How an eclipse becomes a multi-layered laboratory

The eclipse over parts of Europe will briefly reveal the normally hidden solar corona, but natural totality lasts only a few minutes.[5] NASA’s WB-57 jet will chase the Moon’s shadow with four cameras, while NASA-supported balloon teams will measure atmospheric changes as daylight abruptly dims.[8]

Published

The eclipse over parts of Europe will briefly reveal the normally hidden solar corona, but natural totality lasts only a few minutes.[5] NASA’s WB-57 jet will chase the Moon’s shadow with four cameras, while NASA-supported balloon teams will measure atmospheric changes as daylight abruptly dims.[8] Why it matters: The combined campaign can connect coronal structures and outflows with the solar wind while examining how sudden darkness changes ozone and Earth’s temperature- and moisture-sensitive atmospheric boundary layer.[8] Key insights: Aircraft can lengthen the useful observing window by moving with the Moon’s shadow rather than remaining at one ground location.[8] | Four cameras inside the WB-57’s nose cone will image the corona’s structures, outflows and changes.[8] | Balloon measurements target ozone and the atmospheric boundary layer, turning the eclipse into an Earth-science experiment as well as a solar one.[8] | ESA also uses artificial-eclipse missions and computer simulations because natural total eclipses are rare and brief.[5] Cheatsheet facts: What changed: NASA is combining a shadow-chasing WB-57 jet with balloon observations for the Aug. 12 eclipse.[8] | Why now: Totality briefly exposes the corona, creating a rare observing opportunity that lasts at most a few minutes from any natural eclipse vantage point.[5] | Watch next: Watch for the jet’s coronal imagery and balloon measurements of ozone and boundary-layer changes collected during the eclipse.[8]
Visual Cheatsheet Version A for How an eclipse becomes a multi-layered laboratory. Full text follows for assistive technology.
The eclipse over parts of Europe will briefly reveal the normally hidden solar corona, but natural totality lasts only a few minutes.[5] NASA’s WB-57 jet will chase the Moon’s shadow with four cameras, while NASA-supported balloon teams will measure atmospheric changes as daylight abruptly dims.[8] Why it matters: The combined campaign can connect coronal structures and outflows with the solar wind while examining how sudden darkness changes ozone and Earth’s temperature- and moisture-sensitive atmospheric boundary layer.[8] Key insights: Aircraft can lengthen the useful observing window by moving with the Moon’s shadow rather than remaining at one ground location.[8] | Four cameras inside the WB-57’s nose cone will image the corona’s structures, outflows and changes.[8] | Balloon measurements target ozone and the atmospheric boundary layer, turning the eclipse into an Earth-science experiment as well as a solar one.[8] | ESA also uses artificial-eclipse missions and computer simulations because natural total eclipses are rare and brief.[5] Cheatsheet facts: What changed: NASA is combining a shadow-chasing WB-57 jet with balloon observations for the Aug. 12 eclipse.[8] | Why now: Totality briefly exposes the corona, creating a rare observing opportunity that lasts at most a few minutes from any natural eclipse vantage point.[5] | Watch next: Watch for the jet’s coronal imagery and balloon measurements of ozone and boundary-layer changes collected during the eclipse.[8]
X copy pack
Download cheatsheet PNG

Edition complete

You've reached the end of this edition.

Free to start. You'll create an account, then confirm the link before anything runs.

Create your own briefings — freeRead the full editionBrowse every cheatsheetRead in Briefings