INAF Space Weather assets/Solar emissions in the radio bands.
|Facility||Description||Contacts||Logistics and ownerships||Specifications||Data products||Data archiving||National and international involvements|
|SunDish||Single-Dish Imaging and Monitoring of the Sun in the Centimetre-Millimetre band by Italian Radio Telescopes. Single-Dish Radio Telescopes configurations aimed at spectro-polarimetric imaging and spectral timing of the Solar Corona and Chromosphere in the frequency range 1–50 GHz (with primary goals about continuum imaging in K-band)||Alberto Pellizzoni firstname.lastname@example.org||INAF-Osservatorio Astronomico di Cagliari INAF – Istituto di Radioastronomia, Bologna & Noto||Application Type: High-frequency radio monitoring of the Sun Spectro-polarimetric imaging and dynamic spectra||Continuum and spectro-polarimetric images of the Sun, dynamic spectra on selected regions (mostly K-band and in perspective Q-band)||INAF and/or ASI data archiving facilities||Italian Radio Telescope Network|
|INAF – Osservatorio Astronomico di Trieste||LOFAR Observations for Space Weather|
|ASI – Agenzia Spaziale Italiana, Università di Cagliari, Dipartimento di Fisica||SKA Observations for Space Weather|
|Università di Trieste, Dipartimento di Fisica|
|ASTRON – Netherlands Institute for Radio Astronomy|
|Trieste Callisto System||Solar radio spectrography in the VHF and UHF bands. Monitoring of coronal solar radio emissions.||Alessandro Marassi email@example.com||INAF –Osservatorio Astronomico di Trieste||Low time resolution, limited receiving band solar radio spectrography with no polarisation information and no radiometric calibration||Solar radiometric data (arbitrary units) in the 45–81 MHz and 220–420 bands with radio burst automatic identification||Solar radio spectra images (2013–)||e-Callisto solar radio spectrograph network|
|Solar radio spectra FITS files (2013–)||ISWI International Space Weather Initiative|
|Local and global e-Callisto digital archive available via web|
|TSRS – Trieste Solar Radio System 2.0||Multichannel solar radio polarimetry and spectropolarimetry in the UHF and SHF bands (3 m dish; fully automated system). Monitoring of photospheric, chromospheric and coronal radio emissions with special attention to the solar activity index at 2800 MHz and to the solar radio noise in the L-band for GNSS data quality evaluation||Mauro Messerotti firstname.lastname@example.org||INAF-Osservatorio Astronomico di Trieste||Calibrated, high time resolution and high Circular Polrisation accuracy time series at selected frequencies and radio spectra of selected bands.||L-band (1350–1450 MHz) 2800 MHz (narrowband) C-band (3–4 GHz) Ku-band (11.5–12.5 GHz) Ka-band (22–23 GHz)||Time of operation start: 2019 Q1||Italian Radio Telescope Network|
|Solar radio time series||LOFAR Obervations for Space Weather|
|Solar radio spectra images||SKA Observations for Space Weather|
|Solar radio spectra images||ESA Space Situational Awareness|
|Solar radio indices||Enabling science facility for SolO/Metis|
|Data available in near-real-time through a web interface and web services|
|Local archive and long-term preservation archiving in INAF IA2|
|TSRS –Trieste Solar Radio System 1.0||Multichannel solar radio polarimetry in the VHF and UHF bands (10 m and 3 m dish) Solar radio Interferometry in UHF (400 MHz, two dipole arrays at 100 λ) These data provide information about the coronal plasma emissions.||Mauro Messerotti email@example.com||INAF-Osservatorio Astronomico di Trieste CNR-National Research Council Università di Trieste, Dipartimento di Astronomia||Calibrated, High time resolution (50 Hz to 2 kHz sampling rate) and high Circular Polarization accuracy (1%) time series of single-frequency observations Low spatial resolution interferometric observations||Radio polarimetric data On paper 239 MHz (1969–70) 235 MHz (1970–71) 237 MHz (1971–79)||Data on paper recordings only (1969–2003) Data in digital format (1975–1994; events) Data in digital format (1997–2010; all) The data in digital format are stored in I INAF IA2 for long-term preservation.||Space Weather data for USAF|
|In digital format 237, 327, 408, 505, 610, 790 MHz (1979–95)|
|Stop for upgrade (1995–97)||Solar radio monitoring for ESA Space Weather European Network|
|Restart (1997) 237, 327, 408, 610, 1420, 2695 MHz (1997/99–2010) Stop for lightning stroke (2010)|
|Radio interferometric data||Enabling science facility in support of SOHO/UVCS|
|On paper 408 MHz (1979–82)|
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