High Altitude Observatory


The High Altitude Observatory conducts research and provides support and facilities for the solar-terrestrial research community in the areas of solar and heliospheric physics, and the effects of solar variability on the Earth's magnetosphere, ionosphere, and upper atmosphere.
HAO is a laboratory of the National Center for Atmospheric Research. NCAR is managed by the University Corporation for Atmospheric Research, and receives substantial funding from the National Science Foundation.

Mission and vision

HAO's mission is to understand the behavior of the Sun and its impact on the Earth, to support, enhance, and extend the capabilities of the university community and the broader scientific community, nationally and internationally, and to foster the transfer of knowledge and technology. As articulated in its Strategic Plan for 2011-2015, HAO's vision is to: Perform world-leading science to understand fundamentally and with predictive capability the sources and nature of solar and geospace variability; Provide scientific leadership and facilities to serve the wider community in common pursuit of these science objectives, and both support and benefit from the NCAR community; Support the education and training of early-career researchers in solar-terrestrial physics and instrumentation; and Provide advocacy for solar-terrestrial physics, promoting its results, and articulating its societal importance, to the rest of NCAR, the NSF, the university community, and the public.
HAO's telescopes are located at its Mauna Loa Solar Observatory, near the summit of that volcano on the big island of Hawaii. NCAR's solar observatory shares space on the campus of NOAA's larger Mauna Loa Observatory. HAO's researchers are based at NCAR headquarters, in Boulder, Colorado.

Eclipse expeditions

1952 - Khartoum, Sudan
This was a joint HAO – Naval Research Laboratory expedition, which obtained 50 spectra of the eclipse features of the sun.
1958 – Pukapuka, Cook Islands in the Pacific
This was a joint HAO – Sacramento Peak expedition that was unable to obtain a single photo due to rainstorms.
1959 – Fuertaventura, Canary Islands of Spain
A joint HAO – Sacramento Peak expedition
1962 – Lae, New Guinea
1963 – Alaska and Canada
1965 – Bellingshausen Island, South Pacific
1966 – Pulacayo, Bolivia
1970 - San Carlos Youtepec, Mexico
File:Eclipse_in_1970,_Mexico_.jpg|thumb|This photograph of the sun's outer atmosphere, or corona, was taken by a research team from the National Center for Atmospheric Research's High Altitude Observatory during . It was taken at an altitude of 8,800 feet on a remote mountain site in southern Mexico with a special camera designed by Gordon Newkirk of NCAR.
1972 – Cap Chat, Canada
1973 – Loiengalani, Kenya
1980 – Palem, India
HAO in collaboration with Southwestern at Memphis College, Tennessee
1981 – Tarma, Siberia, USSR
HAO in collaboration with the Astronomical Council of the Academy of Sciences of the USSR, Moscow
1983 – Tanjung Kodok, Indonesia
1988 - Mindanao, Philippines
In , Dr. Roberts discusses the High Altitude Observatory expedition to the Philippines to observe the eclipse of March 18. HAO expedition staff included Dick Fisher, Kristy Rock, Mike McGrath, and Lee Lacey.
1991 - Mauna Loa, Hawaii
HAO in collaboration with Rhodes College, Tennessee
1994 - Putre, Chile
1998 – Curaçao, Dutch Antilles
2012 – Palm Cove, Queensland, Australia
2017 -

History

Walter Orr Roberts was a graduate student under Donald Menzel at Harvard, and helped him set up a solar telescope at the Oak Ridge Station of Harvard College Observatory. In 1939, Menzel located a site for a western station in the Colorado mountains. In his unpublished memoirs, Menzel writes: “I returned the following summer, supervised the building of the observatory and an observer’s residence , and started the installation of the equipment.
“This branch of the Harvard College Observatory informally opened on 8 September 1940 at Climax Colorado. Its sole purpose was to study the sun, using the first coronagraph in the western hemisphere.”
Walter Roberts and his wife arrived in the summer of 1940, and remained at the observatory for 7 years. Menzel continues: “In the summer of 1940, however, Walter and I quickly solved the problems of our coronagraph. After I left, he soon had it working properly. He obtained daily records of the spectrum of the corona, which furnished us with a valuable index of solar activity.
At Climax, Walter Roberts quickly proved observationally what most astronomers had previously suspected, that the corona itself rotated with the same period as the solar surface, in something over twenty-five days. He initiated a study of the fine structure of the solar atmosphere, determining the behavior of what he called “spicules,” a phenomenon that I had myself briefly discussed while at Lick Observatory. These studies formed the basis for his doctorate thesis submitted for the degree a year or two later.”
Work at the observatory was classified during WWII because of its value in predicting radio disturbances from the study of the corona. "The wartime work of the observatory was done under the auspices of the Navy, although overall direction remained in the hands of Harvard.” Post WWII, The National Bureau of Standards contracted the observatory for reports on solar activity. In 1946, CU Boulder became a joint sponsor with Harvard of the observatory, while the Central Radio Propagation Laboratory of the NSB funded HAO's operational costs. The headquarters of HAO was moved to Boulder in 1947.

Directors

The founding Director of the High Altitude Observatory was Walter Orr Roberts. The current Director is Scott McIntosh.
A list of all HAO directors since the founding of the Observatory is given below.
HAO DirectorDates in office
Walter Orr Roberts1940 - 1960
John W. Firor1961 - 1968
Gordon A. Newkirk1968 - 1979
Robert M. MacQueen1980 - 1986
Peter A. Gilman1987 - 1989
Thomas E. Holtzer1990 - 1995
Michael T. F. Knölker1995 - 2009
Michael J. Thompson2010 - 2014
Scott W. McIntosh2014 -