Status of OCO-2 and OCO-3: Minutes from the August 3, 2021 OCO-2/OCO-3 Science Team Telecon
No abstract provided
SEARCH · Engineering Papers
Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
Quote a phrase for an exact phrase match. Source license links do not imply unrestricted reuse.
No abstract provided
No abstract provided
No abstract provided
No abstract provided
No abstract provided
No abstract provided
No abstract provided
No abstract provided
No abstract provided
No abstract provided
No abstract provided
No abstract provided
Explore the source record for details and available documents.
This report summarizes radar measurement data of the orbital debris (OD) environment in low Earth orbit (LEO) from the Haystack Ultrawideband Satellite Imaging Radar (HUSIR) operated by the Massachusetts Institute of Technology’s Lincoln Laboratory (MIT/LL) and provided to the National Aeronautics and Space Administration (NASA) Orbital Debris Program Office (ODPO).
This document presents the results of a series of studies performed to develop data-driven rupture limit equations and ballistic limit equations for composite overwrapped pressure vessels. These equations can be used to differentiate between impact conditions that would result in only a small hole or crack from those that would cause catastrophic tank failure. This information would be useful in selecting tank materials to avoid catastrophic tank failure in the event of a perforating on-orbit micrometeoroid or orbital debris particle impact.
Since its creation in 1999, the International VLBI Service for Geodesy and Astrometry (IVS) has documented its progress and current status in the form of annual or biennial reports. The first sixteen years were recorded in the form of annual reports. Starting in 2015/2016 the cadence was changed to two years; hence, this Biennial Report marks eight years of using the two-yearly reporting scheme. The general structure of the reporting has remained stable over the years: the individual components of the IVS contributed short reports describing their numerous activities, progress, and future plans. Without the continued input from the VLBI groups of the international geodetic and astrometric community, this publication could not be compiled and the IVS itself would not be able to flourish. So, once again many thanks to all IVS components who contributed to this Biennial Report
Explore the source record for details and available documents.