Abstract

An instrument package for remotely measuring thermospheric, exospheric, and plasmaspheric structure and composition is described. This instrument will be flown aboard the second test flight of the Black Brant XII rocket, with an expected apogee of approximately 1300 km. A description is given of the experiment package designed for this flight, which consists of a spectrophotometer to measure He I 584 AA, O II 834 AA, O I 989 AA, hydrogen Lyman beta (1025 AA), hydrogen Lyman alpha (1216 AA), and O I 1304 AA transitions, and a photometer to measure the He II 304 AA emission. The He II 304 AA photometer consists of a layered synthetic microstructure (LSM) mirror tuned at 304 AA to focus incidence radiation onto a Channeltron detector. The high altitude to be attained by the rocket is ideally suited to probe the coupling of the various atmospheric regions through the simultaneous measurement of the altitude distributions of several major thermospheric, ionospheric, and exospheric constituents.< <ETX xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink">&gt;</ETX>

Full Text
Paper version not known

Talk to us

Join us for a 30 min session where you can share your feedback and ask us any queries you have

Schedule a call

Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.