Download - Morocco Presentation Mon Stein
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Solar Instruments• Callisto as ETH - contribution to IHY2007 and ISWI
Compound Astronomical Low cost Low frequency Instrument for Spectroscopy and Transportable Observatory
Christian A. MonsteinInstitute of AstronomyWolfgang-Pauli-Strasse 278093 ZürichSwitzerland
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Specification CallistoParameter Main Specification
Frequency range 45.0 MHz … 870.0 MHzany other range, using heterodyne/homodyne converters
Frequency resolution 62.5 KHzRadiometric bandwidth 300 KHzDynamic range ~ 50 dBDetector gain 25 mV/dBNoise figure (9 ± 1) dBMeasuring rate 800 samples/sec max.Number of channels 1…400, nominal 200 frequencies per sweepPower consumption 12 V / ~225 mAWeight ~ 1 kgDimensions 110 mm x 80 mm x 205 mmMaterial cost < 200 € (time needed for production + test ~ 1 week)Inputs 3 configuration files (config, frequency, scheduler)Outputs 1 x FITS-file per 15 minutes and 1 x logfile per day
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IHY2007 24h observationHumain,Belgium
Ooty,India
Mexico
San JoseCosta Rica
Badary,Russia
PentictonUSA?
Zürich+BleienSwitzerland
Gauribi-danur
SouthKorea
MauritiusBrazil
Equador?
UlaanbaatarMongolia
Birr,Ireland Cuba?
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Why outside of Switzerland?
Radio frequency interference Switzerland compared to India and Russia
RFI in different countries
800
1000
1200
1400
1600
1800
2000
2200
2400
2600
500 510 520 530 540 550 560 570 580 590 600
Frequency [MHz]
Det
ecto
rout
put [
mV]
IndiaSwitzerlandBadary
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Callisto in Bleien, Switzerland
Top left: AntennaTop right: Meter wave spectrumBottom right: PCB Callisto
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Callisto in Gauribidanur, India
Left: Self built antenna.
Right V. C. Kathirvaran at Indian Institute of AstrophysicsGauribidanur / Bangalore
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Callisto in Badary/Siberia
Sergey and Andrey in Badary/Siberia
Antenna farm at SSRT
Antenna attached to dish
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Callisto in Daejeon, South Korea
Antenna tower of Solar and Space Weather Group of Korea Astronomy and Space Science Institute (KASI)
Student Hee-Sun reproducinga Callisto-spectrometer as asemester work in physics.
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Callisto at MRT in Mauritius
Self built log-per 20MHz … 860MHz and
Callisto in air-conditioned receiver roomin Bras d'Eau, Poste de Flacq, Mauritius
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First result Callisto in Mauritius
Astronomical outcome, group of type III flare as ‘first light’on May 1st 2009 08:08:30 UT
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How does DiRaC work
DiRaC
ETHZFITS
FITS
FITSRHESSI
Di = DistributedRa = Radio spectrometerC = Control
NOAA / GOES
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Publications
CALLISTO A New Concept for Solar Radio Spectrometer, Arnold Benz et. Al. Kluwer Academic Pub. (2004)On The Disk Hα And Radio Observations of the 2003 Oct. Flare And Coronal Mass Ejection Event (2005)Extended decimeter radio emission after large solar flares, Benz et. Al. (2005)Astronomisches Praktikum der ETH Zürich auf Diavolezza 2980m.ü.M., ORION 335, 4 (2006)Radio Spectrum Measurement at the Gauribidanur Observatory, C. Monstein, R. Ramesh (2007)Construction of an e-CALLISTO Station in Korea, Su-Chan Bong et. al., C. Monstein (2008)A World-Wide Net of Solar Radio Spectrometers: e-CALLISTO, Benz et. al. (2008)Observations of the Solar Radio Emission with the Callisto Spectrometer, Kh. A. Monstein, S. V. Lesovoy,and A. I. Maslov (2009)
Scientific papers(8 accepted and published)
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Info access
http://www.astro.phys.ethz.ch/rapp/http://www.astro.phys.ethz.ch/instrument/callisto/callisto_nf.htmlhttp://www.astro.phys.ethz.ch/instrument/callisto/ecallisto/applidocs.htm
ETH ZürichInstitute of AstronomyChristian MonsteinWolfgang-Pauli-Strasse 27CH-8093 Zürich