Using a civilian telescope to observe solar power generation

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6 FAQs about [Using a civilian telescope to observe solar power generation]
Why do remote and off-grid telescopes emit a lot of energy?
The operational emissions of remote and off-grid telescopes primarily stem from their reliance on fossil fuel generators to meet their energy needs. This demand of mainly electrical energy is needed to power the dish motors and supply the cryogenic cooling for the instruments.
What is the Astronomical Observatory project?
It is the first astronomical observatory project that includes plans for an off-grid, completely renewable energy system right from its design phase (Klaassen et al. 2020; Ramasawmy et al. 2022). The results of this project will inform future efforts in other remote locations.
How many days a week do telescope workers fly in?
In the operation of telescopes in the Atacama, personnel typically fly in for 8-day shifts, after which they fly home and are off-duty for 6 days. In the LCI for the maintenance workers, we include one return-trip from Santiago de Chile to the energy system site per week per worker.
Why do we need a multiscale Observatory?
The physics and dynamics of the Sun necessitate a multiscale problem that can only successfully be understood with improvements to observations of solar activity. With each new mission or telescope, improved spatial and temporal resolution leads to new discoveries.
How much energy does the ATLAST telescope need?
The AtLAST telescope, which will have a 50-m diameter primary mirror and will operate at both day and night, has an expected daily energy demand of 22 MWh e, which exhibits relative stability on an intraday basis but varies seasonally due to the addition or removal of instruments.
Can a telescope detect high-temperature solar plasma?
High-temperature solar plasma emits radiation primarily at EUV and x-ray wavelengths, which must be observed from space. But no conventional reflecting telescope has been fabricated with the extreme accuracy and smoothness necessary to achieve diffraction-limited imaging at those wavelengths.
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