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1973 Concorde eclipse flight

On 30 June 1973, the supersonic jet Concorde 001 intercepted the path of a total solar eclipse and followed the path of totality as it crossed Africa. This feat allowed the passengers to experience a total solar eclipse for 74 minutes, the longest-ever total eclipse observation. Five experiments were carried out during the flight, but they have had limited scientific impact.

Sequence of events
Preparation and lead up In May 1972, Pierre Léna, an astronomer with the Paris Observatory, met with French Concorde test pilot André Turcat over lunch at a restaurant at Toulouse Airport to propose his idea to view the 1973 eclipse from an aircraft. Aboard the flight were Turcat and Dabo; flight mechanic Michel Rétif; radio navigator Hubert Guyonnet; Henri Perrier; and astronomers Léna, Beckman, Donald Hall, Donald Liebenberg, Alain Soufflot, Paul Wraight, and Serge Koutchmy. The plane intercepted the path of totality over Mauritania within one second of the planned rendezvous Mauritania closed its airspace to commercial air traffic to ensure the success of the Concorde's flight. The aircraft flew in the lunar shadow over the Sahara including Mali, Nigeria and Niger, before landing in Fort-Lamy (present-day N'Djamena), in Chad. On the ground on Earth, the longest possible viewing of totality of this eclipse from a fixed location was 7 minutes and 4 seconds. The Concorde experienced 74 minutes of totality with an extended second contact of 7 minutes and extended third contact of 12 minutes. == Aircraft ==
Aircraft
The original Concorde prototype 001 made its first test flight in 1969 from Toulouse Airport. The specific modified version of the aircraft used for this experiment was Concorde 001, registered as F-WTSS. The aircraft has four twin-spool Olympus 593 engines and two onboard inertial guidance systems. Four specially-made portholes were installed in the roof of the aircraft's fuselage to facilitate viewing of the Sun. Infrared and optical cameras were installed in portholes in the plane's roof to capture the Sun's corona with less atmospheric interference than there would be from the ground. F-WTSS is now on display as an exhibit at the Musée de l’air et de l’espace in France along with Air France Concorde 213, registered as F-BTSD. == Scientific observations ==
Scientific observations
Five experiments were carried out during the 1973 Concorde 001 flight. Léna and his team (from one of the Paris universities) focused their efforts on studying the F-corona (the outer part of the Sun's corona, made up of dust particles). Wraight (University of Aberdeen) measured the effects of the eclipse on oxygen atoms in the Earth's atmosphere through a side-porthole. Liebenberg (University of California, Los Alamos Scientific Laboratories) measured pulsations in light intensity, while Beckman (Queen Mary College) observed the far infrared emissions from the chromosphere. == Legacy ==
Legacy
Though this event garnered wide and lasting media attention, solar researchers generally agree that the Concorde's flight has had limited scientific impact. Kevin Reardon of the National Solar Observatory said of the flight, "Strangely no significant results were ever published from the effort. [...] The overall science output was not as notable as the flight itself." Léna himself has admitted, "The five experiments all succeeded, but none of them revolutionized our understanding of the corona" and that "[the experiments] all played their role in the normal progression of scientific knowledge, but there were no extraordinary results." On 11 August 1999, three Concorde aircraftone from France and two from the United Kingdomcarried out a similar feat carrying tourists instead of scientists. Passengers paid $2,400, but experienced only four or five minutes of totality, which was difficult to see because of the aircraft's small windows and the location of the Sun. A similar flight was planned for the 21 June 2001 solar eclipse, but was cancelled after the 2000 plane crash of Air France Flight 4590. == Notes ==
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