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Earth Observing Laboratory
Field Data Archive

ACES: Eclipse Observations with the Airborne Coronal Emission Surveyor

Summary

The Airborne Coronal Emission Surveyor (ACES) is a new instrument using the Airborne Stabilized Platform for Infrared Experiments (ASPIRE) to explore the large-scale coronal IR emission spectrum during the 2024 total solar eclipse. ACES and ASPIRE will fly on the NSF NCAR Gulfstream V along the path of totality during the second Great American Eclipse in 2024. ACES will use the 20 cm optical feed from ASPIRE to map emission line intensity as a function of radius and solar magnetic structure.

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Datasets from this project

Additional information

Related links

Temporal coverage

Begin Date 2024-03-22 14:06:01
End Date 2024-04-09 17:25:59

Spatial coverage


Map data from IBCSO, IBCAO, and Global Topography.

Maximum (North) Latitude: 34.00, Minimum (South) Latitude: 28.00
Minimum (West) Longitude: -111.00, Maximum (East) Longitude: -93.00

NSF

This material is based upon work supported by the NSF National Center for Atmospheric Research, a major facility sponsored by the U.S. National Science Foundation and managed by the University Corporation for Atmospheric Research. Any opinions, findings and conclusions or recommendations expressed in this material do not necessarily reflect the views of the U.S. National Science Foundation.