Title: ILWS and Data Services
1ILWS and Data Services
- D. G. Sibeck, Aaron Roberts
- NASA/GSFC
- Ray Walker
- UCLA
2Topics for This Discussion
- Motivation
- Why is this an ILWS topic?
- What do Researchers Need?
- Obstacles
- Solutions
- Action items
3Motivation
- Progress in space plasma physics frequently
requires the correlative study of data sets from
multiple instruments, spacecraft, simulations,
and agencies. - End-to-end analyses- the type of study fostered
by ILWS- invariably require such correlative
studies
4Why is this an ILWS Topic?
- ILWS-type research requires observations and
model output from multiple international sources. - Coordination can save time, effort, money, reveal
simple solutions. - ILWS can commission a task group to look into the
subject, get the broad view, and coordinate. - Benefits future missions/collaborations.
5What do Researchers Need?
- 1. Tools to search for and retrieve data.
- 2. Services that enable surveys and data set
comparisons (plotting and browsing). - 3. Tools that translate data formats and
transform coordinates. - 4. Tools that enable model-data comparisons
6Obstacles
- Primarily a lack of coordination
- multitude of incompatible efforts and data sets
in a wide variety of locations, data systems, and
formats - Recognition that altruism is the best policy
- Funding focused on missions, rather than
end-to-end studies - Top-down, rather than bottom-up, approach to
providing services - Can result in services that are not user
friendly, comprehensive, extendible, timely.
7Proposed Solutions
- 1. eGY
- 2. Virtual Observatories
- 3. SPASE
8 eGY is an initiative of the International Union
of Geodesy and Geophysicsled by the
International Association of Geomagnetism and
AeronomyeGY Executive Director Dan Baker
sponsored by LASP, NASA, IUGG, IAGA
9Role
- Facilitate, inform, stimulate, encourage, and
promote - Modern data access and services (e-Science for
Geoscience) - Responsible data stewardship
- Cooperation among bodies/initiatives to reduce
duplication and proliferation of standards, and
share expertise - Establishment of virtual observatories throughout
the geosciences - Establishment of criteria to determine optimal
and minimum funding for data activities
supporting research - eGY also serves to provide a link between
programs with related data and information
requirements - IPY, IHY, Planet Earth, and
initiatives such as GEOSS. - eGY will be launched July 7 Perrugia IUGG
Congress
102. Virtual Observatories
A Virtual Observatory (VO) is a service that
unites distributed data repositories and service
providers to allow users to uniformly find,
access and use resources (data, software,
documents, images and services). A VO requires
data set/tool registration, description, and
query tools
11Some National Efforts
- CDPP France Interball, DEMETER, Cluster, GEOS,
Viking.. - NGDC/SPIDR NOAA/SC, ground observations
- DARTS Japan Geotail
- NSSDC/SPDF Heliospheric, L1, magnetospheric
services - Mission level services Cluster, Yohkoh, ACE,
TIMED
12A Virtual Observatory Connects Distributed
Resources
13Early Heliophysics VOs (starting 2001)
- VSO (Virtual Solar Observatory
http//virtualsolar.org) - Delivers solar physics images, spectra, etc. as
FITS files or thumbnails covers most solar
physics products - Recently added browse movies, searching by event
lists, a shopping cart, and other features - VSPO (Virtual Space Physics Observatory
http//vspo.gsfc.nasa.gov) - Access a wide variety of space and solar physics
products, including links to other Virtual
Observatories and data from over 100
observatories/spacecraft - EGSO (European Grid of Solar Observations to
become HELIO EU/ESA) - Emphasizes catalogued events and features to
constrain searches - Was solar initially, but now expanding to all of
HP
14Newer NASA HP VxOs
- VHO (Heliosphere GSFC)
- Has a prototype that delivers some data and
allows multiple query types working on data
descriptions, and collaborating with VMO-G to
enhance middleware. - VITMO (Ionosphere, Thermosphere, Mesosphere APL)
- Existing prototype delivers data based on
parameter- and event-based searches will
incorporate a coincidence tool to aid searches. - VMO (Magnetosphere GSFC and UCLA)
- Developing many SPASE descriptions as well as
useful registry tools and middleware. - ViRBO (Radiation Belts GMU)
- Currently ingesting datasets and developing data
descriptions and a web portal planning a strong
connection to models
15Some Related Heliophysics VOs
- GAIA (Global Auroral Imaging and Access Canada)
- Integrates all-sky camera data from around the
world serves increasing amounts and variety of
ground-based HP data - VSTO (Virtual Solar-Terrestrial Observatory
NSF/NCAR) - Portal for CEDAR (ground-based) data also MLSO
(solar) broad charter. - Based on ontologies and related tools.
- STARS (Solar-Terrestrial data Analysis and
Reference System Japan) - Builds on the DARTS system currently PC
(Windows) based. - See http//hpde.gsfc.nasa.gov for more
documents, links, and details.
163. SPACE Metadata and Data Models
- Uniform access requires uniform metadata
description i.e. a data model or ontology - Metadata about the data, written in a uniform
language (e.g., SPASE) is essential - SPASE is providing the data model for NASA HP
VOs translators may be needed for
interoperability - See http//www.spase-group.org
17Ongoing Efforts
- 1. eGY -- advocating good citizenship
- 2. VxOs -- components of a comprehensive system
- 3. SPASE -- the words we need to describe data
sets and services - A good start
18ILWS Action Items
- Endorse eGY efforts (costs nothing and will
encourage these enthusiasts/advocates). - Endorse open and rapid data sharing policy
- Consider providing incentives for researchers to
share data - Commission a task group to
- Survey what is and what isnt available,
recommend solutions - Describe utility of existing services
- Identify potential partnerships and existing
resources - Communicate ongoing activities, solutions,
opportunities - Establish key links to data sets and services on
our ILWS WWW pages