HelioWebStanford University, Department of Astronomy
flowchart
I[Stanford University, Department of Astronomy]
PI["Parent Institutions (1)"]
CI["Child Institutions (0)"]
AW["Affiliated Works (21)"]
CA["Linked Collaborating Authors (3)"]
I== skos:broader ==>PI
CI== skos:broader ==>I
AW== affil ==>I
AW== author ==>CA
click PI "#parent-institutions"
click CI "#child-institutions"
click AW "#affiliated-works"
click CA "#collaborating-authors"
Parent Institutions [?]
Child Institutions [?]
Affiliated Works
sorted by decreasing year, and then by display-name
- The Right Amount of Glue: Technologies and Standards Relevant to a Future Solar-Terrestrial Data Environment
- Data Integration in the Virtual Solar Observatory
- The Virtual Solar Observatory -- the Why, What, How and Where
- Keck Near-Infrared Observations of Saturn's E and G Rings during Earth's Ring Plane Crossing in August 1995
- STEREO in the Virtual Solar Observatory Context
- Enchancements to the Virtual Solar Observatory
- Evidence for Likely Liquid Hydrocarbons on Titan's Surface from Cassini Radio Science Bistatic Scattering Observations
- The Virtual Solar Observatory and the Heliophysics Meta-Virtual Observatory
- The current and future roles of virtual observatories serving the heliophysical data environment
- Callable Virtual Observatory Functionality: Sample Use Cases
- Dealing with Large Dataset Queries in the Virtual Solar Observatory
- Design Considerations for Data Catalogs
- Encouraging Summer Students in Science by Involving them with EPO: Case Studies
- Magnetic Reconnection Site Suggested by a Double Coronal X-ray Source Observed by RHESSI
- Cross-helicity turbulence model: Application to MHD phenomena from solar convection zone to heliosphere
- The Solar Dynamics Observatory Education and Public Outreach Program: The First Years
- Evidence from Helioradiology of an Inner Tachocline in the Sun
- Far-side seismic maps with HMI
- SDO Citizen Scientists; The Camilla Space Weather Project
- The Rising Phase of Solar Cycle 24: General Solar Wind, Large-Scale Solar Wind Structures, and Sector Asymmetry
- What NASA Does Best - Providing Effective Experiences in Authentic Science: The IRIS Mission EPO Program