In situ, broadband measurement of the radio frequency attenuation length at Summit Station, Greenland

被引：11

作者：

Aguilar, J. A. ^{[1
]}

Allison, P. ^{[2
]}

Beatty, J. J. ^{[2
]}

Besson, D. ^{[3
,4
]}

Bishop, A. ^{[5
,6
]}

Botner, O. ^{[7
]}

Bouma, S. ^{[8
]}

Buitink, S. ^{[9
]}

Cataldo, M. ^{[8
]}

Clark, B. A. ^{[10
]}

Curtis-Ginsberg, Z. ^{[11
]}

Connolly, A. ^{[2
]}

Dasgupta, P. ^{[1
]}

de Kockere, S. ^{[12
]}

de Vries, K. D. ^{[12
]}

Deaconu, C. ^{[11
]}

DuVernois, M. A. ^{[5
,6
]}

Glaser, C. ^{[7
]}

Hallgren, A. ^{[7
]}

Hallmann, S. ^{[13
]}

Hanson, J. C. ^{[14
]}

Hendricks, B. ^{[15
]}

Hornhuber, C. ^{[3
]}

Hughes, K. ^{[11
]}

Karle, A. ^{[5
,6
]}

Kelley, J. L. ^{[5
,6
]}

Kravchenko, I ^{[11
]}

Mulrey, K. ^{[17
]}

Nelles, A. ^{[8
,13
]}

Novikov, A. ^{[3
]}

Nozdrina, A. ^{[3
]}

Oberla, E. ^{[11
]}

Oeyen, B. ^{[18
]}

Pan, Y. ^{[19
]}

Pandya, H. ^{[9
]}

Plaisier, I ^{[8
,13
]}

Punsuebsay, N. ^{[19
]}

Pyras, L. ^{[8
,13
]}

Ryckbosch, D. ^{[18
]}

Scholten, O. ^{[12
,20
]}

Seckel, D. ^{[19
]}

Seikh, M. F. H. ^{[3
]}

Smith, D. ^{[11
]}

Southall, D. ^{[11
]}

Torres, J. ^{[2
]}

Toscano, S. ^{[1
]}

Tosi, D. ^{[5
,6
]}

Van den Broeck, D. J. ^{[9
,12
]}

van Eijndhoven, N. ^{[12
]}

Vieregg, A. G. ^{[11
]}

机构：

[1] Univ Libre Bruxelles, Sci Fac CP230, B-1050 Brussels, Belgium

[2] Ohio State Univ, Ctr Cosmol & AstroParticle Phys, Dept Phys, Columbus, OH 43210 USA

[3] Univ Kansas, Dept Phys & Astron, Lawrence, KS 66045 USA

[4] Natl Nucl Res Univ MEPhI, Kashirskoe Shosse 31, Moscow 115409, Russia

[5] Univ Wisconsin, Wisconsin IceCube Particle Astrophys Ctr WIPAC, Madison, WI 53703 USA

[6] Univ Wisconsin, Dept Phys, Madison, WI 53703 USA

[7] Uppsala Univ, Dept Phys & Astron, SE-75237 Uppsala, Sweden

[8] Friedrich Alexander Univ Erlangen Nuremberg, Erlangen Ctr Astroparticle Phys ECAP, D-91058 Erlangen, Germany

[9] Vrije Univ Brussel, Astrophys Inst, Pl Laan 2, B-1050 Brussels, Belgium

[10] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA

[11] Univ Chicago, Enrico Fermi Inst, Kavli Inst Cosmol Phys, Dept Phys, Chicago, IL 60637 USA

[12] Vrije Univ Brussel, Dienst ELEM, B-1050 Brussels, Belgium

[13] DESY, Platanenallee 6, D-15738 Zeuthen, Germany

[14] Whittier Coll, Whittier, CA 90602 USA

[15] Penn State Univ, Dept Phys, Dept Astron & Astrophys, University Pk, PA 16801 USA

[16] Univ Nebraska, Dept Phys & Astron, Lincoln, NE 68588 USA

[17] Radboud Univ Nijmegen, Dept Astrophys IMAPP, POB 9010, NL-6500 GL Nijmegen, Netherlands

[18] Univ Ghent, Dept Phys & Astron, B-9000 Ghent, Belgium

[19] Univ Delaware, Dept Phys & Astron, Newark, DE 19716 USA

[20] Univ Groningen, Kapteijn Inst, Groningen, Netherlands

[21] Univ Alabama, Dept Phys & Astron, Tuscaloosa, AL 35487 USA

[22] Calif Polytech State Univ San Luis Obispo, Phys Dept, San Luis Obispo, CA 93407 USA

来源：

JOURNAL OF GLACIOLOGY | 2022年 / 68卷 / 272期

基金：

美国国家科学基金会; 欧洲研究理事会;

关键词：

Ground-penetrating radar; ice physics; ice thickness measurements; radio-echo sounding; ROSS ICE SHELF; ANTARCTICA; PERFORMANCE; ENERGY; CORE; ZONE;

D O I：

10.1017/jog.2022.40

中图分类号：

P9 [自然地理学];

学科分类号：

0705 ; 070501 ;

摘要：

Over the last 25 years, radiowave detection of neutrino-generated signals, using cold polar ice as the neutrino target, has emerged as perhaps the most promising technique for detection of extragalactic ultra-high energy neutrinos (corresponding to neutrino energies in excess of 0.01 Joules, or 10(17) electron volts). During the summer of 2021 and in tandem with the initial deployment of the Radio Neutrino Observatory in Greenland (RNO-G), we conducted radioglaciological measurements at Summit Station, Greenland to refine our understanding of the ice target. We report the result of one such measurement, the radio-frequency electric field attenuation length L-alpha. We find an approximately linear dependence of L-alpha on frequency with the best fit of the average field attenuation for the upper 1500 m of ice: < L-alpha > = ((1154 +/- 121) - (0.81 +/- 0.14) (v/MHz)) m for frequencies v is an element of [145 - 3501 MHz.

引用

页码：1234 / 1242

页数：9

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