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journal of advanced research
  
سال:2013 - دوره:4 - شماره:3
  
 
An early prediction of the maximum amplitude of the solar cycle 25
- صفحه:275-278
  
 
Comparison of COSMIC measurements with the IRI-2007 model over the eastern Mediterranean region
- صفحه:297-301
  
 
Deep solar minimum and global climate changes
- صفحه:209-214
  
 
EDITORIAL: Special issue on ‘‘Heliospheric Physics during and after a deep solar minimum’’
- صفحه:205-208
  
 
Education and public outreach at the Carl Sagan Solar Observatory of the University of Sonora
- صفحه:315-319
  
 
Geomagnetism during solar cycle 23: Characteristics
- صفحه:265-274
  
 
Helium shells and faint emission lines from slitlessflash spectra
- صفحه:307-313
  
 
How unprecedented a solar minimum was it?
- صفحه:253-258
  
 
Influence of projection effects on the observed differential rotation rate in the UV corona
- صفحه:283-286
  
 
Plasma properties from the multi-wavelength analysis of the November 1st 2003 CME/shock event
- صفحه:293-296
  
 
Solar origins of solar wind properties during the cycle 23 solar minimum and rising phase of cycle 24
- صفحه:221-228
  
 
Solar quiet day ionospheric source current in the West African region
- صفحه:303-305
  
 
Sources of solar wind over the solar activity cycle
- صفحه:215-220
  
 
Super- and sub-critical regions in shocks driven by radio-loud and radio-quiet CMEs
- صفحه:287-291
  
 
The Space Weather and Ultraviolet Solar Variability (SWUSV) Microsatellite Mission
- صفحه:235-251
  
 
The long-term variability of cosmic ray protons in the heliosphere: A modeling approach
- صفحه:259-263
  
 
The sunspot cycle no. 24 in relation to long term solar activity variation
- صفحه:279-282
  
 
Voyager observations of the interaction of the heliosphere with the interstellar medium
- صفحه:229-233
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