Impact of the 1 April 2026 Artemis II Rocket Launch on the Upper Atmosphere: TIMED/GUVI Observations

Abstract The NASA Artemis II rocket was successfully launched at 06:35 p.m. ET (22:35 UTC) on 1 April 2026 from the Kennedy Space Center (28°35′28″N 80°39′03″W). The rocket plume caused enhanced Lyman α emission (up to ∼3 kR) observed by TIMED/GUVI on 2–6 April (5 days). Its peak intensity decreased linearly from April 3 at a rate ∼740 R/day. The half‐maximum width of the zonal Lyman α intensities at 20°–30° latitude (at ∼01:30 p.m. local solar time) increased from ∼3,000 km on April 2–∼9,000 km on April 6. GUVI also detected significant reductions in O‐130.4 nm and O‐135.6 nm radiances, indicating O density reduction. Weakly enhanced NO ε band intensity (NO density) was also observed on April 2 and 3. These features are due to photochemical processes associated with water vapor in the rocket plume and diffusion.

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Publication Details

Journal
Geophysical Research Letters
Published
2026-10-27
DOI
https://doi.org/10.1029/2026gl125425
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
0.00

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article

Impact of the 1 April 2026 Artemis II Rocket Launch on the Upper Atmosphere: TIMED/GUVI Observations

Yongliang Zhang, Larry J. Paxton, W. H. Swartz, Sam Yee
Geophysical Research Letters
Ionosphere and magnetosphere dynamics
article

Impact of the 1 April 2026 Artemis II Rocket Launch on the Upper Atmosphere: TIMED/GUVI Observations

Yongliang Zhang, Larry J. Paxton, W. H. Swartz, Sam Yee
article en

Abstract

Abstract The NASA Artemis II rocket was successfully launched at 06:35 p.m. ET (22:35 UTC) on 1 April 2026 from the Kennedy Space Center (28°35′28″N 80°39′03″W). The rocket plume caused enhanced Lyman α emission (up to ∼3 kR) observed by TIMED/GUVI on 2–6 April (5 days). Its peak intensity decreased linearly from April 3 at a rate ∼740 R/day. The half‐maximum width of the zonal Lyman α intensities at 20°–30° latitude (at ∼01:30 p.m. local solar time) increased from ∼3,000 km on April 2–∼9,000 km on April 6. GUVI also detected significant reductions in O‐130.4 nm and O‐135.6 nm radiances, indicating O density reduction. Weakly enhanced NO ε band intensity (NO density) was also observed on April 2 and 3. These features are due to photochemical processes associated with water vapor in the rocket plume and diffusion.

Geophysical Research LettersVol. 53(20)
Johns Hopkins University Applied Physics Laboratory (US)
National Aeronautics and Space Administration, NASA Headquarters
Openalex Percentile: Top 14%
Ionosphere and magnetosphere dynamics
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