PLASMA-WAVE OBSERVATIONS WITH GEOTAIL SPACECRAFT

被引:134
作者
MATSUMOTO, H
NAGANO, I
ANDERSON, RR
KOJIMA, H
HASHIMOTO, K
TSUTSUI, M
OKADA, T
KIMURA, I
OMURA, Y
OKADA, M
机构
[1] KANAZAWA UNIV,DEPT ELECT & COMP ENGN,KANAZAWA,ISHIKAWA 920,JAPAN
[2] UNIV IOWA,DEPT PHYS & ASTRON,IOWA CITY,IA 52242
[3] TOKYO DENKI UNIV,DEPT ELECT ENGN,TOKYO 101,JAPAN
[4] KYOTO SANGYO UNIV,INST COMP SCI,KYOTO 603,JAPAN
[5] TOYAMA PREFECTURAL UNIV,DEPT ELECTR & INFORMAT,KOSUGI,TOYAMA 93903,JAPAN
[6] KYOTO UNIV,DEPT ELECT ENGN 2,KYOTO 606,JAPAN
来源
JOURNAL OF GEOMAGNETISM AND GEOELECTRICITY | 1994年 / 46卷 / 01期
关键词
D O I
10.5636/jgg.46.59
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
The main scientific objectives of GEOTAIL Plasma Wave Instrument (PWI) are to investigate the characteristic features of wave phenomena which are generated by a variety of plasma processes occurring within the Earth's magnetosphere. The PWI measures plasma waves in the frequency range from 5.62 Hz to 800 kHz for the electric components and from 5.62 Hz to 12.5 kHz for the magnetic components. The instrument is composed of three distinct sets of receivers: (1) the Sweep Frequency Analyzer (SFA), (2) the Multi-Channel Analyzer (MCA) and (3) the Wave-Form Capture (WFC). The first two receivers are dedicated to wave spectra measurement. while the last one is used to capture actual wave forms of two electric and three magnetic field components for the measured plasma wave emissions. The present paper describes the PWI subsystems and their functions. We also report some results from initial observations made during the traversal of the geomagnetic tail and a skimming pass of the dayside magnetopause. These observational results are useful in providing a good overview of the PWI capabilities as well as elucidating the characteristic features of the wave spectra in these regions.
引用
收藏
页码:59 / 95
页数:37
相关论文
共 48 条
[1]   PLASMA-WAVES NEAR THE MAGNETOPAUSE [J].
ANDERSON, RR ;
HARVEY, CC ;
HOPPE, MM ;
TSURUTANI, BT ;
EASTMAN, TE ;
ETCHETO, J .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1982, 87 (NA4) :2087-2107
[2]  
ANDERSON RR, 1984, ESA SP217 EUR SPAC A, P199
[3]   ISEE OBSERVATIONS OF THE PLASMA SHEET BOUNDARY, PLASMA SHEET, AND NEUTRAL SHEET .2. WAVES [J].
CATTELL, CA ;
MOZER, FS ;
ANDERSON, RR ;
HONES, EW ;
SHARP, RD .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1986, 91 (A5) :5681-5688
[4]   CONTINUUM RADIATION AND ELECTRON-PLASMA OSCILLATIONS IN THE DISTANT GEOMAGNETIC TAIL [J].
CORONITI, FV ;
SCARF, FL ;
KENNEL, CF ;
GURNETT, DA .
GEOPHYSICAL RESEARCH LETTERS, 1984, 11 (07) :661-664
[5]  
FRANDSEN AMA, 1969, IEEE T GEOSCI ELECTR, V6, P61
[6]   NUMERICAL STUDY OF THE SPECTRUM OF BROAD-BAND ELECTROSTATIC NOISE IN THE MAGNETOTAIL [J].
GRABBE, CL .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1987, 92 (A2) :1185-1192
[7]   REGION OF INTENSE PLASMA-WAVE TURBULENCE ON AURORAL FIELD LINES [J].
GURNETT, DA ;
FRANK, LA .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1977, 82 (07) :1031-1050
[8]   ISEE-1 AND ISEE-2 PLASMA-WAVE INVESTIGATION [J].
GURNETT, DA ;
SCARF, FL ;
FREDRICKS, RW ;
SMITH, EJ .
IEEE TRANSACTIONS ON GEOSCIENCE AND REMOTE SENSING, 1978, 16 (03) :225-230
[9]   PLASMA-WAVE TURBULENCE AT THE MAGNETOPAUSE - OBSERVATIONS FROM ISEE 1 AND 2 [J].
GURNETT, DA ;
ANDERSON, RR ;
TSURUTANI, BT ;
SMITH, EJ ;
PASCHMANN, G ;
HAERENDEL, G ;
BAME, SJ ;
RUSSELL, CT .
JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS, 1979, 84 (NA12) :7043-7058
[10]  
GURNETT DA, 1976, J GEOPHYS RES-SPACE, V81, P6059, DOI 10.1029/JA081i034p06059