70 likes | 169 Views
Antarctic Space Sciences Workshop. South Pole Station. Some Highlights Several new experiments/instruments planned Mesospheric temperature mapping Sodium allsky imager VLF beacon Some Problems B2 not optimal for optical experiments
E N D
South Pole Station • Some Highlights • Several new experiments/instruments planned • Mesospheric temperature mapping • Sodium allsky imager • VLF beacon • Some Problems • B2 not optimal for optical experiments • Interference documented in many experiments (e.g., ULF-HF) • ARO facility at capacity • Potential Solutions • New space science building (remote facility) • Single facility? • Multiple buildings? • What is the future use of ARO facility at Pole?
South Pole Station • Sector Management • What is needed? • How should we proceed? • What can we learn from the astronomy groups? • Space Science Consortium • Umbrella group? • Funds for meetings and coordinated management etc. • Web portal: http://www.antarcticspacescience.org
South Pole Station • Future science goals and directions at Pole • AMISR? • SuperDARN? • VLF beacon • Mesospheric temperature mapping • Sodium allsky imager • What is left unattended at South Pole? • What are some common goals of the South Pole community? • Synergy of experiments and instruments
McMurdo/Palmer/Field • McMurdo AMISR? • Conjugate with AMISR at Resolute Bay? • How do we move forward on this? • What is left unattended yet in the Antarctic projects? • What are the goals of observing certain upper atmospheric and geospace parameters at Pole, at McMurdo, at Palmer, and over the Antarctic Plateau. • The Space Sciences community should identify the needs for particular instruments (or systems of detectors) at certain locations over the continent. • For example, if a SuperDARN radar at McMurdo is constructed, would we need another radar at Pole or somewhere else - e.g., Palmer?
McMurdo/Palmer/Field • What are the needs over the Plateau and in West Antarctica? • PENGUIn • WAIS • Low power autonomous magnetometers • Low power autonomous VLF receivers • Active Magnetospheric Probing Facility(Stanford University) • What is the next step? • International workshop? • What could be proposed in the "research corridor" between McMurdo and South Pole along the snow traverse route, including WiFi infrastructure for the technology development support and for science projects? • Long term data archiving • CEDAR model?
Wrap Up — Moving Forward • We need to produce a white paper/report to be submitted to NSF • Identify a cohesive and collaborative program for the next 5 years • Recommendations • Costs and funding model for instrument operations