Reliability of 1.8-meter solar radio telescope at Metsähovi Radio Observatory for long-term solar monitoring

Author:

Uunila Minttu,Kallunki Juha

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference10 articles.

1. Bruevich, E.A., Bruevich, V.V., Yakunina, G.V.: Sun Geosph. 8, 91 (2014)

2. Dominion Radio Astrophysical Observatory web site. http://www.nrc-cnrc.gc.ca/eng/solutions/facilities/drao.html , accessed on June 12, 2015

3. Huang, G.L., Song, Q.W.: Sol. Phys. 264, 345 (2010)

4. Kallunki, J.: Possibilities of the Metsähovi radiotelescopes for solar observations. Licentiate Thesis, Faculty of Information and Natural Sciences, Helsinki University of Technology, Espoo (2009)

5. Kallunki, J., Uunila, M.: Total solar flux intensity at 11.2 GHz as an indicator of solar activity and cyclicity. Int. J. Astron. Astrophys. 4, 437–444 (2014). doi: 10.4236/ijaa.2014.43039

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1. Solar Microwave Emission Associated with Coronal Mass Ejections (CME);Latvian Journal of Physics and Technical Sciences;2022-02-01

2. Development of a radio telescope for the observation of celestial bodies in the Ku Band;Journal of Physics: Conference Series;2019-06-01

3. Forty years of solar radio observations at Metsähovi Radio Observatory;Astronomische Nachrichten;2018-02

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