2016/05/27 by А. Бемпорад, Alessandro Bemporad, Roberto Susino +3 · 2 citations
Physics and Astronomy · #Astron #Astronomy #Astrophysics #Front (military) #Ionosphere and magnetosphere dynamics #Magnetic field #Mechanics #Meteorology #Physics #Shock (circulatory) #Shock front #Shock wave #Solar and Space Plasma Dynamics #Solar physics #Space (punctuation) #Space physics #Stellar, planetary, and galactic studies #astro-ph.SR
paper · pdf · doi:10.3389/fspas.2016.00017
published in Frontiers in Astronomy and Space Sciences 3 (Frontiers Media) · 8 pages, 1 figure
openalex publication_date 2016/05/27 · openalex created_date 2016/06/24 · arxiv created 2016/08/19 · arxiv updated 2016/08/22 · openalex updated_date 2026/08/05
Recent works demonstrated that remote sensing observations of shock waves propagating into the corona and associated with major solar eruptions can be used to derive the strength of coronal magnetic fields met by the shock over a very large interval of heliocentric distances and latitudes. This opinion article will summarize most recent results obtained on this topic and will discuss the weaknesses and strengths of these techniques to open a constructive discussion with the scientific community.