Seismic Images of the Far Side of the Sun
Affiliations
Images of an active region on the far side of the sun were derived by applying seismic holography to recent helioseismic observations from space. Active regions are the centers of energetic phenomena such as solar flares and coronal mass ejections, whose resulting electromagnetic and particle radiation interfere with telecommunications and power transmissions on Earth and can pose significant hazards to astronauts and spacecraft. Synoptic seismic imaging of far-side solar activity will now allow anticipation of the appearance of large active regions more than a week ahead of their arrival on the east solar limb.
Combined Surface Flux Transport and Helioseismic Far-Side Active Region Model (FARM).
Yang D, Heinemann S, Cameron R, Gizon L Sol Phys. 2024; 299(11):161.
PMID: 39618889 PMC: 11602821. DOI: 10.1007/s11207-024-02405-9.
Magnetism, dynamo action and the solar-stellar connection.
Brun A, Browning M Living Rev Sol Phys. 2020; 14(1):4.
PMID: 31997984 PMC: 6956918. DOI: 10.1007/s41116-017-0007-8.
Seismic imaging of the Sun's far hemisphere and its applications in space weather forecasting.
Lindsey C, Braun D Space Weather. 2018; 15(6):761-781.
PMID: 29398984 PMC: 5784405. DOI: 10.1002/2016SW001547.
Posner A, Hesse M, St Cyr O Space Weather. 2015; 12(4):257-276.
PMID: 26213516 PMC: 4508931. DOI: 10.1002/2013SW001007.