The Atacama Large Millimetre/submillimetre Array (ALMA) is the world’s largest ground-based facility for observations at millimeter/submillimeter wavelengths. Inaugurated in March 2013, ALMA has already accomplished ten years of continued steady-state operations. It comprises 66 antennas located approximately 5000 meters at the Chajnantor Plateau in the Atacama Desert in Northern Chile. The ALMA partnership established the ALMA 2030 development program to improve ALMA’s capability to avoid obsolescence for the next decade. The Wideband Sensitivity Upgrade (WSU) project, the first initiative of the ALMA 2030 development program, will replace the entire digital processing system, which includes the wideband digitizers, data transmission system, and data correlation system. A working group was charged to develop a WSU Deployment Concept based on a parallel deployment approach to minimize scientific downtime during the upgrade period, which could last up to five years. In this paper, the authors present the relevant aspects of this analysis and conclusions, which will pave the road to address the definition of the AIVC concept and the corresponding AIVC plan of the WSU project.
Access to the requested content is limited to institutions that have purchased or subscribe to SPIE eBooks.
You are receiving this notice because your organization may not have SPIE eBooks access.*
*Shibboleth/Open Athens users─please
sign in
to access your institution's subscriptions.
To obtain this item, you may purchase the complete book in print or electronic format on
SPIE.org.
INSTITUTIONAL Select your institution to access the SPIE Digital Library.
PERSONAL Sign in with your SPIE account to access your personal subscriptions or to use specific features such as save to my library, sign up for alerts, save searches, etc.