Mario, Fernández Ruiz; Javier, Bussons Gordo; Manuel, Prieto Mateo; Christian, Monstein
Automatic detection of e-Callisto solar radio bursts by Deep Neural Networks Proceedings Article
In: 3rd URSI AT-AP-RASC, Gran Canaria, 29 May – 3 June 2022, 2022.
@inproceedings{nokey,
title = {Automatic detection of e-Callisto solar radio bursts by Deep Neural Networks},
author = {Fernández Ruiz Mario and Bussons Gordo Javier and Prieto Mateo Manuel and Monstein Christian},
url = {http://www.irsol.usi.ch/wp-content/uploads/2022/06/URSI_ATAPRASC_Summary_Paper_FernandezRuiz_2022.pdf},
year = {2022},
date = {2022-06-01},
urldate = {2022-06-01},
booktitle = {3rd URSI AT-AP-RASC, Gran Canaria, 29 May – 3 June 2022},
abstract = {The aim of this work is to build a complete system based
on deep neural networks for automated burst recognition in
radio spectrograms delivered by ground-based solar observatories.
In this summary paper, the automatic system is described
stage by stage and preliminary results for a sample observatory are presented.
},
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The aim of this work is to build a complete system based
on deep neural networks for automated burst recognition in
radio spectrograms delivered by ground-based solar observatories.
In this summary paper, the automatic system is described
stage by stage and preliminary results for a sample observatory are presented.
on deep neural networks for automated burst recognition in
radio spectrograms delivered by ground-based solar observatories.
In this summary paper, the automatic system is described
stage by stage and preliminary results for a sample observatory are presented.
Setzer, M.; Küveler, G.; Zuber, A.; Bianda, M.; Ramelli, R.
Der Sonne auf der Spur Technical Report
publish-industry Verlag GmbH http://www.AuD24.net/PDF/AD12682460, 2013.
@techreport{Setzer2013bb,
title = {Der Sonne auf der Spur},
author = {Setzer, M. and Küveler, G. and Zuber, A. and Bianda, M. and Ramelli, R.},
url = {https://www.irsol.usi.ch/data/Papers/ad12682460.pdf},
year = {2013},
date = {2013-01-01},
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Küveler, G.; Dao, V. D.; Ramelli, R.
Benutzeroberflächen für die Oeffentlichkeitsarbeit astronomischer Einrichtungen Technical Report
2012, (ASTRONOMIE + RAUMFAHRT im Unterricht 127, 49. Jg., Heft 1/2012, S. 43-44.).
@techreport{Küveler2012,
title = {Benutzeroberflächen für die Oeffentlichkeitsarbeit astronomischer Einrichtungen},
author = {Küveler, G. and Dao, V.D. and Ramelli, R.},
year = {2012},
date = {2012-01-01},
note = {ASTRONOMIE + RAUMFAHRT im Unterricht 127, 49. Jg., Heft 1/2012, S. 43-44.},
keywords = {},
pubstate = {published},
tppubtype = {techreport}
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Küveler, G.; Dao, V. D.; Ramelli, R.
The new IRSOL solar telescope control system Technical Report
2011, (Astronomical Notes Vol.332, Issue 5, p.502).
@techreport{2011AN....332..502K,
title = {The new IRSOL solar telescope control system},
author = {Küveler, G. and Dao, V.D. and Ramelli, R.},
url = {http://adsabs.harvard.edu/abs/2011AN....332..502K},
doi = {10.1002/asna.201011515},
year = {2011},
date = {2011-01-01},
urldate = {2011-01-01},
journal = {Astronomische Nachrichten},
volume = {332},
pages = {502},
abstract = {We would like to present a new control system for the solar telescope now in operation at the Swiss institute, Istituto Ricerche Solari Locarno (IRSOL). The control software is multi-client capable, and optionally uses the primary image of the sun projected on a position sensor or the axis encoder for guiding. The hardware and software consist of three completely separate levels, which communicate with each other via ASCII commands. We shall describe the general principles implemented in the course of the development. We consider it important that this text is also applicable to other astronomical device controls. Therefore we explain our specific solution next to general principles.},
note = {Astronomical Notes Vol.332, Issue 5, p.502},
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pubstate = {published},
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We would like to present a new control system for the solar telescope now in operation at the Swiss institute, Istituto Ricerche Solari Locarno (IRSOL). The control software is multi-client capable, and optionally uses the primary image of the sun projected on a position sensor or the axis encoder for guiding. The hardware and software consist of three completely separate levels, which communicate with each other via ASCII commands. We shall describe the general principles implemented in the course of the development. We consider it important that this text is also applicable to other astronomical device controls. Therefore we explain our specific solution next to general principles.
Kleint, L.; Feller, A.; Gisler, D.
Imaging spectropolarimetry with two LiNbO3 Fabry Pérot interferometers and a spectrograph Technical Report
2011, (Astronomy and Astrophysics, Volume 529, A78).
@techreport{2011A&A...529A..78K,
title = {Imaging spectropolarimetry with two LiNbO3 Fabry Pérot interferometers and a spectrograph},
author = {Kleint, L. and Feller, A. and Gisler, D.},
url = {http://adsabs.harvard.edu/abs/2011A%26A...529A..78K},
doi = {10.1051/0004-6361/201015870},
year = {2011},
date = {2011-01-01},
urldate = {2011-01-01},
journal = {Astronomy and Astrophysics},
volume = {529},
pages = {A78},
note = {Astronomy and Astrophysics, Volume 529, A78},
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tppubtype = {techreport}
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Küveler, G.; Dao, V. D.; Zuber, A.; Ramelli, R.
Robotic and Non-Robotic Control of Astrophysical Instruments Technical Report
2010, (“Advances in Astronomy”, vol. 2010, Article ID 620424).
@techreport{2010AdAst2010E..27K,
title = {Robotic and Non-Robotic Control of Astrophysical Instruments},
author = {Küveler, G. and Dao, V.D. and Zuber, A. and Ramelli, R.},
url = {http://www.hindawi.com/journals/aa/2010/620424.html},
doi = {10.1155/2010/620424},
year = {2010},
date = {2010-01-01},
journal = {Advances in Astronomy},
volume = {2010},
pages = {620424},
note = {“Advances in Astronomy”, vol. 2010, Article ID 620424},
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Bulgheroni, A.; Bianda, M.; Caccia, M.; Cappellini, C.; Mozzanica, A.; Ramelli, R.; Risigo, F.
Characterization of a thinned back illuminated MIMOSA V sensor as a visible light camera Technical Report
Nuclear Instruments and Methods no. A, 565, 221, 2006.
@techreport{Bulgheroni2006,
title = {Characterization of a thinned back illuminated MIMOSA V sensor as a visible light camera},
author = {Bulgheroni, A. and Bianda, M. and Caccia, M. and Cappellini, C. and Mozzanica, A. and Ramelli, R. and Risigo, F.},
url = {https://www.irsol.usi.ch/data/Papers/abulgheroni_pixel2005.pdf},
year = {2006},
date = {2006-01-01},
urldate = {2006-01-01},
number = {A, 565, 221},
institution = {Nuclear Instruments and Methods},
abstract = {This paper reports the measurements that have been performed both in the Silicon Detector Laboratory at the University of Insubria (Como, Italy) and at the Instituto Ricerche SOlari Locarno (IRSOL) to characterize a CMOS pixel particle detector as a visible light camera. The CMOS sensor has been studied in terms of Quantum Efficiency in the visible spectrum, image blooming and reset inefficiency in saturation condition. The main goal of these measurements is to prove that this kind of particle detector can also be used as an ultra fast, 100% fill factor visible light camera in solar physics experiments.},
keywords = {},
pubstate = {published},
tppubtype = {techreport}
}
This paper reports the measurements that have been performed both in the Silicon Detector Laboratory at the University of Insubria (Como, Italy) and at the Instituto Ricerche SOlari Locarno (IRSOL) to characterize a CMOS pixel particle detector as a visible light camera. The CMOS sensor has been studied in terms of Quantum Efficiency in the visible spectrum, image blooming and reset inefficiency in saturation condition. The main goal of these measurements is to prove that this kind of particle detector can also be used as an ultra fast, 100% fill factor visible light camera in solar physics experiments.
Weisshaar, E.; Küveler, G.; Bianda, M.
Schnelle und genaue Methode zur Schwerpunktfindung in Messreihen Technical Report
2003, (Photonik, 35. Jg. No. 4- 2003, S. 46 – 48).
@techreport{Weisshaar2003,
title = {Schnelle und genaue Methode zur Schwerpunktfindung in Messreihen},
author = {Weisshaar, E. and Küveler, G. and Bianda, M.},
url = {https://www.irsol.usi.ch/data/Papers/Fourier_Methode.pdf},
year = {2003},
date = {2003-01-01},
journal = {2003 Photonik, 35. Jg. No. 4- 2003, S. 46 – 48},
note = {Photonik, 35. Jg. No. 4- 2003, S. 46 – 48},
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pubstate = {published},
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}
Küveler, G.; Klein, R.; Bianda, M.
Einsatz industrieller Bildverarbeitung in der Grundlagenforschung Technical Report
2003, (Photonik, 35, 66-68).
@techreport{Küveler2003,
title = {Einsatz industrieller Bildverarbeitung in der Grundlagenforschung},
author = {Küveler, G. and Klein, R. and Bianda, M.},
url = {https://www.irsol.usi.ch/data/Papers/Flare_photonik.pdf},
year = {2003},
date = {2003-01-01},
journal = {Photonik, 35, 66-68},
note = {Photonik, 35, 66-68},
keywords = {},
pubstate = {published},
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Küveler, G.; Wiehr, E.; Bianda, M.
Eine sensorgestützte Computersteuerung für Sonnenteleskope Technical Report
2000, (Automatisierungstechnische Praxis, 42 Heft 7, 50-54).
@techreport{Küveler2000,
title = {Eine sensorgestützte Computersteuerung für Sonnenteleskope},
author = {Küveler, G. and Wiehr, E. and Bianda, M.},
year = {2000},
date = {2000-01-01},
booktitle = {Automatisierungstechnische Praxis},
volume = {42 Heft 7},
pages = {50-54},
note = {Automatisierungstechnische Praxis, 42 Heft 7, 50-54},
keywords = {},
pubstate = {published},
tppubtype = {techreport}
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Küveler, G.; Wiehr, E.; Thomas, D.; Harzer, M.; Bianda, M.; Epple, A.; Sütterlin, P.; Weisshaar, E.
Automatic guiding of the primary image of solar Gregory telescopes Technical Report
1998, (Solar Physics, 182, 247-255).
@techreport{1998SoPh..182..247K,
title = {Automatic guiding of the primary image of solar Gregory telescopes},
author = {Küveler, G. and Wiehr, E. and Thomas, D. and Harzer, M. and Bianda, M. and Epple, A. and Sütterlin, P. and Weisshaar, E.},
url = {https://www.irsol.usi.ch/data/Papers/Papers/SP182-247.pdf},
doi = {10.1023/A:1005077109403},
year = {1998},
date = {1998-01-01},
urldate = {1998-01-01},
journal = {Solar Physics},
volume = {182},
pages = {247-255},
abstract = {The primary image reflected from the field stop of solar Gregory telescopes is used for automatic guiding. This new system avoids temporal varying influences from the bending of the telescope tube by the main mirror's gravity and from offsets between the telescope and a separate guiding refractor. The required stiffness of the guider mechanics and the small areas of the sensors demand small f numbers for the guider optics, which cause problems with the image quality and with heat. Problems also arise from the pinhole in the telescope's field stop which is imaged as a dark dot on the sensor. Pointing errors introduced by the telescope affect shifts of the solar image on the sensor. These are numerically determined by Fourier methods which are found to be less sensitive to noise than profile centering methods. Several types of guiders are tested, the final equipment, now installed at the Gregory telescopes at Tenerife and at Locarno, is described.},
note = {Solar Physics, 182, 247-255},
keywords = {},
pubstate = {published},
tppubtype = {techreport}
}
The primary image reflected from the field stop of solar Gregory telescopes is used for automatic guiding. This new system avoids temporal varying influences from the bending of the telescope tube by the main mirror's gravity and from offsets between the telescope and a separate guiding refractor. The required stiffness of the guider mechanics and the small areas of the sensors demand small f numbers for the guider optics, which cause problems with the image quality and with heat. Problems also arise from the pinhole in the telescope's field stop which is imaged as a dark dot on the sensor. Pointing errors introduced by the telescope affect shifts of the solar image on the sensor. These are numerically determined by Fourier methods which are found to be less sensitive to noise than profile centering methods. Several types of guiders are tested, the final equipment, now installed at the Gregory telescopes at Tenerife and at Locarno, is described.
Küveler, G.; Bianda, M.
Ein Observatorium wird automatisiert – Computereinsatz in der professionellen Astronomie Technical Report
1993, (ASTRONOMIE + Raumfahrt 17, S. 10-12.).
@techreport{Küveler1993,
title = {Ein Observatorium wird automatisiert – Computereinsatz in der professionellen Astronomie},
author = {Küveler, G. and Bianda, M.},
year = {1993},
date = {1993-01-01},
booktitle = {ASTRONOMIE + Raumfahrt 17},
pages = {10-12},
note = {ASTRONOMIE + Raumfahrt 17, S. 10-12.},
keywords = {},
pubstate = {published},
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Bianda, M.; Küveler, G.
L’automatizzazione di un osservatorio. Technical Report
1993, (REVISTATECHNICA 10, S. 79-81.).
@techreport{Bianda1993,
title = {L’automatizzazione di un osservatorio.},
author = {Bianda, M. and Küveler, G.},
year = {1993},
date = {1993-01-01},
booktitle = {REVISTATECHNICA},
volume = {10},
pages = {79-81},
note = {REVISTATECHNICA 10, S. 79-81.},
keywords = {},
pubstate = {published},
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