Statistical analysis of solar wind parameters and geomagnetic indices during HILDCAA/HILDCAA∗ occurrences between 1998 and 2007
暂无分享,去创建一个
[1] V. Klausner,et al. An Alternative Method for Identifying Interplanetary Magnetic Cloud Regions , 2017 .
[2] R. Hajra,et al. A study on the main periodicities in interplanetary magnetic field Bz component and geomagnetic AE index during HILDCAA events using wavelet analysis , 2016 .
[3] V. Klausner,et al. An alternative way to identify local geomagnetically quiet days: a case study using wavelet analysis , 2016 .
[4] B. Tsurutani,et al. Relativistic electron acceleration during HILDCAA events: are precursor CIR magnetic storms important? , 2015, Earth, Planets and Space.
[5] B. Tsurutani,et al. RELATIVISTIC (E > 0.6, > 2.0, AND > 4.0 MeV) ELECTRON ACCELERATION AT GEOSYNCHRONOUS ORBIT DURING HIGH-INTENSITY, LONG-DURATION, CONTINUOUS AE ACTIVITY (HILDCAA) EVENTS , 2015 .
[6] B. Tsurutani,et al. Superposed epoch analyses of HILDCAAs and their interplanetary drivers: Solar cycle and seasonal dependences , 2014 .
[7] Margarete Oliveira Domingues,et al. Daubechies wavelet coefficients: a tool to study interplanetary magnetic field fluctuations , 2014, 1404.2835.
[8] B. Tsurutani,et al. Solar wind‐magnetosphere energy coupling efficiency and partitioning: HILDCAAs and preceding CIR storms during solar cycle 23 , 2014 .
[9] B. Tsurutani,et al. Relativistic electron acceleration during high‐intensity, long‐duration, continuous AE activity (HILDCAA) events: Solar cycle phase dependences , 2014 .
[10] B. Tsurutani,et al. Solar cycle dependence of High‐Intensity Long‐Duration Continuous AE Activity (HILDCAA) events, relativistic electron predictors? , 2013 .
[11] Bruce T. Tsurutani,et al. The Interplanetary Causes of Magnetic Storms: A Review , 2013 .
[12] F. Guarnieri. The Nature of Auroras During High‐Intensity Long‐Duration Continuous AE Activity (HILDCAA) Events: 1998 to 2001 , 2013 .
[13] C. Russell. Solar Wind and Interplanetary Magnetic Field: A Tutorial , 2013 .
[14] C. Russell,et al. Comparing Solar Minimum 23/24 with Historical Solar Wind Records at 1 AU , 2011 .
[15] Ezequiel Echer,et al. Interplanetary conditions causing intense geomagnetic storms (Dst ≤ −100 nT) during solar cycle 23 (1996–2006) , 2008 .
[16] R. Schwenn,et al. Solar Wind Sources and Their Variations Over the Solar Cycle , 2007 .
[17] Christopher T. Russell,et al. Properties of Stream Interactions at One AU During 1995 – 2004 , 2006 .
[18] Y. Kasahara,et al. Corotating solar wind streams and recurrent geomagnetic activity: A review , 2006 .
[19] Harald U. Frey,et al. Coordinated studies of the geospace environment using Cluster, satellite and ground-based data: an interim review , 2005 .
[20] G. Moon,et al. SEASONAL AND UNIVERSAL TIME VARIATIONS OF THE AU, AL AND DST INDICES , 2003 .
[21] W. Gonzalez,et al. Solar and interplanetary causes of very intense geomagnetic storms , 2001 .
[22] Ian G. Richardson,et al. Sources of geomagnetic activity over the solar cycle: Relative importance of coronal mass ejections, high‐speed streams, and slow solar wind , 2000 .
[23] Robert L. Lysak,et al. Introduction to Space Physics , 1995 .
[24] B. Tsurutani,et al. Interplanetary origin of geomagnetic activity in the declining phase of the solar cycle , 1995 .
[25] A. Viljanen,et al. On induction effects at EISCAT and IMAGE magnetometer stations , 1995 .
[26] H. W. Kroehl,et al. What is a geomagnetic storm , 1994 .
[27] J. Gosling. Coronal mass ejections: The link between solar and geomagnetic activity* , 1993 .
[28] G. Parks,et al. Physics Of Space Plasmas: An Introduction , 1991 .
[29] B. Tsurutani,et al. Interplanetary Alfvén waves and auroral (substorm) activity: IMP 8 , 1990 .
[30] B. Tsurutani,et al. Solar wind-magnetosphere coupling during intense magnetic storms (1978-1979) , 1989 .
[31] B. Tsurutani,et al. Origin of interplanetary southward magnetic fields responsible for major magnetic storms near solar maximum (1978–1979) , 1988 .
[32] B. Tsurutani,et al. The cause of high-intensity long-duration continuous AE activity (HILDCAAs): Interplanetary Alfvén wave trains , 1987 .
[33] Wolfgang Baumjohann,et al. Estimation of ionospheric electric fields and currents from a regional magnetometer array , 1985 .
[34] N. R. Sheeley,et al. A pictorial comparison of interplanetary magnetic field polarity, solar wind speed, and geomagnetic disturbance index during the sunspot cycle , 1977 .
[35] J. Harvey,et al. Coronal holes, solar wind streams, and recurrent geomagnetic disturbances: 1973–1976 , 1976 .
[36] E. Smith,et al. Observations of interaction regions and corotating shocks between one and five AU - Pioneers 10 and 11. [solar wind streams] , 1976 .
[37] F. Mozer,et al. A quantitative model for the potential resulting from reconnection with an arbitrary interplanetary magnetic field , 1974 .
[38] Masahisa Sugiura,et al. Auroral electrojet activity index AE and its universal time variations. , 1966 .
[39] Masahisa Sugiura,et al. Hourly values of equatorial dst for the igy , 1963 .
[40] J. Dungey. Interplanetary Magnetic Field and the Auroral Zones , 1961 .
[41] D. Evans,et al. Evidence for particle injection as the cause of Dst reduction during HILDCAA events , 2004 .
[42] B. Tsurutani,et al. Are high-intensity long-duration continuous AE activity (HILDCAA) events substorm expansion events? , 2004 .
[43] S. Suess,et al. From the Sun, Auroras, Magnetic Storms, Solar Flares, Cosmic Rays , 1998 .
[44] P. Mayaud,et al. Derivation, Meaning, and Use of Geomagnetic Indices , 1980 .