Physics
Scientific paper
Dec 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011agufmsa31a1956b&link_type=abstract
American Geophysical Union, Fall Meeting 2011, abstract #SA31A-1956
Physics
[0310] Atmospheric Composition And Structure / Airglow And Aurora, [2439] Ionosphere / Ionospheric Irregularities, [2494] Ionosphere / Instruments And Techniques, [7999] Space Weather / General Or Miscellaneous
Scientific paper
Ionospheric irregularities, also known as ionospheric bubbles, are transient features of the low and middle latitude ionosphere with important implications for operational systems. Understanding irregularity formation, development, and evolution is vital for efforts within NASA and DoD to forecast scintillation. Irregularity structures have been studied primarily using ground-based systems, though some spaced-based remote and in-situ sensing has been performed. An ionospheric observatory aboard the International Space Station (ISS) would provide new capability to study low- and mid-latitude ionospheric structures on a global scale. By combining for the first time high-sensitivity in-track photometry with vertical ionospheric airglow spectrographic imagery, we demonstrate that high-fidelity optical tomographic reconstruction of bubbles can be performed from the ISS. Ground-based imagery can supplement the tomography by providing all-sky images of ionospheric structures (e.g. bubbles and TIDs) and of signatures of lower atmospheric dynamics, such as gravity waves, that may play a role in irregularity formation. The optical instrumentation can be augmented with additional sensors to provide measurements of scintillation and in situ plasma density, composition, and drifts.
Budzien Scott A.
Chakrabarti Sangeeta
Chua Damien H.
Coker Clayton
Dymond Kenneth
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