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    显示项目76-100 / 481. (共20页)
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    日期题名作者
    2010 Elliptical model of cutoff boundaries for the solar energetic particles measured by POES satellites in December 2006 Dmitriev,AV; Jayachandran,PT; Tsai,LC
    2010 Gigantic jets with negative and positive polarity streamers Chou,JK; Kuo,CL; Tsai,LY; Chen,AB; Su,HT; Hsu,RR; Cummer,SA; Li,J; Frey,HU; Mende,SB; Takahashi,Y; Lee,LC
    2010 Global, seasonal, and local time variations of ion density structure at the low-latitude ionosphere and their relationship to the postsunset equatorial irregularity occurrences Su,SY; Chen,MQ; Chao,CK; Liu,CH
    2010 Identification of earthquake signals from groundwater level records using the HHT method Chen,CH; Wang,CH; Liu,JY; Liu,C; Liang,WT; Yen,HY; Yeh,YH; Chia,YP; Wang,Y
    2010 Ionospheric electron content anomalies detected by a FORMOSAT-3/COSMIC empirical model before and after the Wenchuan Earthquake Kakinami,Y; Liu,JY; Tsai,LC; Oyama,KI
    2010 Ionospheric positive storm phases at the magnetic equator close to sunset Huang,CM; Chen,MQ; Liu,JY
    2010 ISUAL far-ultraviolet events, elves, and lightning current Chang,SC; Kuo,CL; Lee,LJ; Chen,AB; Su,HT; Hsu,RR; Frey,HU; Mende,SB; Takahashi,Y; Lee,LC
    2010 Longitudinal development of low-latitude ionospheric irregularities during the geomagnetic storms of July 2004 Li,GZ; Ning,BQ; Hu,LH; Liu,LB; Yue,XA; Wan,WX; Zhao,BQ; Igarashi,K; Kubota,M; Otsuka,Y; Xu,JS; Liu,JY
    2010 Magnetopause expansions for quasi-radial interplanetary magnetic field: THEMIS and Geotail observations Suvorova,AV; Shue,JH; Dmitriev,AV; Sibeck,DG; McFadden,JP; Hasegawa,H; Ackerson,K; Jelinek,K; Safrankova,J; Nemecek,Z
    2010 Midlatitude summer nighttime anomaly of the ionospheric electron density observed by FORMOSAT-3/COSMIC Lin,CH; Liu,CH; Liu,JY; Chen,CH; Burns,AG; Wang,W
    2010 Modeling the presunrise plasma heating in the low- to midlatitude topside ionospheres Chao,CK; Su,SY; Huba,JD; Oyama,KI
    2010 Observations of Equatorial Kelvin Wave Modes in FORMOSAT-3/COSMIC GPS RO Temperature Profiles Brahmanandam,PS; Chu,YH; Liu,J
    2010 Parallel proton fire hose instability in gyrotropic Hall MHD model Wang,BJ; Hau,LN
    2010 Periodic solar wind forcing due to recurrent coronal holes during 1996-2009 and its impact on Earth's geomagnetic and ionospheric properties during the extreme solar minimum Ram,ST; Liu,CH; Su,SY
    2010 Predawn ionospheric heating observed by Hinotori satellite Kakinami,Y; Balan,N; Liu,JY; Oyama,KI
    2010 Pre-seismic geomagnetic anomaly and earthquake location Chen,CH; Liu,JY; Lin,PY; Yen,HY; Hattori,K; Liang,WT; Chen,YI; Yeh,YH; Zeng,XP
    2010 Quiet time meridional (vertical) ion drifts at low and middle latitudes observed by ROCSAT-1 Pacheco,EE; Heelis,RA; Su,SY
    2010 Remote sensing of smoke plumes with moderate resolution imaging spectroradiometer reflectance measurements Lin,TH; Liu,GR; Chen,YC
    2010 Reply to comment by Lei et al. on &quot;A new aspect of ionospheric E region electron density morphology&quot; Chu,YH; Wu,KH; Su,CL
    2010 Role of mixed precipitating cloud systems on the typhoon rainfall Pan,CJ; Reddy,KK; Lai,HC; Yang,SS
    2010 Seismo-ionospheric anomalies of the GPS-TEC appear before the 12 May 2008 magnitude 8.0 Wenchuan Earthquake Jhuang,HK; Ho,YY; Kakinami,Y; Liu,JY; Oyama,KI; Parrot,M; Hattori,K; Nishihashi,M; Zhang,DH
    2010 Spatial Features of Current Systems of SFE-Flares Accompanied by Gamma Radiation Parkhomov,VA; Dmitriev,AV; Bazarzhapov,AD
    2010 Spatial profile of magnetic field in the near-Earth plasma sheet prior to dipolarization by THEMIS: Feature of minimum B Saito,MH; Hau,LN; Hung,CC; Lai,YT; Chou,YC
    2010 Stepwise feature of aurora during substorm expansion compared with the near-Earth tail dipolarization: Possible types of substorm dynamics Saito,MH; Miyashita,Y; Fujimoto,M; Liou,K; Saito,Y; Sigwarth,JB
    2010 Studying the Lunar Ionosphere with SELENE Radio Science Experiment Imamura,T; Iwata,T; Yamamoto,Z; Mochizuki,N; Kono,Y; Matsumoto,K; Liu,QH; Noda,H; Hanada,H; Oyama,K; Nabatov,A; Futaana,Y; Saito,A; Ando,H

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