A nonnegligible type of eruption in the solar atmosphere—jets

LIU Jia-Jia; WANG Yu-Ming

doi:10.7693/wl20161101

PHYSICS > 2016 > 45(11): 689-700. > DOI: 10.7693/wl20161101

LIU Jia-Jia, WANG Yu-Ming. A nonnegligible type of eruption in the solar atmosphere—jets[J]. PHYSICS, 2016, 45(11): 689-700. DOI: 10.7693/wl20161101

Citation:

LIU Jia-Jia, WANG Yu-Ming. A nonnegligible type of eruption in the solar atmosphere—jets[J]. PHYSICS, 2016, 45(11): 689-700. DOI: 10.7693/wl20161101

Citation:

LIU Jia-Jia, WANG Yu-Ming. A nonnegligible type of eruption in the solar atmosphere—jets[J]. PHYSICS, 2016, 45(11): 689-700. DOI: 10.7693/wl20161101

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A nonnegligible type of eruption in the solar atmosphere—jets

LIU Jia-Jia^†,
WANG Yu-Ming

CAS Key Laboratory of Geospace Environment,School of Earth and Space Sciences,University of Science and Technology of China,Hefei 230026,China

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Received Date: September 07, 2016
Published Date: November 11, 2016

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Abstract

The first solar jet seen by human beings was observed as an Hα surge by the Mt.Wilson Observatory in the 1920s. As jets are neither as dazzling as solar flares, nor can they affect the terrestrial environment like coronal mass ejections (CME), they failed to attract much attention. However, recent progress has shown that jets are playing very important roles in solar magnetic field topology and evolution, interacting with solar magnetohydradynamics (MHD) waves (such as Alfvénic waves), and heating local corona and accelerating fast solar winds. They could also have a close relationship with extreme solar eruptions such as flares and CMEs. In this article, we will briefly introduce the theories and observations of solar jets, and then describe our recent study on a solar jet triggering a fast coronal mass ejection. Finally, we will summarize some key problems that need to be solved, and key points for future research.
- solar activity,
- solar jet,
- coronal mass ejection,
- magnetic reconnection,
- solar flare

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