@proceedings {1051,
	title = {CINEMA/MOVIE - A NASA research mission to study the Earth{\textquoteright}s magnetic tail, and its conjugate Citizen Science},
	year = {2026},
	month = {03/2026},
	publisher = {HamSCI},
	address = {Newington, CT},
	abstract = {<p>CINEMA is a NASA mission of 9 spacecraft in Low-Earth Orbit, recently approved to move into development, to study the Earth{\textquoteright}s magnetic tail by detecting particles that are accelerated to the poles.\&nbsp; MOVIE is its conjugate Citizen Science initiative, part of which includes building out ground instruments to compliment the main mission, expected to include All-Sky Cameras, Magnetometers, and various Radio Receivers to probe the coinciding ionospheric conditions.</p>
},
	author = {Michael Hartinger and Robyn Millan and Nathaniel Frissell and Kristina Collins and David G. McGaw}
}
@conference {544,
	title = {HamSCI Personal Space Weather: Architecture and Applications to Radio Astronomy},
	booktitle = {Annual (Summer) Eastern Conference},
	year = {2021},
	month = {07/2021},
	publisher = {Society of Amateur Radio Astronomers (SARA)},
	organization = {Society of Amateur Radio Astronomers (SARA)},
	address = {Virtual},
	abstract = {<p>The Ham Radio Science Citizen Investigation (HamSCI) Personal Space Weather Station (PSWS) project is a citizen science initiative to develop a new modular set of ground-based instrumentation for the purpose of studying the structure and dynamics of the terrestrial ionosphere, as well as the larger, coupled geospace system. PSWS system instrumentation includes radio receivers sensitive to frequencies ranging from the very low frequency (VLF) through very high frequency (VHF) bands, a Global Navigation Satellite System (GNSS) receiver to provide Total Electron Content (TEC) measurements and serve as a precision time and frequency reference, and a ground magnetometer sensitive to ionospheric and geospace currents. Although the PSWS is designed primarily for space weather and space science, its modular and open design in both hardware and software allows for a variety of use cases. The core radio instrument of the PSWS, the TangerineSDR, is a wideband, direct sampling 100~kHz to 60~MHz field programmable gate array (FPGA)-based software defined radio (SDR) receiver with direct applicability to radio astronomy. In this paper, we describe the PSWS and TangerineSDR architecture, show examples of how the TangerineSDR could be used to observe Jovian decametric emission, and discuss the applicability of the TangerineSDR to radio astronomy in general.</p>
},
	url = {https://rasdr.org/store/books/books/journals/proceedings-of-annual-conference},
	author = {Nathaniel A. Frissell and Scott H. Cowling and Thomas C. McDermott and John Ackermann and David Typinski and William D. Engelke and David R. Larsen and David G. McGaw and Hyomin Kim and David M. Witten, II and Julius M. Madey and Kristina V. Collins and John C. Gibbons and David Kazdan and Aidan Montare and Dev Raj Joshi and Veronica I. Romanek and Cuong D. Nguyen and Stephen A. Cerwin and William Liles and Jonathan D. Rizzo and Ethan S. Miller and Juha Vierinen and Philip J. Erickson and Mary Lou West}
}
