|Organization||National Center for Atmospheric Research|
|Established||8 September 1940|
Location of High Altitude Observatory
The High Altitude Observatory (HAO) conducts research and provides support and facilities for the solar-terrestrial physics 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). NCAR is managed by the University Corporation for Atmospheric Research (UCAR), and receives substantial funding from the National Science Foundation (NSF).
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.
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
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 Provocation No. 214, Dr. Roberts discusses the High Altitude Observatory (HAO) 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 - Preparing for the 2017 Eclipse
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 [on the mining property of Climax Molybdenum Company at Climax, Colorado], and started the installation of the equipment.
“This branch of the Harvard College Observatory informally opened on 8 September 1940 at Climax Colorado (elevation 11,520 ft.). 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 (throughout WWII and beyond). 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 (CRPL) of the NSB funded HAO's operational costs. The headquarters of HAO was moved to Boulder in 1947.
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 Director||Dates in office|
|Walter Orr Roberts||1940 - 1960|
|John W. Firor||1961 - 1968|
|Gordon A. Newkirk||1968 - 1979|
|Robert M. MacQueen||1980 - 1986|
|Peter A. Gilman||1987 - 1989|
|Thomas E. Holtzer||1990 - 1995|
|Michael T. F. Knölker||1995 - 2009|
|Michael J. Thompson||2010 - 2014|
|Scott W. McIntosh||2014 -|