Abstract
Large spherical balloons are a promising new option for deploying extremely large, yet light-weight mirrors for stratospheric and space-based applications. However, their lack of a rigid, precise structure presents a unique challenge for optically correcting nonspherical distortions, particularly at shorter wavelengths. In this paper, we present the design and characterization of a lab prototype for a 10-m aperture telescope for observing the water vapor emission line at 538 mum (557 GHz), as well as considerations for future flight-worthy versions.
| Original language | English (US) |
|---|---|
| Article number | 8721068 |
| Pages (from-to) | 409-416 |
| Number of pages | 8 |
| Journal | IEEE Transactions on Terahertz Science and Technology |
| Volume | 9 |
| Issue number | 4 |
| DOIs | |
| State | Published - Jul 2019 |
Keywords
- Antennas and propagation
- control systems
- optical control
- radio astronomy
ASJC Scopus subject areas
- Radiation
- Electrical and Electronic Engineering
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