TY - Generic T1 - HamSCI 2024 Day 1 Closing Remarks T2 - HamSCI Workshop 2024 Y1 - 2024 A1 - Nathaniel A. Frissell JF - HamSCI Workshop 2024 PB - HamSCI ER - TY - Generic T1 - HamSCI 2024 Day 1 Welcome and Opening Remarks T2 - HamSCI Workshop 2024 Y1 - 2024 A1 - Nathaniel A. Frissell JF - HamSCI Workshop 2024 PB - HamSCI CY - Cleveland, OH ER - TY - Generic T1 - HamSCI 2024 Day 2 Welcome and Opening Remarks T2 - HamSCI Workshop 2024 Y1 - 2024 A1 - Nathaniel A. Frissell JF - HamSCI Workshop 2024 PB - HamSCI CY - Cleveland, OH ER - TY - Generic T1 - High Frequency Raytracing for Studying the Ionosphere and Radio Propagation (Invited Tutorial) T2 - HamSCI Workshop 2024 Y1 - 2024 A1 - Katherine Zawdie AB -

High Frequency (HF) raytracing is a tool to study the propagation of HF radio waves through the ionosphere. This presentation will cover the basics of raytracing, including typical inputs and outputs. We will review the different physics that may be included in the raytracer and how changes in the ionosphere may affect the radio wave propagation. A brief description of how to use a raytracer for common applications will be provided. The applicable frequency ranges and limitations of this technique will be also discussed.

JF - HamSCI Workshop 2024 PB - HamSCI CY - Cleveland, OH ER - TY - Generic T1 - High Resolution WSPR Transmissions for Ionospheric Research T2 - HamSCI Workshop 2024 Y1 - 2024 A1 - Rob Robinett A1 - Paul M. Elliott AB -

There are currently over 4000 HAM radio stations worldwide continuously transmitting and receiving beacon signals using the WSPR RF modulation format.  WSPR is implemented in the open source WSJT-x application program authored by Nobel Laureate Joe Taylor and a large group of contributors. Recent software enhancements to WSJT-x and newly available low-cost transmit and receive hardware using GPS disciplined oscillators permit records of these transmissions (known as ‘spots’) to be used to study ionospheric events like Travelling Ionospheric Disturbances. Records of those 3 million+ receptions per day are publicly available to all researchers and citizen scientists in a SQL database which ensures access for all. In this presentation we give an introduction to WSPR, the publicly available databases where the ‘spots’ are stored.  Also included are websites with text, map and graphical outputs which allow easy queries about ’spots’ and examples of low cost research quality transmitters and receivers which are in operation.

JF - HamSCI Workshop 2024 ER - TY - Generic T1 - The Ham Radio Project: Exploring the Electromagnetic Spectrum (Invited Tutorial) T2 - HamSCI Workshop 2023 Y1 - 2023 A1 - Jesse Alexander AB -

The National Radio Astronomy Observatory (NRAO) recently received funding from ARDC for a new 2-year project designed to teach young adults about the electromagnetic spectrum while sharing the excitement of amateur (ham) radio among BIPOC and LGBTQIA+ students. The project goals are to: Introduce students to the Electromagnetic Spectrum and radio technologies; develop a scalable, shareable curriculum via SuperKnova; provide hands-on activities to deepen subject knowledge, and support student attainment of Technician and General Class Amateur Radio Licenses.

JF - HamSCI Workshop 2023 PB - HamSCI CY - Scranton, PA ER - TY - Generic T1 - HamSCI 2023 Day 1 Welcome and Opening Remarks T2 - HamSCI Workshop 2023 Y1 - 2023 A1 - Nathaniel Frissell JF - HamSCI Workshop 2023 PB - HamSCI CY - Scranton, PA ER - TY - Generic T1 - HamSCI 2023 Day 2 Welcome and Opening Remarks T2 - HamSCI Workshop 2023 Y1 - 2023 A1 - Nathaniel A. Frissell JF - HamSCI Workshop 2023 PB - HamSCI CY - Scranton, PA ER - TY - Generic T1 - HamSCI: Continuing a Long Tradition of Amateur Radio Citizen Science T2 - HamSCI Workshop 2023 Y1 - 2023 A1 - Robert Reif AB -

In 1957, 1958 I was a high school student, and only an amateur radio operator for two years when I joined the American Radio Relay League (ARRL) Propagation Research Project. This ARRL program was supported by the Air Force and collected information on Ionospheric VHF radio propagation from reports by radio amateurs.  The program was part of the 1957, 1958 International Geophysical Year (IGY). This was a world wide program to study the Earth.  It involved scientists from 67 countries and made many contributions to our knowledge of Earth. The ionosphere was one of the subjects or study. The American Radio Relay League (ARRL), in cooperation with the US Air Force, set up a program to collect observation reports from radio amateurs of unusual propagation on frequency bands of 50 MHz and above. I was happy and proud to be one of these amateur stations. In reflection of the more that 60 years since, I am certain that this early experience in the ham science (HamSCI) of the 1950s was part of my decision to follow a carrier in science and engineering. A carrier that included the Apollo program at one end and the Space Shuttle program at the other. I want to point out that an early experience in science and technology as a young radio amateur can and did lead to successful and exciting carrier.

JF - HamSCI Workshop 2023 PB - HamSCI CY - Scranton, PA ER - TY - MGZN T1 - HamSCI Workshop 2023: A Radio Science Collaboration Y1 - 2023 A1 - Mikitin, G AB -
More than 150 space physics researchers, educators, engineers, college students, licensed amateurs, and members of the Ham Radio Science Citizen Investigation (HamSCI) community came together at the sixth annual HamSCI Workshop on March 17 – 18, 2023, where they listened, learned, and contributed to scientific investigations involving the Earth’s ionosphere and magnetosphere. This year’s workshop was presented by The University of Scranton, and it emphasized cooperation between HamSCI’s professional science community and its volunteer citizen scientists, many of whom are active amateur radio operators.
JF - QST VL - 107 UR - https://www.arrl.org/qst IS - 10 ER - TY - JOUR T1 - Heliophysics and amateur radio: citizen science collaborations for atmospheric, ionospheric, and space physics research and operations JF - Frontiers in Astronomy and Space Sciences Y1 - 2023 A1 - Frissell, Nathaniel A. A1 - Ackermann, John R. A1 - Alexander, Jesse N. A1 - Benedict, Robert L. A1 - Blackwell, William C. A1 - Boedicker, Rachel K. A1 - Cerwin, Stephen A. A1 - Collins, Kristina V. A1 - Cowling, Scott H. A1 - Deacon, Chris A1 - Diehl, Devin M. A1 - Di Mare, Francesca A1 - Duffy, Timothy J. A1 - Edson, Laura Brandt A1 - Engelke, William D. A1 - Farmer, James O. A1 - Frissell, Rachel M. A1 - Gerzoff, Robert B. A1 - Gibbons, John A1 - Griffiths, Gwyn A1 - Holm, Sverre A1 - Howell, Frank M. A1 - Kaeppler, Stephen R. A1 - Kavanagh, George A1 - Kazdan, David A1 - Kim, Hyomin A1 - Larsen, David R. A1 - Ledvina, Vincent E. A1 - Liles, William A1 - Lo, Sam A1 - Lombardi, Michael A. A1 - MacDonald, Elizabeth A. A1 - Madey, Julius A1 - McDermott, Thomas C. A1 - McGaw, David G. A1 - McGwier, Robert W. A1 - Mikitin, Gary A. A1 - Miller, Ethan S. A1 - Mitchell, Cathryn A1 - Montare, Aidan A1 - Nguyen, Cuong D. A1 - Nordberg, Peter N. A1 - Perry, Gareth W. A1 - Piccini, Gerard N. A1 - Pozerski, Stanley W. A1 - Reif, Robert H. A1 - Rizzo, Jonathan D. A1 - Robinett, Robert S. A1 - Romanek, Veronica I. A1 - Sami, Simal A1 - Sanchez, Diego F. A1 - Sarwar, Muhammad Shaaf A1 - Schwartz, Jay A. A1 - Serra, H. Lawrence A1 - Silver, H. Ward A1 - Skov, Tamitha Mulligan A1 - Swartz, David A. A1 - Themens, David R. A1 - Tholley, Francis H. A1 - West, Mary Lou A1 - Wilcox, Ronald C. A1 - Witten, David A1 - Witvliet, Ben A. A1 - Yadav, Nisha AB -

The amateur radio community is a global, highly engaged, and technical community with an intense interest in space weather, its underlying physics, and how it impacts radio communications. The large-scale observational capabilities of distributed instrumentation fielded by amateur radio operators and radio science enthusiasts offers a tremendous opportunity to advance the fields of heliophysics, radio science, and space weather. Well-established amateur radio networks like the RBN, WSPRNet, and PSKReporter already provide rich, ever-growing, long-term data of bottomside ionospheric observations. Up-and-coming purpose-built citizen science networks, and their associated novel instruments, offer opportunities for citizen scientists, professional researchers, and industry to field networks for specific science questions and operational needs. Here, we discuss the scientific and technical capabilities of the global amateur radio community, review methods of collaboration between the amateur radio and professional scientific community, and review recent peer-reviewed studies that have made use of amateur radio data and methods. Finally, we present recommendations submitted to the U.S. National Academy of Science Decadal Survey for Solar and Space Physics (Heliophysics) 2024–2033 for using amateur radio to further advance heliophysics and for fostering deeper collaborations between the professional science and amateur radio communities. Technical recommendations include increasing support for distributed instrumentation fielded by amateur radio operators and citizen scientists, developing novel transmissions of RF signals that can be used in citizen science experiments, developing new amateur radio modes that simultaneously allow for communications and ionospheric sounding, and formally incorporating the amateur radio community and its observational assets into the Space Weather R2O2R framework. Collaborative recommendations include allocating resources for amateur radio citizen science research projects and activities, developing amateur radio research and educational activities in collaboration with leading organizations within the amateur radio community, facilitating communication and collegiality between professional researchers and amateurs, ensuring that proposed projects are of a mutual benefit to both the professional research and amateur radio communities, and working towards diverse, equitable, and inclusive communities.

VL - 10 UR - https://www.frontiersin.org/articles/10.3389/fspas.2023.1184171/fullhttps://www.frontiersin.org/articles/10.3389/fspas.2023.1184171/full JO - Front. Astron. Space Sci. ER - TY - Generic T1 - History of the Art of DXing and Contesting T2 - HamSCI Workshop 2023 Y1 - 2023 A1 - Ron Wilcox AB -

Rich in the history of amateur or ham radio is the art of DXing and contesting. DXing is short for distance. A DXpedition is a trip to operate in a rare location or country. Contests involve hundreds to thousands of operators attempting to “work” or contact as many operators of a defined criteria as possible. These DXer’s and contesters are generally very skilled. These skills involve “pulling out” a single call sign out of a cacophony of dozens to hundreds of call signs, being able to hear and understand very weak signals, and being able to receive and transmit information rapidly and accurately. These operators have simple to large, advanced antenna systems, and equipment ranging from analog and tubes to state-of-the-art software defined radios (SDRs). They are a valuable resource to gathering data, as for example in the eclipse of 2017 and looking forward, to the eclipses of 2023 and 2024. How this all started is an important and fascinating part of ham radio history. This presentation will, in a humorous and personal way, present four important pioneers and tell their story, with their impact and influence. We will cover from the early 1900’s to the early 1960’s.

JF - HamSCI Workshop 2023 PB - HamSCI CY - Scranton, PA ER - TY - Generic T1 - How Do I Talk From Scranton to Pakistan Using​ High Frequency Amateur Radio?​ T2 - HamSCI Workshop 2023 Y1 - 2023 A1 - Zainab Shah A1 - Gwyn Griffiths A1 - Rob Robinett A1 - Nathaniel Frissell AB -

This poster will demonstrate the possible ways to send propagation transmissions from The University of Scranton to Karachi, Pakistan. To do this, VOACAP will be used to map out possible paths and peak times for transmission and then WSRP.rocks will be used to compare the empirical VOACAP model outputs to observed data. A recommendation will then be made for the optimal time and frequency to communicate using high frequency (HF) radio between Scranton, PA and Karachi, Pakistan.

JF - HamSCI Workshop 2023 PB - HamSCI CY - Scranton, PA ER - TY - Generic T1 - Ham Radio and the Discovery of the Ionosphere (Keynote) T2 - HamSCI Workshop 2022 Y1 - 2022 A1 - Chen-Pang Yeang AB -

Ham radio's involvement in the discovery of the ionosphere during the early 20th century constitutes a core part of the radio amateur community's collective memory. I will review this episode in a broader historical context. Why radio waves could propagate over long distances along the earth's curvature had been debated since the invention of wireless telegraphy in the late 1890s. By the 1910s, physicists' consensus was that radio waves bounced back from an electrically conductive surface in the upper sky known as the "Kennelly-Heaviside layer." Meanwhile, electrical engineers' empirical studies led to the so-called "Austin-Cohen formula" that predicted a decrease of propagating range with wavelength, implying that transoceanic or transcontinental wireless communication could only be achieved at wavelengths longer than 200 m. Despite these scientific convictions, the American Radio Relay League (ARRL) and its sister organizations in the UK and France in the 1920s embarked large-scale collective experiments for transatlantic wireless signal transmission at wavelengths shorter than 200 m. Their success challenged the Austin-Cohen formula. In addition, ARRL members collaborated with US naval researchers to experiment with medium-range radio-wave propagation. Their studies resulted in the identification of the skip zone—that radio signals disappeared at certain distances from a transmitter but emerged again at a further range. These findings from radio amateurs’ activities paved a crucial ground for the British and American scientists Edward Appleton, Miles Barnett, Gregory Breit, and Merle Tuve to perform radio experiments that provided direct evidence for the ionosphere—a more complex geophysical entity than the Kennelly-Heaviside layer. In this talk, I will examine the radio amateurs' collective experiments in the discovery of the ionosphere. I will also discuss the implications of this form of collaboration to ham radio's later collective technical activities and engagements with "citizen science."

JF - HamSCI Workshop 2022 PB - HamSCI CY - Huntsville, AL ER - TY - Generic T1 - HamSCI Plans for the Study of the 2023 and 2024 Solar Eclipse Impacts on Radio and the Ionosphere T2 - Dayton Hamvention Y1 - 2022 A1 - Nathaniel A. Frissell JF - Dayton Hamvention PB - Dayton Amateur Radio Association CY - Xenia, OH UR - https://hamsci.org/publications/hamsci-plans-study-2023-and-2024-solar-eclipse-impacts-radio-and-ionosphere ER - TY - Generic T1 - Hardware Design of the Grape2 Data Collection Sequencing Engine T2 - HamSCI Workshop 2022 Y1 - 2022 A1 - John Gibbons AB -

A review of the design process for the creation of the sequencing logic to drive the data acquisition system on the Grape 2 analog data collection engine.  Design requirements and trade-offs between different design techniques will be discussed.  The design process from requirements , flow chart and finally to hardware implementation will be reviewed.  Final implementation will be demonstrated with the aid of a logic analyzer.

JF - HamSCI Workshop 2022 PB - HamSCI CY - Huntsville, AL ER - TY - Generic T1 - HF Doppler Observations of Traveling Ionospheric Disturbances in a WWV Signal Received with a Network of Low Cost HamSCI Personal Space Weather Stations T2 - HamSCI Workshop 2022 Y1 - 2022 A1 - Veronica Romanek A1 - Nathaniel A. Frissell A1 - William Liles A1 - John Gibbons A1 - Kristina V. Collins AB -

Traveling Ionospheric Disturbances (TIDs) are quasi-periodic variations in ionospheric electron density that are often associated with atmospheric gravity waves. TIDs cause amplitude and frequency variations in high frequency (HF, 3 30 MHz) refracted radio waves. The authors present an analysis of observations of TIDs made with Ham Radio Science Citizen Investigation ( HamSCI ) Low Cost Personal Space Weather Stations (PSWS) located in Northwestern New Jersey and near Cleveland, Ohio. The TIDs were detected in the Doppler shifted carrier of the received signal from the 10 MHz WWV frequency and time standard station in Fort Collins, CO. Using a lagged cross correlation analysis, we demonstrate a method for determining TID wavelength, direction, and period using the collected WWV HF Doppler shifted data.

JF - HamSCI Workshop 2022 PB - HamSCI CY - Huntsville, AL ER - TY - MGZN T1 - Ham Radio Creates a Planet-Sized Space Weather Sensor Network Y1 - 2021 A1 - Kristina V. Collins A1 - David Kazdan A1 - Nathaniel Frissell JF - QST VL - 105 UR - https://www.arrl.org/qst IS - 8 ER - TY - JOUR T1 - Ham Radio Forms a Planet-Sized Space Weather Sensor Network JF - Eos Y1 - 2021 A1 - Collins, Kristina A1 - Kazdan, David A1 - Frissell, Nathaniel VL - 102 UR - https://eos.org/features/ham-radio-forms-a-planet-sized-space-weather-sensor-network JO - Eos ER - TY - CONF T1 - HamSCI Campaign Co-Design (Panel Discussion) T2 - HamSCI Workshop 2021 Y1 - 2021 A1 - Kristina V. Collins A1 - Nathaniel A. Frissell A1 - Philip J. Erickson A1 - Laura Brandt A1 - Elizabeth MacDonald A1 - Michael Black A1 - Gareth Perry JF - HamSCI Workshop 2021 PB - HamSCI CY - Virtual ER - TY - Generic T1 - HamSCI: Ham Radio Science Citizen Investigation T2 - ISWAT Meeting Y1 - 2021 A1 - Frissell, Nathaniel A. A1 - Sanchez, Diego A1 - Perry, Gareth W. A1 - Kaeppler, Stephen R. A1 - Joshi, Dev Raj A1 - Engelke, William D. A1 - Thomas, Evan G. A1 - Coster, Anthea J. A1 - Erickson, Philip J. A1 - Ruohoniemi, J. Michael A1 - Baker, Joseph B. H. A1 - Gerzoff, Robert JF - ISWAT Meeting PB - International Space Weather Action Team (ISWAT) CY - Virtual ER - TY - CONF T1 - HamSCI Personal Space Weather: Architecture and Applications to Radio Astronomy T2 - Annual (Summer) Eastern Conference Y1 - 2021 A1 - Nathaniel A. Frissell A1 - Scott H. Cowling A1 - Thomas C. McDermott A1 - John Ackermann A1 - David Typinski A1 - William D. Engelke A1 - David R. Larsen A1 - David G. McGaw A1 - Hyomin Kim A1 - David M. Witten, II A1 - Julius M. Madey A1 - Kristina V. Collins A1 - John C. Gibbons A1 - David Kazdan A1 - Aidan Montare A1 - Dev Raj Joshi A1 - Veronica I. Romanek A1 - Cuong D. Nguyen A1 - Stephen A. Cerwin A1 - William Liles A1 - Jonathan D. Rizzo A1 - Ethan S. Miller A1 - Juha Vierinen A1 - Philip J. Erickson A1 - Mary Lou West AB -

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.

JF - Annual (Summer) Eastern Conference PB - Society of Amateur Radio Astronomers (SARA) CY - Virtual UR - https://rasdr.org/store/books/books/journals/proceedings-of-annual-conference ER - TY - CONF T1 - HamSCI Personal Space Weather Station (PSWS): Architecture and Current Status T2 - NSF CEDAR (Coupling, Energetics, and Dynamics of Atmospheric Regions) Y1 - 2021 A1 - Nathaniel A. Frissell A1 - Dev Joshi A1 - Veronica I. Romanek A1 - Kristina V. Collins A1 - Aidan Montare A1 - David Kazdan A1 - John Gibbons A1 - William D. Engelke A1 - Travis Atkison A1 - Hyomin Kim A1 - Scott H. Cowling A1 - Thomas C. McDermott A1 - John Ackermann A1 - David Witten A1 - Julius Madey A1 - H. Ward Silver A1 - William Liles A1 - Steven Cerwin A1 - Philip J. Erickson A1 - Ethan S. Miller A1 - Juha Vierinen AB -

Recent advances in geospace remote sensing have shown that large-scale distributed networks of ground-based sensors pay large dividends by providing a big picture view of phenomena that were previously observed only by point-measurements. While existing instrument networks provide excellent insight into ionospheric and space science, the system remains undersampled and more observations are needed to advance understanding. In an effort to generate these additional measurements, the Ham Radio Science Citizen Investigation (HamSCI, hamsci.org) is working with the Tucson Amateur Packet Radio Corporation (TAPR, tapr.org), an engineering organization comprised of volunteer amateur radio operators and engineers, to develop a network of Personal Space Weather Stations (PSWS). These instruments that will provide scientific-grade observations of signals-of-opportunity across the HF bands from volunteer citizen observers as part of the NSF Distributed Array of Small Instruments (DASI) program. A performance-driven PSWS design (~US$500) will be a modular, multi-instrument device that will consist of a dual-channel phase-locked 0.1-60 MHz software defined radio (SDR) receiver, a ground magnetometer with (~10 nT resolution and 1-sec cadence), and GPS/GNSS receiver to provide precision time stamping and serve as a GPS disciplined oscillator (GPSDO) to provide stability to the SDR receiver. A low-cost PSWS (< US$100) that measures Doppler shift of HF signals received from standards stations such as WWV (US) and CHU (Canada) and includes a magnetometer is also being developed. HF sounding algorithms making use of signals of opportunity will be developed for the SDR-based PSWS. All measurements will be collected into a central database for coordinated analysis and made available for public access.

JF - NSF CEDAR (Coupling, Energetics, and Dynamics of Atmospheric Regions) PB - CEDAR CY - Virtual ER - TY - Generic T1 - HamSCI Personal Space Weather Station (PSWS): Fall 2021 Update T2 - TAPR-ARRL Digital Communications Conference Y1 - 2021 A1 - Frissell, Nathaniel A. A1 - Joshi, Dev Raj A1 - Collins, Kristina A1 - Montare Aidan A1 - Kazdan, David A1 - Engelke, William D. A1 - Atkison, Travis A1 - Kim, Hyomin A1 - Cowling, Scott H. A1 - McDermott, Thomas C. A1 - Ackermann, John A1 - Witten, David A1 - Madey, Jules A1 - Silver, H. Ward A1 - Liles, W. A1 - Cerwin, Stephen A. A1 - Erickson, Phillip J. A1 - Miller, Ethan S, A1 - Vierinen, Juha JF - TAPR-ARRL Digital Communications Conference PB - ARRL-TAPR CY - Virtual UR - https://youtu.be/MHkz7jNynOg?t=1990 ER - TY - Generic T1 - HamSCI: The Ionosphere from Your Backyard T2 - AMSAT SA Space Symposium Y1 - 2021 A1 - Frissell, Nathaniel A. JF - AMSAT SA Space Symposium PB - AMSAT-SA CY - South Africa (Virtual) ER - TY - Generic T1 - HamSCI: Today’s Community and Future Directions T2 - ARRL-TAPR Digital Communications Conference Y1 - 2021 A1 - Frissell, Nathaniel A. JF - ARRL-TAPR Digital Communications Conference PB - ARRL-TAPR CY - Virtual UR - https://youtu.be/kVY3E3e--_I?t=1512 ER - TY - Generic T1 - Hardware System Update: Data Engine, RF Module, Clock Module, Magnetometer T2 - ARRL-TAPR Digital Communications Conference Y1 - 2021 A1 - Cowling, Scott H. JF - ARRL-TAPR Digital Communications Conference PB - ARRL-TAPR CY - Virtual UR - https://youtu.be/MHkz7jNynOg?t=2886 ER - TY - CONF T1 - HF Doppler Observations of Traveling Ionospheric Disturbances in a WWV Signal Received with a Network of Low-Cost HamSCI Personal Space Weather Stations T2 - NSF CEDAR (Coupling, Energetics, and Dynamics of Atmospheric Regions) Y1 - 2021 A1 - Veronica I. Romanek A1 - Nathaniel A. Frissell A1 - Dev Joshi A1 - William Liles A1 - Clair Trop A1 - Kristina Collins A1 - Gareth Perry AB -

Traveling Ionospheric Disturbances (TIDs) are quasi-periodic variations in ionospheric electron density that are often associated with atmospheric gravity waves. TIDs cause amplitude and frequency variations in high frequency (HF, 3-30 MHz) refracted radio waves. We present observations of TIDs made with a network of Ham Radio Science Citizen Investigation (HamSCI) Low-Cost Personal Space Weather Stations (PSWS) with nodes located in Pennsylvania, New Jersey, and Ohio. The TIDs were detected in the Doppler shifted carrier of the received signal from the 10 MHz WWV frequency and time standard station in Fort Collins, CO. Using a lagged cross correlation analysis, we demonstrate a method for determining TID wavelength, direction, and period using the collected WWV HF Doppler shifted data.

JF - NSF CEDAR (Coupling, Energetics, and Dynamics of Atmospheric Regions) PB - CEDAR CY - Virtual ER - TY - CONF T1 - HF Doppler Observations of Traveling Ionospheric Disturbances in the WWV Signal Received with a Network of Low-Cost HamSCI Personal Space Weather Stations T2 - American Geophysical Union Fall Meeting Y1 - 2021 A1 - Romanek, Veronica I. A1 - Frissell, Nathaniel A. A1 - Joshi, Dev Raj A1 - Liles, William A1 - Trop, Clair A1 - Collins, Kristina A1 - Perry, Gareth W. AB -

Traveling Ionospheric Disturbances (TIDs) are quasi-periodic variations in ionospheric electron density that are often associated with atmospheric gravity waves. TIDs cause amplitude and frequency variations in high frequency (HF, 3-30 MHz) refracted radio waves. We present observations of TIDs made with a network of Ham Radio Science Citizen Investigation (HamSCI) Low-Cost Personal Space Weather Stations (PSWS) with nodes located in Pennsylvania, New Jersey, and Ohio. The TIDs were detected in the Doppler shifted carrier of the received signal from the WWV frequency and time standard station near Fort Collins, CO. Using a lagged cross correlation analysis, we demonstrate a method for determining TID wavelength, direction, and period using the collected WWV HF Doppler shifted data.

JF - American Geophysical Union Fall Meeting PB - American Geophysical Union CY - New Orleans, LA UR - https://agu.confex.com/agu/fm21/meetingapp.cgi/Paper/888443 ER - TY - Generic T1 - HF Doppler Observations of Traveling Ionospheric Disturbances in the WWV Signal Received with a Network of Low-Cost HamSCI Personal Space Weather Stations T2 - ARRL-TAPR Digital Communications Conference Y1 - 2021 A1 - Romanek, Veronica I. A1 - Frissell, Nathaniel A. A1 - Joshi, Dev Raj A1 - Liles, William A1 - Trop, Claire A1 - Collins, Kristina A1 - Perry, Gareth W. JF - ARRL-TAPR Digital Communications Conference PB - ARRL-TAPR CY - Virtual UR - https://youtu.be/kVY3E3e--_I?t=3495 ER - TY - CONF T1 - HF Doppler Observations of Traveling Ionospheric Disturbances in a WWV Signal Received with a Network of Low-Cost HamSCI Personal Space Weather Stations T2 - Annual (Summer) Eastern Conference Y1 - 2021 A1 - Veronica I. Romanek A1 - Nathaniel A. Frissell A1 - Dev Raj Joshi A1 - William Liles A1 - Claire C. Trop A1 - Kristina V. Collins A1 - Gareth W. Perry AB -

Traveling Ionospheric Disturbances (TIDs) are quasi-periodic variations in ionospheric electron density that are often associated with atmospheric gravity waves. TIDs cause amplitude and frequency variations in high frequency (HF, 3-30 MHz) refracted radio waves. One way to detect TIDs is through the use of a Grape Personal Space Weather Station (PSWS). The Grape PSWS successfully detected TIDs in the Doppler shifted carrier of the received signal from the 10 MHz WWV frequency and time standard station in Fort Collins, CO. This paper will present an explanation of how the Grape PSWS was used to collect data, and how scientist can use this data to further investigate the ionosphere.

JF - Annual (Summer) Eastern Conference PB - Society of Amateur Radio Astronomers (SARA) CY - Virtual UR - https://rasdr.org/store/books/books/journals/proceedings-of-annual-conference ER - TY - Generic T1 - History of Antenna Technology at the Arecibo Observatory, Arecibo Puerto Rico T2 - HamSCI Workshop 2021 Y1 - 2021 A1 - James K. Breakall AB -

The Arecibo Observatory first opened in 1963 and has been a marvel in engineering ever since. It has been a monumental instrument for scientific research in the fields of astronomy, planetary radar, ionospheric probing and HF heating modification, and optical probing of the atmosphere. While the science and the discoveries are well known to many, the antenna technology and engineering are equally as impressive as the discoveries. The original concept, by Prof. William Gordon in the Electrical Engineering Department at Cornell University, was for a 1000 foot parabolic dish aiming only at zenith, with no tracking capability for studies of the ionosphere with the newly developed technique of incoherent scatter radar (ISR). Fortunately, knowledge of some on going research with spherical reflectors was suggested where the feed could be moved to slew the beam. The rest is history that will be the described in this talk up to the collapse. Most of the 430 MHz 96 foot line feed broke off and fell through the dish in 2017 during Hurricane Maria. Then in December 2020, the platform fell into the dish destroying large sections of the dish and the equipment in the platform. There is so much more to tell about the engineering at Arecibo that will be the subject of this presentation at HamSCI 2021. 

 

JF - HamSCI Workshop 2021 PB - HamSCI CY - Scranton, PA (Virtual) UR - https://hamsci2021-uscranton.ipostersessions.com/?s=C9-8F-A9-0F-A8-29-2C-C5-63-16-4B-2E-E7-47-F7-0A ER - TY - CONF T1 - HamSCI Distributed Array of Small Instruments Personal Space Weather Station (DASI-PSWS): Architecture and Current Status (Invited) T2 - NSF CEDAR (Coupling, Energetics, and Dynamics of Atmospheric Regions) Y1 - 2020 A1 - N. A. Frissell A1 - D. Joshi A1 - K. Collins A1 - A. Montare A1 - D. Kazdan A1 - J. Gibbons A1 - S. Mandal A1 - W. Engelke A1 - T. Atkison A1 - H. Kim A1 - A. J. Gerrard A1 - J. S. Vega A1 - S. H. Cowling A1 - T. C. McDermott A1 - J. Ackermann A1 - D. Witten A1 - H. W. Silver A1 - W. Liles A1 - S. Cerwin A1 - P. J. Erickson A1 - E. S. Miller AB -

Recent advances in geospace remote sensing have shown that large-scale distributed networks of ground-based sensors pay large dividends by providing a big picture view of phenomena that were previously observed only by point-measurements. While existing instrument networks provide excellent insight into ionospheric and space science, the system remains undersampled and more observations are needed to advance understanding. In an effort to generate these additional measurements, the Ham Radio Science Citizen Investigation (HamSCI, hamsci.org) is working with the Tucson Amateur Packet Radio Corporation (TAPR, tapr.org), an engineering organization comprised of volunteer amateur radio operators and engineers, to develop a network of Personal Space Weather Stations (PSWS). These instruments that will provide scientific-grade observations of signals-of-opportunity across the HF bands from volunteer citizen observers as part of the NSF Distributed Array of Small Instruments (DASI) program. A performance-driven PSWS design (~US$500) will be a modular, multi-instrument device that will consist of a dual-channel phase-locked 0.1-60 MHz software defined radio (SDR) receiver, a ground magnetometer with (~10 nT resolution and 1-sec cadence), and GPS/GNSS receiver to provide precision time stamping and serve as a GPS disciplined oscillator (GPSDO) to provide stability to the SDR receiver. A low-cost PSWS (< US$100) that measures Doppler shift of HF signals received from standards stations such as WWV (US) and CHU (Canada) and includes a magnetometer is also being developed. HF sounding algorithms making use of signals of opportunity will be developed for the SDR-based PSWS. All measurements will be collected into a central database for coordinated analysis and made available for public access.

JF - NSF CEDAR (Coupling, Energetics, and Dynamics of Atmospheric Regions) CY - Santa Fe, NM (Virtual) UR - http://cedarweb.vsp.ucar.edu/wiki/index.php/2020_Workshop:MainVG ER - TY - Generic T1 - HamSCI PSWS Overview and Status T2 - ARRL-TAPR Digital Communications Conference Y1 - 2020 A1 - Frissell, N. A. JF - ARRL-TAPR Digital Communications Conference PB - ARRL-TAPR CY - Virtual UR - https://www.youtube.com/watch?v=n9p0FpZkxE4 ER - TY - CONF T1 - HamSCI: Space Weather Operational Resources and Needs of the Amateur Radio Community T2 - American Meteorological Society Annual Meeting Y1 - 2020 A1 - Nathaniel A. Frissell A1 - Philip J. Erickson A1 - Ethan S. Miller A1 - William Liles A1 - H. Ward Silver A1 - R. Carl Luetzelschwab A1 - Tamitha Skov AB -

The amateur (ham) radio community is a global community of over 3 million people who use and build radio equipment for communications, experimentation, and science. By definition, amateur radio is a volunteer service, with the operators required to hold government-issued licenses that are typically earned by passing knowledge tests covering radio regulations and practices, radio theory, and electromagnetic theory. In the United States, there are about 750,000 licensed hams, ranging in age from very young to very old, and ranging in experience from neophyte to people with advanced degrees in radio engineering and science. Amateur radio operators are licensed to transmit on bands spread across the radio frequency (RF) spectrum, from very low frequency (VLF) up to hundreds of gigahertz. The purpose of these communications range from mission-critical emergency and public service communications to social contacts to highly competitive contests and achievement award programs. Many of these communications rely on trans-ionospheric paths, and therefore are heavily influenced by conditions in near-Earth space, or space weather.
Amateurs today obtain space weather and propagation prediction information from sources such as the NOAA Space Weather Prediction Center (SWPC), spaceweather.com, the Voice of America Coverage Analysis Program (VOACAP), amateur radio propagation columnists (ARRL, RSGB, and CQ Magazine), and spaceweatherwoman.com (Dr. Tamitha Skov). In order to predict success for their communications efforts, hams often use parameters such as smoothed sunspot number, 10.7 cm wavelength solar flux proxy, and the planetary Kp and Ap indices as inputs to predict radio propagation performance. Traditionally, these predictions focus on the driving influence of space conditions and the sun’s output. However, frontier research in the space sciences community has revealed that for improved predictive success, much more information needs to be provided on neutral atmosphere dynamics from the lower atmosphere and its coupled effects on the ionosphere, and predictions need to be available at higher temporal and spatial resolution. Lower atmospheric influences include atmospheric gravity waves that can couple to traveling ionospheric disturbances that can dramatically alter radio propagation paths. Tropospheric phenomena such as temperature inversions and wind shear also affect VHF and UHF propagation. To be most useful, the ham community needs operational products that provide real time nowcasts and multi-day forecasts which predict how space weather through the whole atmosphere affects radio wave propagation on global scale and at all operational wavelengths.
To help with this effort, hams can provide data with unique spatial and temporal coverage back to the research and forecast community. The amateur radio community has already started this process with the creation of multiple global-scale, real-time propagation reporting systems such as the Weak Signal Propagation Reporting Network (WSPRNet), PSKReporter, and the Reverse Beacon Network (RBN). Studies by the Ham radio Science Citizen Investigation (HamSCI) have shown that data from these systems, if applied correctly, can effectively be used to study ionospheric space weather events. Experienced amateurs keep detailed records of verified point-to-point contacts and have extensive experience operating under a wide variety of geophysical conditions and locations, both of which can provide unique insights when shared with the professional research community. In this presentation, we will describe efforts led by the HamSCI collective to provide this research community feedback through active HamSCI community email lists and annual HamSCI workshops. We will also describe strategies with good initial success at amateur-professional collaboration, including a HamSCI-led amateur radio community - professional research community partnership to create a network of HamSCI Personal Space Weather Stations (PSWS), which will allow citizen scientists to make science-grade space weather observations from their own backyards.

JF - American Meteorological Society Annual Meeting PB - American Meteorological Society Annual Meeting CY - Boston, MA UR - https://ams.confex.com/ams/2020Annual/meetingapp.cgi/Paper/370904 ER - TY - CONF T1 - HamSCI – The Ionosphere from your Backyard T2 - HamCation Y1 - 2020 A1 - Nathaniel A. Frissell JF - HamCation PB - Orlando Amateur Radio Club CY - Orlando, FL ER - TY - MGZN T1 - Hands-On-SDR: TangerineSDR Y1 - 2020 A1 - Scotty Cowling AB -

The inspiration for TangerineSDR came from the HamSCI [8] group as a request for SDR hardware that could be used as a Personal Space Weather Station (PSWS). Their need resulted in the four-hour Sunday seminar at the TAPR Digital Communications Conference in Albuquerque, NM, on September 16, 2018. At TAPR, our first response was, “Let’s find a commercial SDR that we can incorporate into a PSWS kit”. Existing hardware would be our best bet for a quick solution. After some research and further consultation with the scientists at HamSCI, it became clear that there was no affordable (less than US $500) solution that met PSWS requirements. This article explains the TangerineSDR project and requirements.
 

Reprinted with permission; copyright ARRL.

JF - QEX UR - http://www.arrl.org/qex/ ER - TY - Generic T1 - HF Propagation Measurement Techniques and Analyses T2 - ARRL-TAPR Digital Communications Conference Y1 - 2020 A1 - Cerwin, S. JF - ARRL-TAPR Digital Communications Conference PB - ARRL-TAPR CY - Virtual UR - https://www.youtube.com/watch?v=n9p0FpZkxE4 ER - TY - CONF T1 - Ham Radio 2.0 - Science, Service, Skill (Keynote Address) T2 - HamSCI Workshop 2019 Y1 - 2019 A1 - H. Ward Silver AB -

Amateur radio sits at the junction of technology, volunteerism, and craft.  Which of those doors by which you enter the world of ham radio - science, service, skill - colors your expectations and interests, often for life.  Yet the technical and demographic changes sweeping through society have not overlooked amateur radio.  The service faces many challenges to long-held traditions and assumptions.  What tools can we provide to not just meet the challenges but prosper, keeping amateur radio vibrant and enjoyable in order to develop our skills and support our fellow citizens, fulfilling our Basis and Purpose along the way?  Speaking from a technical background to a technical audience, we'll consider both our opportunities and obligations to amateur radio writ large while enjoying a chuckle or two, as well.

JF - HamSCI Workshop 2019 PB - HamSCI CY - Cleveland, OH ER - TY - CONF T1 - Ham Radio for Space Scientists (Invited Tutorial) T2 - HamSCI Workshop 2019 Y1 - 2019 A1 - R. Carl Luetzelschwab AB -

Due to inadvertent interference to commercial and military communications, Amateur Radio operators (hams) were forced to wavelengths of 200 meters and shorter by the Radio Act of 1912. This exile, along with a “we’ll show them” spirit, provided new opportunities for important discoveries and data taking by hams. Initially the sheer number of hams provided wide geographic data coverage. In recent years, data-taking systems have been developed by hams. With the focus of this Workshop being “Ionospheric Effects and Sensing”, this presentation will review the contribution by hams to propagation science and their collaboration with the scientific community on propagation issues. Some of the topics covered will be trans-equatorial propagation, long-delayed echoes (LDEs), MINIMUF propagation predictions, fading tests with the Bureau of Standards, the ARRL-IGY propagation research project, the Reverse Beacon Network (RBN), the Weak Signal Propagation Reporter (WSPR) and data from DXpeditions.

JF - HamSCI Workshop 2019 PB - HamSCI CY - Cleveland, OH ER - TY - CONF T1 - Hams: The First Makers T2 - HamSCI Workshop 2019 Y1 - 2019 A1 - Frankie Bonte A1 - Seamus Bonte AB -

Amateur radio operators were the first Makers. In the early days of radio, they constructed the first receivers in the form of crude crystal radio sets. As those receivers became more complex, they scoured the neighborhoods for parts that were cast aside or other broken electronics to make their own transmitters. They developed the first computers and attached them to transceivers, creating the digital modes we use today. Every Ham is part machinist, electronics technician, and computer scientist, driven by the magic that is radio. Today’s Makers have many of the same traits as a Ham. They love to create technology and put it to use to benefit others. However, Makers require key resources and know-how to continue creating or making. Just as radio clubs bring together Hams to solve problems and share solutions, MakerSpaces provide the geographic location for Makers to gather. This gives them access to specialized equipment and allows them opportunities for group creativity and cooperation among like-minded tinkers. MakerSpaces, such as Think[box] at Case Western and The Point at Otterbein University, are centers with tools and equipment to enable Makers to complete projects and share ideas. This presentation will detail the various types of equipment typically found in a MakerSpace, how one can utilize a MakerSpace as a ham radio operator to fulfill learning and technological needs, and where to find MakerSpaces. We will go on to show how Ham radio can benefit from Makers, and how MakerSpaces can evolve through the inclusion of Hams.

JF - HamSCI Workshop 2019 PB - HamSCI CY - Cleveland, OH ER - TY - CONF T1 - HamSCI HF Receiver Requirements T2 - HamSCI Workshop 2019 Y1 - 2019 A1 - T. C. McDermott AB -

This paper outlines general requirements for the HAMSCI HF receiver equipment. The objectives of Scientific Research prescribe maximum performance and flexibility while the needs of the citizen science community impose significant cost constraints. The general requirements therefore balance the science capability of the HF receiver with the cost. The paper covers architecture of the receiver, key performance metrics, and trade-offs in performance. The actual equipment realization is not covered in this paper.

JF - HamSCI Workshop 2019 PB - HamSCI CY - Cleveland, OH ER - TY - CONF T1 - HamSCI Magnetometer Network for Space Weather Monitoring T2 - HamSCI Workshop 2019 Y1 - 2019 A1 - Hyomin Kim A1 - Nathaniel A. Frissell AB -

Besides auroral observations, magnetic field measurements are one of the traditional ways of observing the space weather phenomena on the ground. To that end, magnetic sensors, “magnetometer”, are typically used for space research. The instrument has a wide range of applications including metal detection, non-contact switch, non-destructive testing, oil/coal exploration, military as well as space research. Magnetometers on the ground provide critical information about how solar activities impact the earth’s magnetic fields (magnetosphere) and ionosphere. In particular, geomagnetically induced currents (GIC) due to temporal changes in magnetic fields (dB/dt) are a very important issue in space weather. A densely-spaced magnetometer array, as proposed in the HamSCI space weather station project, will demonstrate their space weather monitoring capability in unprecedented spatial extent. Here, we propose and compare three types of inexpensive, simple, mid-grade magnetometers utilizing the anisotropic magneto-resistive (AMR), magneto-inductive and fluxgate technologies. The proposed magnetometers will be designed to measure large- and medium-scale geomagnetic activities approximately from a few to hundreds of nT. Preliminary prototype test results and their design, fabrication, calibration and installation plans are presented.

JF - HamSCI Workshop 2019 PB - HamSCI CY - Cleveland, OH ER - TY - CONF T1 - HamSCI Personal Space Weather Station: A New Tool for Citizen Science Geospace Research T2 - USNC–URSI National Radio Science Meeting Y1 - 2019 A1 - J. S. Vega A1 - N. A. Frissell A1 - P. J. Erickson A1 - A. J. Gerrard AB -

Recent advances in geospace remote sensing have shown that large-scale distributed networks of ground-based sensors pay large dividends by providing a big picture view of phenomena that were previously observed only by point-measurements. Notable examples include the improved understanding of traveling ionospheric disturbance (TID) sources based on observations from the high frequency (HF) Super Dual Auroral Radar Network (SuperDARN) radars and GNSS-based total electron content remote sensing networks. While these existing networks provide excellent insight into TID science, the system remains undersampled (especially at HF) and more observations are needed to advance understanding. Additionally, previous measurements have revealed that characteristics of medium scale traveling ionospheric disturbances (MSTIDs) observed on the bottomside ionosphere using oblique HF sounding by SuperDARN differ from integrated ionospheric measurements of MSTIDs made using GNSS-TEC. These differences have yet to be accounted for, and additional observations could aid in understanding the propagation of MSTIDs from the bottom to the top of the ionosphere. In an effort to generate these additional measurements, the Ham Radio Science Citizen Investigation (HamSCI, hamsci.org) is working with the Tucson Amateur Packet Radio Corporation (TAPR, tapr.org), an engineering organization comprising of volunteer amateur radio operators and engineers, to develop a network of Personal Space Weather Stations that will provide scientific-grade observations of signals-of-opportunity across the HF bands from volunteer citizen observers. These measurements will play a key role in the characterization of ionospheric variability across the geographic regions in which these stations are deployed. We will describe concepts, key software patterns for radio science, and proposed timelines for the Personal Space Weather Station project. A particular focus will be assembling the proper metadata for science grade observations, and strategies for lightweight calibration of radio sensors. Initial project efforts concentrate on a wideband receiving station and backing software data distribution system.

JF - USNC–URSI National Radio Science Meeting PB - U.S. National Committee for URSI CY - Boulder, CO UR - https://nrsmboulder.org/ ER - TY - CONF T1 - HF Spectrum Playback using Gnuradio (Demonstration) T2 - HamSCI Workshop 2019 Y1 - 2019 A1 - John Ackermann JF - HamSCI Workshop 2019 PB - HamSCI CY - Cleveland, OH ER - TY - CONF T1 - High Frequency Communications Response to Solar Activity in September 2017 as Observed by Amateur Radio Networks T2 - HamSCI Workshop 2019 Y1 - 2019 A1 - Nathaniel A. Frissell A1 - Joshua S. Vega A1 - Evan Markowitz A1 - Andrew J. Gerrard A1 - William D. Engelke A1 - Philip J. Erickson A1 - Ethan S. Miller A1 - R. Carl Luetzelschwab A1 - Jacob Bortnik AB -

Numerous solar flares and coronal mass ejection‐induced interplanetary shocks associated with solar active region AR12673 caused disturbances to terrestrial high‐frequency (HF, 3–30 MHz) radio communications from 4–14 September 2017. Simultaneously, Hurricanes Irma and Jose caused significant damage to the Caribbean Islands and parts of Florida. The coincidental timing of both the space weather activity and hurricanes was unfortunate, as HF radio was needed for emergency communications. This paper presents the response of HF amateur radio propagation as observed by the Reverse Beacon Network and the Weak Signal Propagation Reporting Network to the space weather events of that period. Distributed data coverage from these dense sources provided a unique mix of global and regional coverage of ionospheric response and recovery that revealed several features of storm time HF propagation dynamics. X‐class flares on 6, 7, and 10 September caused acute radio blackouts during the day in the Caribbean with recovery times of tens of minutes to hours, based on the decay time of the flare. A severe geomagnetic storm with Kpmax = 8+ and SYM‐Hmin = −146 nT occurring 7–10 September wiped out ionospheric communications first on 14 MHz and then on 7 MHz starting at ∼1200 UT 8 September. This storm, combined with affects from additional flare and geomagnetic activity, contributed to a significant suppression of effective HF propagation bands both globally and in the Caribbean for a period of 12 to 15 days.

JF - HamSCI Workshop 2019 PB - HamSCI CY - Cleveland, OH ER - TY - JOUR T1 - High Frequency Communications Response to Solar Activity in September 2017 as Observed by Amateur Radio Networks JF - Space Weather Y1 - 2019 A1 - Frissell, Nathaniel A. A1 - Vega, Joshua S. A1 - Markowitz, Evan A1 - Gerrard, Andrew J. A1 - Engelke, William D. A1 - Erickson, Philip J. A1 - Miller, Ethan S. A1 - Luetzelschwab, R. Carl A1 - Bortnik, Jacob KW - Amateur Radio KW - Geomagnetic Storm KW - Ham Radio KW - HF Radio Propagation KW - Radio Blackout KW - Solar Flare AB -

Abstract Numerous solar flares and coronal mass ejection (CME) induced interplanetary shocks associated with solar active region AR12673 caused disturbances to terrestrial high frequency (HF, 3--30 MHz) radio communications from 4-14 September 2017. Simultaneously, Hurricanes Irma and Jose caused significant damage to the Caribbean Islands and parts of Florida. The coincidental timing of both the space weather activity and hurricanes was unfortunate, as HF radio was needed for emergency communications. This paper presents the response of HF amateur radio propagation as observed by the Reverse Beacon Network (RBN) and the Weak Signal Propagation Reporting Network (WSPRNet) to the space weather events of that period. Distributed data coverage from these dense sources provided a unique mix of global and regional coverage of ionospheric response and recovery that revealed several features of storm-time HF propagation dynamics. X-class flares on 6, 7, and 10 September caused acute radio blackouts during the day in the Caribbean with recovery times of tens of minutes to hours, based on the decay time of the flare. A severe geomagnetic storm withKpmax = 8 + and?SYM ? Hmin =  ? 146?nT occurring 7-10 September wiped out ionospheric communications first on 14 MHz and then on 7 MHz starting at~1200 UT 8 September. This storm, combined with affects from additional flare and geomagnetic activity, contributed to a significant suppression of effective HF propagation bands both globally and in the Caribbean for a period of 12 to 15 days.

UR - https://doi.org/10.1029/2018SW002008 JO - Space Weather ER - TY - CONF T1 - History of Case ARC and W8EDU T2 - HamSCI Workshop 2019 Y1 - 2019 A1 - James Galm JF - HamSCI Workshop 2019 PB - HamSCI CY - Cleveland, OH ER - TY - CONF T1 - How Real-Time Scoreboards Change Contesting T2 - Dayton Hamvention Y1 - 2019 A1 - Victor Androsov A1 - Randy Thompson JF - Dayton Hamvention PB - Ham Radio 2.0 CY - Xenia, OH ER - TY - CONF T1 - High Frequency Communications Response to Solar Activity in September 2017 as Observed by Amateur Radio Networks T2 - Fall AGU Y1 - 2018 A1 - Frissell, Nathaniel A. A1 - Vega, Joshua S. A1 - Markowitz, Evan A1 - Gerrard, Andrew J. A1 - Engelke, William D. A1 - Erickson, Philip J. A1 - Miller, Ethan S. A1 - Luetzelschwab, R. Carl A1 - Bortnik, Jacob KW - Amateur Radio KW - Geomagnetic Storm KW - Ham Radio KW - HF Radio Propagation KW - Radio Blackout KW - Solar Flare AB -

Numerous solar flares and coronal mass ejection (CME) induced interplanetary shocks associated with solar active region AR12673 caused disturbances to terrestrial high frequency (HF, 3–30 MHz) radio communications from 4-14 September 2017. Simultaneously, Hurricanes Irma and Jose caused significant damage to the Caribbean Islands and parts of Florida. The coincidental timing of both the space weather activity and hurricanes was unfortunate, as HF radio was needed for emergency communications. This paper presents the response of HF amateur radio propagation as observed by the Reverse Beacon Network (RBN) and the Weak Signal Propagation Reporting Network (WSPRNet) to the space weather events of that period. Distributed data coverage from these dense sources provided a unique mix of global and regional coverage of ionospheric response and recovery that revealed several features of storm-time HF propagation dynamics. X-class flares on 6, 7, and 10 September caused acute radio blackouts during the day in the Caribbean with recovery times of tens of minutes to hours, based on the decay time of the flare. A severe geomagnetic storm withKpmax = 8 + and SYM − Hmin = − 146 nT occurring 7-10 September wiped out ionospheric communications first on 14 MHz and then on 7 MHz starting at 1200 UT 8 September. This storm, combined with affects from additional flare and geomagnetic activity, contributed to a significant suppression of effective HF propagation bands both globally and in the Caribbean for a period of 12 to 15 days.

JF - Fall AGU PB - American Geophysical Union CY - Washington, DC UR - https://agu.confex.com/agu/fm18/meetingapp.cgi/Paper/419847 ER - TY - CONF T1 - HamSCI and the 2017 Total Solar Eclipse T2 - American Geophysical Union Fall Meeting Y1 - 2017 A1 - N. A. Frissell A1 - J. D. Katz A1 - S. W. Gunning A1 - J. S. Vega A1 - A. J. Gerrard A1 - M. L. Moses A1 - G. D. Earle A1 - M. L. West A1 - P. J. Erickson A1 - E. S. Miller A1 - R. Gerzoff A1 - H. Ward Silver JF - American Geophysical Union Fall Meeting PB - American Geophysical Union CY - New Orleans, LA ER - TY - CONF T1 - HamSCI and the 2017 Total Solar Eclipse T2 - 2017 Annual Meeting of the APS Mid-Atlantic Section Y1 - 2017 A1 - N. A. Frissell A1 - J. D. Katz A1 - S. W. Gunning A1 - J. S. Vega A1 - M. L. West A1 - G. D. Earle A1 - M. L. Moses A1 - H. W. Silver JF - 2017 Annual Meeting of the APS Mid-Atlantic Section PB - American Physical Society CY - Newark, NJ ER - TY - CONF T1 - HamSCI and the 2017 Total Solar Eclipse T2 - HamSCI-UK Y1 - 2017 A1 - N. A. Frissell A1 - W. Engelke A1 - J. D. Katz A1 - J. S. Vega JF - HamSCI-UK PB - HamSCI-UK CY - Milton Keynes, UK ER - TY - CONF T1 - HamSCI and the 2017 Total Solar Eclipse T2 - NSF CEDAR (Coupling, Energetics, and Dynamics of Atmospheric Regions) Y1 - 2017 A1 - N. A. Frissell A1 - J. R. Ackermann A1 - G. D. Earle A1 - P. J. Erickson A1 - A. J. Gerrard A1 - R. B. Gerzoff A1 - S. W. Gunning A1 - M. Hirsch A1 - J. D. Katz A1 - S. R. Kaeppller A1 - R. W. McGwier A1 - E. S. Miller A1 - M. L. Moses A1 - G. Perry A1 - S. E. Reyer A1 - A. Shovkoplyas A1 - H. W. Silver A1 - J. S. Vega A1 - RBN Team JF - NSF CEDAR (Coupling, Energetics, and Dynamics of Atmospheric Regions) CY - Keystone, CO ER - TY - CONF T1 - HamSCI and the 2017 Total Solar Eclipse (Experiment Description) T2 - ARRL and TAPR Digital Communications Conference Y1 - 2017 A1 - N. A. Frissell A1 - J. S. Vega A1 - J. D. Katz A1 - S. W. Gunning A1 - A. J. Gerrard A1 - M. L. Moses A1 - G. D. Earle A1 - E. S. Miller A1 - J. D. Huba A1 - M. Hirsch A1 - H. W. Silver A1 - S. E. Reyer A1 - J. R. Ackermann A1 - M. D. Suhar A1 - D. Bern AB -

On 21 August 2017, a total solar eclipse will cause the shadow of the moon to traverse the United States from Oregon to South Carolina in just over 90 minutes. The sudden absence of sunlight due to the eclipse, especially solar UV and x-rays, provides an impulse function to the upper atmosphere that modifies the neutral dynamics, plasma concentrations, and related properties. In spite of more than 60 years of research, open questions remain regarding eclipse-induced ionospheric impacts. Ham radio operators’ advanced technical skills and inherent interest in ionospheric science make the amateur radio community ideal for contributing to and and participating in large-scale ionospheric sounding experiments. This pa- per describes the Solar Eclipse QSO Party (SEQP), the HF Wideband Recording Experiment, and the Eclipse Frequency Measurement Test (FMT), three amateur radio experiments designed to study the 2017 total solar eclipse. These experi- ments are coordinated by HamSCI, the Ham radio Science Citizen Investigation, a citizen science organization that connects the amateur radio community to the professional space science research community for mutual benefit.

JF - ARRL and TAPR Digital Communications Conference CY - St. Louis, MO UR - https://www.tapr.org/pub_dcc.html ER - TY - CONF T1 - HamSCI and the 2017 Total Solar Eclipse (First Results) T2 - ARRL and TAPR Digital Communications Conference Y1 - 2017 A1 - N. A. Frissell A1 - W. Engelke A1 - J. D. Katz A1 - S. W. Gunning A1 - J. S. Vega JF - ARRL and TAPR Digital Communications Conference CY - St. Louis, MO UR - https://www.tapr.org/pub_dcc.html ER - TY - CONF T1 - HamSCI: The Ham Radio Science Citizen Investigation (Banquet Presentation) T2 - NSF CEDAR (Coupling, Energetics, and Dynamics of Atmospheric Regions) Y1 - 2017 A1 - N. A. Frissell A1 - J. R. Ackermann A1 - J. Dzekevich A1 - G. D. Earle A1 - P. J. Erickson A1 - A. J. Gerrard A1 - R. B. Gerzoff A1 - S. W. Gunning A1 - M. Hirsch A1 - J. D. Katz A1 - S. R. Kaeppler A1 - R. W. McGwier A1 - E. S. Miller A1 - M. L. Moses A1 - G. Perry A1 - S. E. Reyer A1 - A. Shovkoplyas A1 - H. W. Silver A1 - J. S. Vega A1 - RBN Team JF - NSF CEDAR (Coupling, Energetics, and Dynamics of Atmospheric Regions) CY - Keystone, CO ER - TY - CONF T1 - The H.A.R.C. Database and Visualization Utilities T2 - ARRL and TAPR Digital Communications Conference Y1 - 2017 A1 - J. D. Katz A1 - W. Engelke A1 - N. A. Frissell AB -

HamSCI’s goal is to construct a symbiotic relationship between the formal research community and the Amateur Radio community. To facilitate this transfer of knowledge HamSCI must pioneer technologies that allow scientists to easily obtain and understand Amateur Radio data. This task necessitates the creation of warehousing and visualization facilities that allow scientists to easily understand and make use of our data sets. We are currently testing a database and visualization toolkit designed to handle our existing 2 billion-record long QSO log. This data set represents a compiled version of data gathered by the Reverse Beacon Network, WSPRNet, and PSKReporter. Our goal is to build a robust, fast, and queryable front end to the massive, and currently underuti- lized, data sources created by Amateur Radio operators.

JF - ARRL and TAPR Digital Communications Conference CY - St. Louis, MO UR - https://www.tapr.org/pub_dcc.html ER - TY - MGZN T1 - HamSCI: Ham Radio Science Citizen Investigation Y1 - 2016 A1 - H. W. Silver JF - QST VL - 100 UR - http://hamsci.org/sites/default/files/publications/201608_QST_Silver_HamSCI.pdf IS - 8 ER - TY - CONF T1 - HamSCI: The Ham Radio Science Citizen Investigation T2 - Fall 2016 American Geophysical Union Y1 - 2016 A1 - Nathaniel A. Frissell A1 - Magdalina L. Moses A1 - Gregory Earle A1 - Robert W. McGwier A1 - Ethan S. Miller A1 - Steven R. Kaeppler A1 - H. Ward Silver A1 - Felipe Ceglia A1 - David Pascoe A1 - Nicholas Sinanis A1 - Peter Smith A1 - Richard Williams A1 - Alex Shovkoplyas A1 - Andrew J. Gerrard AB -

Amateur (or “ham”) radio operators are individuals with a non-pecuniary interest in radio technology, engineering, communications, science, and public service. They are licensed by their national governments to transmit on amateur radio frequencies. In many jurisdictions, there is no age requirement for a ham radio license, and operators from diverse backgrounds participate. There are more than 740,000 hams in the US, and over 3 million (estimated) worldwide. Many amateur communications are conducted using transionospheric links and thus affected by space weather and ionospheric processes. Recent technological advances have enabled the development of automated ham radio observation networks (e.g. the Reverse Beacon Network, www.reversebeacon.net) and specialized operating modes for the study of weak-signal propagation. The data from these networks have been shown to be useful for the study of ionospheric processes. In order to connect professional researchers with the volunteer-based ham radio community, HamSCI (Ham Radio Science Citizen Investigation, www.hamsci.org) has been established. HamSCI is a platform for publicizing and promoting projects that are consistent with the following objectives: (1) Advance scientific research and understanding through amateur radio activities. (2) Encourage the development of new technologies to support this research. (3) Provide educational opportunities for the amateur community and the general public. HamSCI researchers are working with the American Radio Relay League (ARRL, www.arrl.org) to publicize these objectives and recruit interested hams. The ARRL is the US national organization for amateur radio with a membership of over 170,000 and a monthly magazine, QST. HamSCI is currently preparing to support ionospheric research connected to the 21 Aug 2017 Total Solar Eclipse by expanding coverage of the Reverse Beacon Network and organizing a large-scale ham radio operating event (“QSO Party”) to generate data during the eclipse.

JF - Fall 2016 American Geophysical Union PB - American Geophysical Union CY - San Francisco UR - http://hamsci.org/sites/default/files/publications/2016_AGU_Frissell_HamSCI.pdf ER - TY - ABST T1 - HamSCI and the 2017 Total Solar Eclipse (HamSCI Founding Document) Y1 - 2015 A1 - Nathaniel A. Frissell A1 - Magdalina L. Moses A1 - Gregory D. Earle A1 - Robert McGwier A1 - H. Ward Silver UR - https://hamsci.org/publications/hamsci-and-2017-total-solar-eclipse-hamsci-founding-document ER -