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   journal of advanced research   
سال:2013 - دوره:4 - شماره:3


  tick  An early prediction of the maximum amplitude of the solar cycle 25 - صفحه:275-278

  tick  Comparison of COSMIC measurements with the IRI-2007 model over the eastern Mediterranean region - صفحه:297-301

  tick  Deep solar minimum and global climate changes - صفحه:209-214

  tick  EDITORIAL: Special issue on ‘‘Heliospheric Physics during and after a deep solar minimum’’ - صفحه:205-208

  tick  Education and public outreach at the Carl Sagan Solar Observatory of the University of Sonora - صفحه:315-319

  tick  Geomagnetism during solar cycle 23: Characteristics - صفحه:265-274

  tick  Helium shells and faint emission lines from slitlessflash spectra - صفحه:307-313

  tick  How unprecedented a solar minimum was it? - صفحه:253-258

  tick  Influence of projection effects on the observed differential rotation rate in the UV corona - صفحه:283-286

  tick  Plasma properties from the multi-wavelength analysis of the November 1st 2003 CME/shock event - صفحه:293-296

  tick  Solar origins of solar wind properties during the cycle 23 solar minimum and rising phase of cycle 24 - صفحه:221-228

  tick  Solar quiet day ionospheric source current in the West African region - صفحه:303-305

  tick  Sources of solar wind over the solar activity cycle - صفحه:215-220

  tick  Super- and sub-critical regions in shocks driven by radio-loud and radio-quiet CMEs - صفحه:287-291

  tick  The Space Weather and Ultraviolet Solar Variability (SWUSV) Microsatellite Mission - صفحه:235-251

  tick  The long-term variability of cosmic ray protons in the heliosphere: A modeling approach - صفحه:259-263

  tick  The sunspot cycle no. 24 in relation to long term solar activity variation - صفحه:279-282

  tick  Voyager observations of the interaction of the heliosphere with the interstellar medium - صفحه:229-233
 

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