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.
Data access
Additional information
Related links |
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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