Detection of Solar Wind Disturbances: Mexican Array Radio Telescope IPS Observations at 140 MHz

[1]  A. Buffington,et al.  Comparison of Solar Wind Speeds Using Wavelet Transform and Fourier Analysis in IPS Data , 2015 .

[2]  M. Tokumaru,et al.  The wavelet transform function to analyze interplanetary scintillation observations , 2014 .

[3]  J. Gonzalez-Esparza,et al.  Numeric and analytic study of interplanetary coronal mass ejection and shock evolution: Driving, decoupling, and decaying , 2011 .

[4]  P. K. Manoharan.  Ooty Interplanetary Scintillation – Remote-Sensing Observations and Analysis of Coronal Mass Ejections in the Heliosphere , 2010 .

[5]  J. Gonzalez-Esparza,et al.  Observations of Interplanetary Scintillation (IPS) Using the Mexican Array Radio Telescope (MEXART) , 2010 .

[6]  P. K. Manoharan,et al.  Evolution of Coronal Mass Ejections in the Inner Heliosphere: A Study Using White-Light and Scintillation Images , 2006 .

[7]  J. Gonzalez-Esparza,et al.  The MEXART interplanetary scintillation array in Mexico , 2004 .

[8]  M. Tokumaru,et al.  Global Structure of Interplanetary Coronal Mass Ejections Retrieved from the Model Fitting Analysis of Radio Scintillation Observations , 2003 .

[9]  M. Tokumaru,et al.  Toroidal-shaped interplanetary disturbance associated with the halo coronal mass ejection event on 14 July 2000 , 2003 .

[10]  R. Fallows,et al.  EISCAT measurements of solar wind velocity and the associated level of interplanetary scintillation , 2002 .

[11]  N. Gopalswamy,et al.  Interplanetary acceleration of coronal mass ejections , 2000 .

[12]  P. K. Manoharan.  The solar cause of interplanetary disturbances observed in the distance range 0.24–1 AU , 1997 .

[13]  M. Dryer,et al.  Travelling interplanetary disturbances detected using interplanetary scintillation at 327 MHz , 1996 .

[14]  M. Dryer,et al.  Solar wind velocity and normalized scintillation index from single-station IPS observations , 1995 .

[15]  P. K. Manoharan.  Three-dimensional structure of the solar wind: Variation of density with the solar cycle , 1993 .

[16]  P. Janardhan,et al.  Angular source size measurements and interstellar scattering at 103 MHz using interplanetary scintillation , 1993 .

[17]  B. Rickett,et al.  Evolution of the solar wind structure over a solar cycle: Interplanetary scintillation velocity measurements compared with coronal observations , 1991 .

[18]  P. K. Manoharan,et al.  Determination of solar-wind velocities using single-station measurements of interplanetary scintillation , 1990 .

[19]  A. Hewish,et al.  The sources of large-scale heliospheric disturbances , 1986 .

[20]  P. Duffett-Smith,et al.  Observing interplanetary disturbances from the ground , 1982, Nature.

[21]  S. Ananthakrishnan,et al.  Observations of Interplanetary Scintillations at 327 MHz , 1974 .