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A Sample IHY 2007 Instrumentation Proposal

A Sample IHY 2007 Instrumentation Proposal. J. Kasper, B. Thompson, N. Fox. Overview. New technology: cheap radio receivers and computers to conduct low-frequency radio observations Option (1) low-frequency monitoring of solar radio bursts with single dipoles

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A Sample IHY 2007 Instrumentation Proposal

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  1. A Sample IHY 2007 Instrumentation Proposal J. Kasper, B. Thompson, N. Fox

  2. Overview • New technology: cheap radio receivers and computers to conduct low-frequency radio observations • Option (1) low-frequency monitoring of solar radio bursts with single dipoles • Option (2) 8-16 element arrays for all sky monitoring

  3. Low Frequency Antennae For a variety of reasons the designs for low-frequency radio antennae can be very straightforward This discussion borrows from figures developed by MIT,NRL, and ASTRON for the LOFAR project PVC pipe and copper wire

  4. Costing Let’s get a feel for the costs first, then talk about potential science Base cost estimates on LOFAR “compact core” Antenna + Receiver ~ $1,725 for 32 MHz bandwidth, full Stokes Computer + Processing board ~ $2,000 Infrastructure? Internet connection?

  5. What Science? Ionospheric scintillation and RFI make interferometric imaging very difficult at these low frequencies So we could either produce power spectra of the total power incident on the receiver (dominated by the Sun) Or we could build imaging arrays with low spatial resolution to act as all-sky monitors Virgo A seen by VLA at 74 MHz

  6. 1) Solar Spectra • Build simple stations consisting of a single antenna, receiver, and computer ( ~ $4,000 ) • The Sun will be the dominant contribution to the daytime signal, so produce • Produce high-resolution power spectra from 10-100 MHz at each station • Distribute these receivers across the globe to gain 24-hour coverage of the Sun at low frequencies • Observations are uploaded to a single data center

  7. Existing President 40 30 F [MHz] 20 10 The Bruny Island Radio Spectrometer (BIRS)1 W.C. Erickson Operational since 1994, observing from 3-30 MHz 1http://fourier.phys.utas.edu.au/birs/descrip.html

  8. 1) Proposal • Propose to the GLOBE program to produce these systems and make them available to classrooms • The computer would calculate the power spectra and both upload them to the central data center and display the results in real time in the classroom • Setup and operation is very straightforward • We gain continuous low frequency radio coverage of the Sun • The students learn about electromagnetism and the dynamic nature of the Sun

  9. 2) An Imaging Array Combine 8-16 of the individual receivers to construct an imaging array with low spatial resolution that monitors 30ox30o patch Antennae + Receivers $16,000-$32,000 Big single time cost is development of software

  10. 2) Proposal • Work with UNBSS to coordinate funding for universities to assemble and operate these arrays • Students learn about radio interferometers, solar and Jovian emission mechanisms • Science: Track emission from Jupiter as well as the Sun. Discovery potential, e.g. prompt afterglow from GRBs (HETE,SWIFT) • Would aim for he construction of several of these arrays

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