Radio astronomers find a lost satellite
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The detection of SOHO raises hopes for its recovery
28 July 1998 Ground-based radio telescopes have been
able to detect the Solar and Heliospheric Observatory (SOHO)
spacecraft and have found it rotating slowly near its original
position in space, a potentially important step toward possible
recovery of direct communications with the spacecraft.
Radio contact with SOHO, a joint mission of the European Space Agency (ESA) and NASA, was interrupted on June 24, an event under review by a joint ESA/NASA investigation board.
|With the encouragement of Dr. Alan Kiplinger of the National Oceanic and Atmospheric Administration's Space Environment Center in Boulder, CO, researchers at the U.S. National Astronomy and Ionosphere Center (NAIC) in Arecibo, Puerto Rico, used the facility's 305-meter (990-foot) diameter radio telescope to transmit a signal toward SOHO on July 23. The 70-meter dish of NASA's Deep Space Network in Goldstone, CA, acted as a receiver, locating the spacecraft's echo and tracking it using radar techniques for more than an hour.|
|How was SOHO Detected?|
The Arecibo Observatory, located in Puerto Rico, is operated by the National Astronomy and Ionosphere Center. The giant 305 meter dish is the world's most powerful RADAR. It can transmit pulses of radio energy with up to 500 mega-watts of power. The Arecibo radar has been used to map the surfaces of Venus and Mars, and to study the properties of near-Earth asteroids.
|Astronomers used a technique called bistatic radar to detect SOHO. Bistatic radar means that two radar dishes work together, in this case the 70m Goldstone antenna and the 305m Arecibo dish. The Arecibo dish is so large that its steering is limited. SOHO was only in its field of view for about an hour. The Arecibo RADAR team utilized the entire hour transmitting powerful pulses toward the satellite. Meanwhile, NASA's Deep Space Network radio antenna in Goldstone, CA, which is 60 degrees longitude to the west of Arecibo, was used to pick up the reflections. This is a technique that has also been used to study the rings of Saturn and asteroids. The image (right) shows the animated radar blip from the satellite recorded at Goldstone. The image links to a larger animation courtesy of Astronomy Now.|
Artist's conception of a bistatic RADAR experiment.
Preliminary analysis of the radar data, which is ongoing, indicates that SOHO is still in its nominal halo orbit and is turning slowly at a rate of roughly one revolution per minute. Staff members of NAIC and the Deep Space Network, in close cooperation with ESA and NASA, are continuing to analyze the radar data to extract more precise information on SOHO's location and motion, which in turn could help in future recovery efforts, as SOHO's solar panels turn toward the Sun.
Until recently the mission has been a spectacular success. According to Dr. David Hathaway of the NASA/MSFC Space Sciences Lab, SOHO observations have greatly advanced our understanding of coronal mass ejections ("CMEs"), solar magnetic fields, and the internal structure of the sun. "One thing SOHO does better than any earth-bound observatory is see the solar corona," explained Dr. Hathaway. "Coronagraphs here on Earth can only detect the inner, brightest parts of the corona, but SOHO can see 50 to 100 times further out, 24 hrs a day."
Solar physicists have been waiting expectantly for the year 2000 when the next solar maximum is expected to occur, but without SOHO observers will be operating with a severe handicap. "We'll be blind to many types of global activity on the sun," says Dr. Hathaway. "Also, SOHO was expected to complement observations by the ACE and TRACE spacecraft, already in orbit. We're really hoping that SOHO will be recovered."
ESA and NASA engineers are continuing their efforts to re-establish
radio data communication with the spacecraft, encouraged by the
radar measurement of a slow spin rate, which suggests minimal
structural damage has occurred. The slow spin rate also raises
hopes that within the next two months SOHO's solar panels will
once again rotate into the correct position to power the spacecraft,
and when that happens ground controllers will be able to re-establish
The Arecibo radar team was led by Dr. Donald Campbell. The NAIC is operated by Cornell University, Ithaca, NY, under a cooperative agreement with the U.S. National Science Foundation, Washington, DC. The Deep Space Network is managed by NASA's Jet Propulsion Laboratory, Pasadena, CA.