Open AccessOn the Little‐Known Consequences of the 4 August 1972 Ultra‐Fast Coronal Mass Ejecta: Facts, Commentary, and Call to Action
Author(s) -
Knipp Delores J.,
Fraser Brian J.,
Shea M. A.,
Smart D. F.
Publication year - 2018
Publication title -
space weather
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.254
H-Index - 56
ISSN - 1542-7390
DOI - 10.1029/2018sw002024
Subject(s) - space weather , coronal mass ejection , ejecta , geomagnetically induced current , geomagnetic storm , solar flare , plasmasphere , storm , geophysics , magnetosphere , solar wind , history , meteorology , physics , astronomy , magnetic field , quantum mechanics , supernova
Today the extreme space weather events of early August 1972 are discussed as benchmarks for Sun‐Earth transit times of solar ejecta (14.6 hr) and for solar energetic particle fluxes (10 MeV ion flux >70,000 cm −2 ·s −1 ·sr −1 ). Although the magnetic storm index, Dst, dipped to only −125 nT, the magnetopause was observed within 5.2 R E and the plasmapause within 2 R E . Widespread electric‐ and communication‐grid disturbances plagued North America late on 4 August. There was an additional effect, long buried in the Vietnam War archives that add credence to the severity of the storm impact: a nearly instantaneous, unintended detonation of dozens of sea mines south of Hai Phong, North Vietnam on 4 August 1972. The U.S. Navy attributed the dramatic event to magnetic perturbations of solar storms . Herein we discuss how such a finding is broadly consistent with terrestrial effects and technological impacts of the 4 August 1972 event and the propagation of major eruptive activity from the Sun to the Earth. We also provide insight into the solar, geophysical, and military circumstances of this extraordinary situation. In our view this storm deserves a scientific revisit as a grand challenge for the space weather community, as it provides space‐age terrestrial observations of what was likely a Carrington‐class storm.