Cosmic Ray & Star Formation
Type II Seesaw Portal and PAMELA/Fermi LAT Signals
Does Cosmic -ray flux vary during total solar eclipse (TSE) ? A random walk through TSEs PRANABA K NAYAK On behalf of TIFR Mumbai and J.C. Bose Institute.
Modeling the Sun’s global magnetic field
Modeling the Sun’s global magnetic field Karel Schrijver SHINE 2006 "[The] most important attitude is to find which forgotten physical processes are responsible.
Does Cosmic -ray flux vary during total solar eclipse (TSE) ? A random walk through TSEs
![Modeling the Sun’s global magnetic field Karel Schrijver SHINE 2006 "[The] most important attitude is to find which forgotten physical processes are responsible.](https://static.fdocuments.in/doc/330x215/5697bf731a28abf838c7ee80/modeling-the-suns-global-magnetic-field-karel-schrijver-shine-2006-the.jpg)
