بيانات النشر: Uppsala universitet, Elektricitetslära
Uppsala universitet, Högenergifysik
Univ Libre Bruxelles, Sci Fac, CP 230, B-1050 Brussels, Belgium.
Ohio State Univ, Dept Phys, Ctr Cosmol & Astroparticle Phys, Columbus, OH 43210 USA.
Univ Kansas, Dept Phys & Astron, Lawrence, KS 66045 USA.;Natl Nucl Res Univ MEPhI, Kashirskoe Shosse 31, Moscow 115409, Russia.
Friedrich Alexander Univ Erlangen Nuremberg, Erlangen Ctr Astroparticle Phys ECAP, D-91058 Erlangen, Germany.
Vrije Univ Brussel, Inst Astrophys, Pleinlaan 2, B-1050 Brussels, Belgium.
Calif Polytechn State Univ, Phys Dept, San Luis Obispo, CA 93407 USA.
Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA.
Univ Chicago, Enrico Fermi Inst, Kavli Inst Cosmol Phys, Dept Phys, Chicago, IL 60637 USA.
Vrije Univ Brussel, Dienst ELEM, B-1050 Brussels, Belgium.
Univ Wisconsin Madison, Wisconsin IceCube Particle Astrophys Ctr WIPAC, Madison, WI 53703 USA.;Univ Wisconsin Madison, Dept Phys, Madison, WI 53703 USA.
DESY, Platanenallee 6, D-15738 Zeuthen, Germany.
Whittier Coll, Whittier, CA 90602 USA.
Penn State Univ, Dept Astron & Astrophys, Dept Phys, University Pk, PA 16801 USA.
Univ Kansas, Dept Phys & Astron, Lawrence, KS 66045 USA.
Lawrence Berkeley Natl Lab, Berkeley, CA 94720 USA.
Friedrich Alexander Univ Erlangen Nuremberg, Erlangen Ctr Astroparticle Phys ECAP, D-91058 Erlangen, Germany.;DESY, Platanenallee 6, D-15738 Zeuthen, Germany.
Univ Ghent, Dept Phys & Astron, B-9000 Ghent, Belgium.
Vrije Univ Brussel, Dienst ELEM, B-1050 Brussels, Belgium.;Univ Groningen, Kapte Inst, Groningen, Netherlands.
Univ Delaware, Dept Phys & Astron, Newark, DE 19716 USA.
Vrije Univ Brussel, Inst Astrophys, Pleinlaan 2, B-1050 Brussels, Belgium.;Vrije Univ Brussel, Dienst ELEM, B-1050 Brussels, Belgium.
Calif Polytechn State Univ, Phys Dept, San Luis Obispo, CA 93407 USA.;Penn State Univ, Dept Astron & Astrophys, Dept Phys, University Pk, PA 16801 USA.
Proceedings of Science
نبذة مختصرة : The Radio Neutrino Observatory in Greenland (RNO-G) is designed to make the first observations of ultra-high energy neutrinos at energies above 10 PeV, playing a unique role in multi-messenger astrophysics as the world's largest in-ice Askaryan radio detection array. The experiment will be composed of 35 autonomous stations deployed over a 5 x 6 km grid near NSF Summit Station in Greenland. The electronics chain of each station is optimized for sensitivity and low power, incorporating 150 - 600 MHz RF antennas at both the surface and in ice boreholes, low-noise amplifiers, custom RF-over-fiber systems, and an FPGA-based phased array trigger. Each station will consume 25 W of power, allowing for a live time of 70% from a solar power system. The communications system is composed of a high-bandwidth LTE network and an ultra-low power LoRaWAN network. I will also present on the calibration and DAQ systems, as well as status of the first deployment of 10 stations in Summer 2021.
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