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- Transforming the Arecibo Observatory into a Classroom31 Mar, 2020
- Arecibo Observatory re-enters VLBI network with 21st-century backend31 Mar, 2020
- JWST Workshop 31 Mar, 2020
- Management Update (COVID-19, Eartquakes, Transmitters)27 Mar, 2020
- NANOGrav Meeting Hosted at UCF27 Mar, 2020
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- REU Student Mishaal Jan Publishes Summer Research Study about Massive Star Forming Region26 Mar, 2020
- AO helps detect Magnetar in the Cow26 Mar, 2020
- Pulsar Astronomy and Physics at the Arecibo Observatory with Dr. Joanna Rankin26 Mar, 2020
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- GBO/AO Single Dish and Observer Training Workshops (May 11-20, 2020)05 Feb, 2020
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- The Arecibo Observatory Congratulates Dr. Martha P. Haynes, Recipient of 2019 Bruce Gold Medal11 Dec, 2019
The sensitivity of the Arecibo Observatory made possible to observe Gyrolines
Byadmin03 November 2017 Atmospheric
“Gyroline is observed and investigated theoretically and experimentally... The analysis is supported by range-resolved incoherent scatter spectrograms measured recently at Arecibo... The sensitivity of the Arecibo Observatory was prerequisite for this study”.
Title: The sensitivity of the Arecibo Observatory made possible to observe GyrolinesCitation: Hysell, D. L., J. Vierinen, and M. P. Sultzer (2017), On the theory of the incoherent scatter gyrolines, Radio Sci., 52, 723–730, doi:10.1002/2017RS006283.
Web Link: http://onlinelibrary.wiley.com/doi/10.1002/2017RS006283/full
Keywords: incoherent scatter spectrograms, arecibo, gyroline, hysell, vierinen, sultzer