Abstract
Solar physics has seen a decade of exciting science and discoveries, which were driven by new instruments for ground- and space-based observations. Multi-wavelength observations involving many observatories now routinely cover the whole solar atmosphere from photosphere, to chromosphere, transition region, corona, and heliosphere and have become an integral part in any type of space weather forecasting. The solar photosphere and chromosphere has historically been the domain of ground-based observatories and this review will be based on observations and research projects that have been carried out at the Big Bear Solar Observatory (BBSO) to illustrate current trends and prospects for ground-based experimental solar physics.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.