High time resolution PFISR and optical observations of naturally enhanced ion acoustic lines

被引:15
|
作者
Michell, R. G. [1 ]
Lynch, K. A. [1 ]
Heinselman, C. J. [2 ]
Stenbaek-Nielsen, H. C. [3 ]
机构
[1] Dartmouth Coll, Dept Phys & Astron, Hanover, NH 03755 USA
[2] SRI Int, Menlo Pk, CA 94025 USA
[3] Univ Alaska Fairbanks, Inst Geophys, Fairbanks, AK 99775 USA
关键词
Ionosphere; Plasma waves and instabilities; Wave-particle interactions; Magnetospheric physics; Auroral phenomena; FIELD-ALIGNED CURRENTS; RADAR OBSERVATIONS; AURORAL IONOSPHERE; EISCAT SVALBARD; ALFVEN WAVES; PLASMA; INSTABILITIES; ENERGIZATION; ACCELERATION; FLUCTUATIONS;
D O I
10.5194/angeo-27-1457-2009
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Observations of naturally enhanced ion acoustic lines (NEIALs) taken with the Poker Flat Incoherent Scatter Radar (PFISR) using a mode with very high time resolution are presented. The auroral event took place over Poker Flat, Alaska on 8 February 2007 at 09: 35 UT (similar to 22:00 MLT), and the radar data are complemented by common-volume high-resolution auroral imaging. The NEIALs occurred during only one of the standard 15-s integration periods. The raw data of this time show very intermittent NEIALs which occur only during a few very short time intervals (<= 1s) within the 15-s period. The time sampling of the raw data, similar to 19 ms on average, allows study of the time development of the NEIALs, though there are indications that even finer time resolution would be of interest. The analysis is based on the assumption that the NEIAL returns are the result of Bragg scattering from ion-acoustic waves that have been enhanced significantly above thermal levels. The spectra of the raw data indicate that although the up-and down-shifted shoulders can both become enhanced at the same time, (within 19 ms), they are most often enhanced individually. The overall power in the up-and down-shifted shoulders is approximately equal throughout the event, with the exception of one time, when very large up-shifted power was observed with no corresponding down-shifted power. This indicates that during the 480 mu s pulse, the strongly enhanced ion-acoustic waves were only traveling downward and not upward. The exact time that the NEIALs occurred was when the radar beam was on the boundary of a fast-moving (similar to 10 km/s), bright auroral structure, as seen in the high resolution auroral imaging of the magnetic zenith. When viewed with high time resolution, the occurrence of NEIALs is associated with rapid changes in auroral luminosity within the radar field of view due to fast-moving auroral fine structures.
引用
收藏
页码:1457 / 1467
页数:11
相关论文
共 50 条
  • [31] HIGH-RESOLUTION OBSERVATIONS OF INTERSTELLAR SODIUM D LINES WITH AN INTERFEROMETER
    VAUGHAN, AH
    MUNCH, G
    ASTRONOMICAL JOURNAL, 1966, 71 (03): : 184 - &
  • [32] High time resolution observations of Cataclysmic Variables with OPTIMA
    Kanbach, Gottfried
    Stefanescu, Alexander
    Duscha, Sven
    Steinle, Helmut
    Burwitz, Vadim
    Schwope, Axel
    UNIVERSE AT SUB-SECOND TIMESCALES: HIGH TIME RESOLUTION ASTROPHYSICS, 2008, 984 : 32 - +
  • [33] Advances in fusion of high resolution underwater optical and acoustic data
    Singh, H
    Roman, C
    Whitcomb, L
    Yoerger, D
    PROCEEDINGS OF THE 2000 INTERNATIONAL SYMPOSIUM ON UNDERWATER TECHNOLOGY, 1998, : 206 - 211
  • [34] High-resolution observations of shallow-water acoustic propagation with distributed acoustic sensing
    Shen, Zhichao
    Wu, Wenbo
    Lin, Ying-Tsong
    Journal of the Acoustical Society of America, 2024, 156 (04): : 2237 - 2249
  • [35] High-resolution observations of shallow-water acoustic propagation with distributed acoustic sensing
    Shen, Zhichao
    Wu, Wenbo
    Lin, Ying-Tsong
    JOURNAL OF THE ACOUSTICAL SOCIETY OF AMERICA, 2024, 156 (04): : 2237 - 2249
  • [36] HIGH-RESOLUTION RADIO AND OPTICAL OBSERVATIONS OF NGC 6888
    WENDKER, HJ
    SMITH, LF
    ISRAEL, FP
    HABING, HJ
    DICKEL, HR
    ASTRONOMY & ASTROPHYSICS, 1975, 42 (02) : 173 - 185
  • [37] High-resolution optical and infrared observations of molecules in comets
    Kim, SJ
    Minh, YC
    Hyung, S
    Kim, YH
    ASTROCHEMISTRY: FROM MOLECULAR CLOUDS TO PLANETARY SYSTEMS, 2000, (197): : 471 - 480
  • [38] Acoustic force mapping in a hybrid acoustic-optical micromanipulation device supporting high resolution optical imaging
    Thalhammer, Gregor
    McDougall, Craig
    MacDonald, Michael Peter
    Ritsch-Marte, Monika
    LAB ON A CHIP, 2016, 16 (08) : 1523 - 1532
  • [39] Nonlinear beam generated plasma waves as a source for enhanced plasma and ion acoustic lines
    Daldorff, L. K. S.
    Pecseli, H. L.
    Trulsen, J. K.
    Ulriksen, M. I.
    Eliasson, B.
    Stenflo, L.
    PHYSICS OF PLASMAS, 2011, 18 (05)
  • [40] Escaping ion measurement with high time resolution on CHS
    Shinohara, K.
    Isobe, M.
    Darrow, D. S.
    REVIEW OF SCIENTIFIC INSTRUMENTS, 2006, 77 (10):