Astronomy Activities

Many Internet2 member institutions are developing and using high performance networking applications for optical astronomy, radio astronomy, remote instrumentation, data sharing, and other collaborative activities. Click here for information on activities in VLBI and radio astronomy.

Activities

The Gemini Observatory

With funding and support from the National Science Foundation (NSF), the Gemini Observatory established a new Internet pathway in August 2002, which will provide its twin telescopes with the data transfer capabilities required to handle the enormous amounts of scientific information created by Gemini's sophisticated instrumentation. This new link between Gemini's twin, 8-meter telescopes located on Mauna Kea, Hawaii, and on Cerro Pachón in the Chilean Andes was made possible with the support and technology of Internet2 and AMPATH, a Florida International University international Internet exchange point to research institutions in South America. Under development for almost five years, this link allows Gemini to move forward towards its goal of becoming the world's first "cyber observatory." According to Peter Michaud, Public Information and Outreach Manager for the Gemini Observatory, "A virtual ribbon cutting on August 13, 2002 officially inaugurated the new link between the twin observatories. This link will allow astronomers to access skies in both the northern and southern hemispheres without having to travel to Hawaii or Chile."

SARA Observatory

Astronomers at a six different universities in the southeastern U.S. are able to take advantage of the clear desert skies in Arizona to perform their celestial research without having to leave their campuses. Members of the Southeastern Association for Research in Astronomy (SARA) consortium use Internet2 high-performance networks to remotely control the 0.9-meter Ritchy-Critchen reflecting telescope at Kitt Peak Observatory, located southwest of Tucson, AZ at 6,800 feet above sea level. According to Dr. James Webb, Director of the SARA Observatory, “In order to perform remote observing in real-time and get quality data, network speed, reliability, and bandwidth are critical.” Webb, who recently gave a presentation on remote observing at the Internet2 Joint Techs Workshop, added “Before Internet2, network latency and dropouts severely impacted observing. With Internet2, latency is small enough and dropouts rare enough to have essentially no impact on observing.” A typical remote observing session starts with a check on the weather in Tucson. The astronomer then logs on to the telescope control computer using Virtual Network Computing (VNC is a platform independent, client-based system written by AT&T Laboratories), creates directories to hold the images, opens the dome on the telescope, observes, closes the dome on the telescope, and log off VNC. The actual images from the observing session are simply transferred back to any home or office computer using FTP. Webb summarized the benefits of remote observing, “It allows us to save travel money, keep our on-campus teaching commitments, and still collect scientific data from the best possible sites.”

Aricebo Observatory

As one of the premier facilities for radio/radar astronomy and atmospheric science, the Aricebo Observatory in Puerto Rico is a key component of several large-scale research programs involving multiple instruments around the globe and in space. The 305m telescope's unique sensitivity is needed for quick confirmation of new discoveries within its space and frequency coverage, precise tracking and imaging of small solar system objects which may be visible for only a few days, and measurement of ionospheric effects barely detectable elsewhere. The design of the instrument is shaped by multidisciplinary needs and enables it to respond quickly and flexibly to "targets of opportunity". A remote observing capability is useful for flexible telescope scheduling, as well as for coordinated observing projects with multiple spaced instruments, which are common in atmospheric investigations. Plans call for development of a "Virtual Control Room" permitting remote observers to perform high-quality observations over Internet2 without travelling to the site.Given the large data-gathering capability of the Arecibo telescope, special techniques are often required to perform realtime signal processing and parameter estimation on the acquired data. Certain investigations e.g pulsar searches require supercomputer-class computing resources to implement sophisticated reduction algorithms. Good use of the available observing time often implies getting data reduced before the next available slot, i.e high-bandwidth access to a supercomputer. Here the role of the Observatory is that of a source of raw data with a participating supercomputer center supplying the computational resources.

Astronomy BOF

The Internet2 Astronomy Birds of a Feather (BOF) group brings together individuals from the field of astronomy to share knowledge of astronomy, remote instrumentation, data sharing, and other activities.

Archives

Presentations from the Astronomy BOF meeting, held in conjunction with the Joint Techs meeting in Honolulu, HI, 28 January 2004.

Presentations from the Astronomy BOF meeting, held at the Ampath Workshop, 29-31 January 2003.

Contact Info
Russ Hobby
Manager of the Science & Engineering Initiative
rdhobby@internet2.edu

 

 

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