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Future High-Resolution and High-Cadence Observations for Unraveling Eruptive Solar Features

Many of the key advances in solar science over the previous fifty years have been strongly influenced by imaging with increasing resolution and cadence of the Sun’s atmosphere from space. There is still much room for further advances in this area in the coming decades. Here we demonstrate this need using as an example recent past advances of the features known as solar coronal jets. Over the last few decades jet studies have progressed substantially, and much of this is due to improved resolution and cadence in imaging, along with concurrent magnetic field and spectroscopic observations.
Document ID
20205007416
Acquisition Source
Marshall Space Flight Center
Document Type
White Paper
Authors
Alphonse C Sterling
(Marshall Space Flight Center Redstone Arsenal, Alabama, United States)
Ronald L Moore
(University of Alabama in Huntsville Huntsville, Alabama, United States)
Date Acquired
September 10, 2020
Publication Date
September 1, 2020
Publication Information
Subject Category
Solar Physics
Funding Number(s)
WBS: 955518.02.01.06.32
Distribution Limits
Public
Copyright
Use by or on behalf of the US Gov. Permitted.
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