S. K. Solanki

Study reveals the link between solar faculae brightness and magnetic field strength.

Understanding darker regions in the Sun's corona linked to weak magnetic fields.

Combining data from two spacecraft reveals how solar brightness changes over time.

Researchers catalog sunspots to deepen understanding of solar activity and magnetic fields.

Scientists study the corona's heating mechanisms and complex emission line behavior.

Scientists investigate axions and their role in dark matter through innovative detection methods.

Examining the reliability and significance of solar magnetograms in understanding solar activity.

Recent findings from the CAST experiment refine limits on axion interactions.