Modified from Workshop Proposal
Establishing
a Digital Library To Support Education In
Earth and
Space Science:
A Proposal
To Conduct A Community-Wide Meeting

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