small groups

 

Day 3 - 2nd Meeting Day

Plenary

Small group reports on progress

Reframing questions/redirecting efforts (as necessary)

Work sessions in small groups

Lunch

Closing plenary

Final reports from small groups

Reaching consensus

Closing Reception

Day 4 - Travel Day

4. FOLLOW-ON ACTIVITIES[back to the letter]

4.1 "First Impressions" Report

A "first impressions" report summarizing the main points of the plan of action devised at the meeting will be available to the funding agencies by 1 September.

4.2 Meeting Report

Dr. Cathy Manduca, Dr. David Mogk and Dr. John Snow will prepare the meeting report. They will compile and edit material produced by the working groups and add introductory and concluding material as needed. They will be charged with extracting the vision, conclusions, and recommendations from the workshop.

4.3 Posting A Draft Report to the World Wide Web

In mid September, a draft of the meeting report will be posted to the World Wide Web for community review and comment. The opportunity to review and comment on the report will be advertised widely via e-mail list servers such as geo-ed@arbuckle.geo.utulsa.edu (which reaches over 200 Earth and Space Science educators). Comments will be received for a 60-day period (cutoff at the end of July).

Comments for the community will be considered in preparing the final draft of the report.

4.4 Report Review

The authors will have a final draft report prepared by mid January. This will be provided to all meeting participants for final review and comment (cutoff mid February).

6.0 REFERENCES

American Geophysical Union, Scrutiny of Undergraduate Geoscience Education - Is the viability of the Geoscience in Jeopardy. Proceedings of the Chapman Conference. American Geophysical Union, Washington, D.C., 1994.

Ireton, M.F.W., Manduca, C.A., and Mogk, D.W. eds, Shaping the Future of Undergraduate Earth Science Education-Innovation and Change Using an Earth System Approach, American Geophysical Union, Washington, D.C., 1997.

National Research Council (NRC), Distributed Geolibraries: Spatial Information Resources, work in progress.

National Research Council (NRC98), Developing a Digital National Library for Undergraduate Science, Mathematics, Engineering, and Technology Education, National Academy Press, Washington, D.C., 1998.

National Research Council (NRC96): National Science Education Standards, National Academy Press, Washington, D.C., 1996.

National Science Foundation (NSF99), Geoscience Education Program Announcement, NSF 99-44, Arlington, VA, 1999.

National Science Foundation (NSF98), Information Technology: Its Impact on Undergraduate Education in Science, Mathematics, Engineering, and Technology, NSF 98-82, Arlington, VA, 1998.

National Science Foundation (NSF96), Shaping the Future: New Expectations for Undergraduate Education in Science, Mathematics, Engineering, and Technology, NSF 96-139, Arlington, VA, 1996.

University Corporation for Atmospheric Research (UCAR): Program for the Advancement of Geoscience Education (PAGE) Community Planning Workshop Interim Report, http://www.page.ucar.edu/pub/map.htm, 1998

 

Appendix 1[back to the letter]

Recommendation from Panel 7

In

Shaping The Future (Ireton et al., 1996; hereafter STF)

To All Stakeholders With Interests in Undergraduate Earth System Science Education

  1. Speak with a common voice to affirm and promote NSES and Earth system science.

  2. Publicize and promote implementation of the NSES and Earth system science at the K-12 level, on college campuses, to society memberships, to the general science community, to informal educators, and to the public at large through publications, workshops, and public presentations.

  3. Develop a coherent, sustainable, and open consortium, linking the educational missions of K-12, undergraduate, graduate, and informal science communities. All participants in the consortium should share in and reinforce common efforts in faculty development, curriculum development, and dissemination. (Joint recommendation with Panel 5).

The consortium would have the following characteristics in form and function:

Provide leadership and a common voice for the Earth and space sciences community:

a. governance would be directed by the member institutions;

b. a permanent staff who would be employed with expertise in science, science education, curriculum development, and instructional and other related technologies, as well as materials dissemination and software support; and

c. one- to two-year rotating positions would be provided for the scientific community to participate.

The benefits of the central organization include:

a. better coordination and less redundancy in the development of curricular materials;

b. development of standardized software and other technology tools for accessing
research data;

c. more efficient dissemination of instructional materials; and

d. opportunities for a broader integration of disciplines in Earth and space system science.

Appendix 2

Sample Questions To Be Addressed

 

Typical community concerns to be addressed include…

What is the scope of the library -what types of material go into it?

How will the materials be reviewed?

What evaluation materials are required for acceptance?

 

Who are the intended primary users (e.g. researchers? faculty, students? teachers?)

How would the users like the materials organized and indexed? (I.e., what are the key things users want to be able to sort out at a first or second pass?)

How will users get access?

How will the system be managed (e.g. who decides if we want to change something)?

How will the community provide input during the development of the library?

How will the community pay for the library in the long haul?

How will this advance the Earth and Space Science educational agenda?

Why is this is an important thing to do?

 

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