|
|
|
|||||||||||||||||
| JOURNAL HOME | HELP | CONTACT PUBLISHER | SUBSCRIBE | ARCHIVE | SEARCH | TABLE OF CONTENTS |
University of Colorado, Boulder, USA
National Center for Atmospheric Research, Boulder, USA
Australian National University, Canberra, Australia
Corresponding author: EcoBabe{at}lasp.colorado.edu
Imagine a world in which scientific data can be readily accessed by anyone seeking them. This, in a nutshell, is the premise of the Electronic Geophysical Year (eGY), one of the "international science years" commemorating the 50th anniversary of the International Geophysical Year (IGY). In the Earth and space sciences, as in other disciplines, ready and open access to the vast and growing collections of cross-disciplinary digital information is the key to understanding and responding to complex Earth and space system phenomena that influence human survival. We have a shared responsibility to create and implement strategies to realize the full potential of digital information and services for present and future generations.
Two developments have brought us to the threshold of a new revolution in our understanding of Earth and space science. First, our ability to collect data has increased dramatically, with pervasive networks of observational stations on the ground, in the oceans, in the atmosphere, and in space. This "wiring" of the planet is, in part, a legacy of the IGY, a time when a global network of observatories and the World Data Centers were established. As a result, today, petabytes of data about our planet are collected daily—data that are critical for our understanding of our planet and how it is changing.
Second, modern digital communications and information management provide an unprecedented ability to access and share information and processing capability (Figure 1). The Internet has become the "great equalizer" for communities around the world, connecting us all politically, culturally, and scientifically. For scientific data, open access to data and information from around the globe means that everyone can participate in the forward flow of scientific progress in unprecedented numbers. It means that local scientific phenomena can be placed into a global picture readily and with ease.
|
| Goals of the eGY |
|---|
|
|
|---|
The eGY provides a cooperative environment and an international mandate to help revolutionize data availability and access worldwide. Through eGY, the scientific community, as well as other interested stakeholders, can share experiences and expertise. Coordination of activities reduces replication and promotes standard sets of best practices that will ultimately lead to increases in interoperability. The eGY focuses on several areas to meet these goals, including:
The eGY also promotes the development of showcase projects and demonstrations that exemplify the best eGY practices. From geohazards to the geospace environment, from programs that support data modeling to education and outreach programs, the demonstrations being developed through the eGY year will stand as a lasting legacy.
| Virtual observatories: The future of scientific access to data |
|---|
|
|
|---|
|
The Virtual Solar Observatory (http://umbra.nascom.nasa.gov/vso/) is an example of a fully functional, highly developed virtual observatory that exemplifies many of the aspects of distributed data systems that eGY is promoting. Data from dozens of solar satellites and ground stations are available through the interface. Searchable by time interval, instrument, source, spectral range, as well as common terms used to describe data products, the Virtual Solar Observatory offers easy access to state-of-the-art solar data.
Another example of VO technology is the IRIS network for seismic activity. Seismic data are not only of interest to active scientists; they are critical input for tsunami early warning systems that are being developed. Another example is the Madrigal Virtual Observatory which provides coordinated access to world-wide incoherent scatter radar data which samples the Earth's middle and upper atmosphere (ionosphere, aurora, etc.).
As VO infrastructure is being accessed on a daily basis by very diverse user communities, it is becoming a critical and often invisible component of the technical infrastructure that must be kept in place—available, robust under load, scalable, and able to evolve as the underlying implementation technologies evolve. This question of sustainability is now one that agencies and institutions are beginning to face.
| The importance of connecting the general public from their backyard to a global picture |
|---|
|
|
|---|
Data for the nonscientist needs context and constraint. In order for data to be accessible to the general public, the virtual observatories need to provide supporting information that defines the data for the user, as well as a limited set of choices to keep the user from being overwhelmed. One telling example was brought forward recently by a middle school teacher in Colorado who was interested in showing her class the "real data" of the 11-year solar cycle. She went to a virtual observatory that most logically would have the data she was looking for and began to search. She found that she needed to know either the name of the satellite that collected the data or the specific spectral range (e.g., UV, near-IR) in order to view the data. And though she tried playing with the interface to see if she could stumble on what she was looking for, there was so much data available in so many different forms that she ultimately gave up and turned instead to Google Images to find an image that would suffice. When asked why she didn't simply start with Google, her reply was telling, namely that she saw value in presenting to her students data that "real scientists" use because it helps students connect to the idea that they, too, can be scientists.
It is important to emphasize that the limits the Colorado teacher experienced do not come from faulty virtual observatory design. Virtual observatories can only do what they are designed to do, and most are designed to service the scientific community, not the general public. And yet, it is increasingly the case that the general public wants access to these data. Many virtual observatories have heard this message and have developed solutions that allow access to their data by a broader audience. In the simplest forms, the VO will provide background material and educational material on their subject for people to use.
The USGS has long had some of the best educational resources on earthquakes in its repertoire. While it doesn't directly have anything to do with the data available at the USGS Web site, this material does arm nonspecialists with important background information that allows them to come to the data more informed. At the other end of the spectrum, some virtual observatories are building interfaces for the general user. IRIS (www.iris.edu) and the National Virtual Observatory (www.us-vo.org) each have developed interfaces that both simplifies and constrains the data for the general user.
| How to get involved with the eGY |
|---|
|
|
|---|
You also can support and promote eGY by advertising and promoting eGY nationally and internationally, displaying posters and distributing eGY literature at meetings, publishing news articles about eGY and its messages, and by joining in eGY efforts, including working groups and committees. For more information, please contact the eGY secretariat (bill.peterson@lasp.colorado.edu).
| ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
| JOURNAL HOME | HELP | CONTACT PUBLISHER | SUBSCRIBE | ARCHIVE | SEARCH | TABLE OF CONTENTS |