Radar-Interferometric Asteroid Imaging Using a Flexible Software Correlator

Astronomy and Astrophysics – Astronomy

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

1

Scientific paper

We've developed a technique to use a radio interferometer to image near earth objects (NEOs) during their close Earth approach when they can be illuminated by a ground-based radar system. There is great potential for this technique to yield detailed information that is complementary to other observational methods. We are using the NAIC's Arecibo Observatory's 1 MW 13 cm radar transmitter with the NRAO's Very Long Baseline Array (VLBA) as the receiving instrument. The VLBA, with antenna spacings of several thousands of kilometers, has a potential resolution on the order of milli-arcseconds; a couple of orders of magnitude smaller than typical ground-based telescopic observations, and sufficient to determine the gross shapes and orientations of spin vectors. Milli-arcsecond astrometry of these quickly moving objects can greatly improve their orbits and extend the span over which future Earth encounters can be predicted.
The VLBA hardware correlator limits the frequency resolution and complicates incorporating a model of the near-field geometry. Typical target bandwidths are ˜1 Hz while the correlator's narrowest resolution is 120 Hz. To avoid these difficulties a specialized computer interface was designed to transfer the raw data to commercial PCs. We can now use this system to obtain the individual antenna data streams and subsequently correlate them in software, bypassing the hardware correlator entirely. Software processing permits synthesis of narrower frequency bins, plus easier access for iterations to improve the near field model or correct a poor ephemeris a posteriori. This system could also be used to achieve high time resolution on strong sources.
We have recently used this system to observe near Earth asteroid (25143) Itokawa, a sub-kilometer sized object that passed within 0.013 AU of the Earth and is the target of the Japanese Hayabusa mission.
The National Radio Astronomy Observatory is a facility of the NSF operated under cooperative agreement by Associated Universities, Inc. The Arecibo Observatory is part of the National Astronomy and Ionosphere Center, which is operated by Cornell University under a cooperative agreement with the NSF.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Radar-Interferometric Asteroid Imaging Using a Flexible Software Correlator does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Radar-Interferometric Asteroid Imaging Using a Flexible Software Correlator, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Radar-Interferometric Asteroid Imaging Using a Flexible Software Correlator will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1276979

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.