An HF Software‐Defined Radar to Study the Ionosphere
In this paper, a novel design and implementation of a software‐defined high‐frequency ionospheric radar, the Penn State Ionospheric Radar Imager (PIRI), is described. Furthermore, preliminary results produced by the system (located at 40.71° N, 77.97° W) are presented. PIRI is designed to be a modes...
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Veröffentlicht in: | Radio science 2019-09, Vol.54 (9), p.839-849 |
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description | In this paper, a novel design and implementation of a software‐defined high‐frequency ionospheric radar, the Penn State Ionospheric Radar Imager (PIRI), is described. Furthermore, preliminary results produced by the system (located at 40.71° N, 77.97° W) are presented. PIRI is designed to be a modest and low‐cost radar system, which is composed mostly of commercial‐off‐the‐shelf products and utilizing open‐source software to perform pulse generation, pulse coding, downconversion, data acquisition, and signal processing. It is designed to be mobile, as it can easily be deployed at temporary locations to study local ionospheric disturbances. For the results presented herein, the radar operating frequency was 5.125 MHz. However, as the system is software defined and short active receive antennas are used, only the transmit antenna needs to be changed to operate over the entire high‐frequency (HF) band. The two orthogonal receive antennas enable both linear and circular polarization measurements. Peak transmit power of the system is 500 W. PIRI is designed to be a modest and cost‐effective alternative to the current standard HF ionospheric sounding systems and can be readily replicated.
Key Points
Implementation of a low cost, software‐defined HF radar for ionospheric research is explained
Open‐source software and commercial‐off‐the‐shelf products are used
The system allows comprehensive analysis of events such as sporadic E and spread F |
doi_str_mv | 10.1029/2018RS006773 |
format | Article |
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Key Points
Implementation of a low cost, software‐defined HF radar for ionospheric research is explained
Open‐source software and commercial‐off‐the‐shelf products are used
The system allows comprehensive analysis of events such as sporadic E and spread F</description><identifier>ISSN: 0048-6604</identifier><identifier>EISSN: 1944-799X</identifier><identifier>DOI: 10.1029/2018RS006773</identifier><language>eng</language><publisher>Washington: Blackwell Publishing Ltd</publisher><subject>Antennas ; Circular polarization ; Data acquisition ; Ionosphere ; Ionospheric disturbances ; Ionospheric sounding ; Open source software ; Radar ; Radar equipment ; radar system design ; remote sensing ; Signal processing ; software‐defined radar ; System effectiveness</subject><ispartof>Radio science, 2019-09, Vol.54 (9), p.839-849</ispartof><rights>2019. American Geophysical Union. All Rights Reserved.</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c4102-c561e513bae561197a9b0e91b7bb8e97741c391d51aaf8e19619f3ad50e3b9c23</citedby><cites>FETCH-LOGICAL-c4102-c561e513bae561197a9b0e91b7bb8e97741c391d51aaf8e19619f3ad50e3b9c23</cites><orcidid>0000-0003-2209-6966 ; 0000-0002-5416-7039</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://onlinelibrary.wiley.com/doi/pdf/10.1029%2F2018RS006773$$EPDF$$P50$$Gwiley$$H</linktopdf><linktohtml>$$Uhttps://onlinelibrary.wiley.com/doi/full/10.1029%2F2018RS006773$$EHTML$$P50$$Gwiley$$H</linktohtml><link.rule.ids>314,776,780,1411,1427,11493,27901,27902,45550,45551,46384,46443,46808,46867</link.rule.ids></links><search><creatorcontrib>Bostan, Salih Mehmed</creatorcontrib><creatorcontrib>Urbina, Julio V.</creatorcontrib><creatorcontrib>Mathews, John D.</creatorcontrib><creatorcontrib>Bilén, Sven G.</creatorcontrib><creatorcontrib>Breakall, James K.</creatorcontrib><title>An HF Software‐Defined Radar to Study the Ionosphere</title><title>Radio science</title><description>In this paper, a novel design and implementation of a software‐defined high‐frequency ionospheric radar, the Penn State Ionospheric Radar Imager (PIRI), is described. Furthermore, preliminary results produced by the system (located at 40.71° N, 77.97° W) are presented. PIRI is designed to be a modest and low‐cost radar system, which is composed mostly of commercial‐off‐the‐shelf products and utilizing open‐source software to perform pulse generation, pulse coding, downconversion, data acquisition, and signal processing. It is designed to be mobile, as it can easily be deployed at temporary locations to study local ionospheric disturbances. For the results presented herein, the radar operating frequency was 5.125 MHz. However, as the system is software defined and short active receive antennas are used, only the transmit antenna needs to be changed to operate over the entire high‐frequency (HF) band. The two orthogonal receive antennas enable both linear and circular polarization measurements. Peak transmit power of the system is 500 W. PIRI is designed to be a modest and cost‐effective alternative to the current standard HF ionospheric sounding systems and can be readily replicated.
Key Points
Implementation of a low cost, software‐defined HF radar for ionospheric research is explained
Open‐source software and commercial‐off‐the‐shelf products are used
The system allows comprehensive analysis of events such as sporadic E and spread F</description><subject>Antennas</subject><subject>Circular polarization</subject><subject>Data acquisition</subject><subject>Ionosphere</subject><subject>Ionospheric disturbances</subject><subject>Ionospheric sounding</subject><subject>Open source software</subject><subject>Radar</subject><subject>Radar equipment</subject><subject>radar system design</subject><subject>remote sensing</subject><subject>Signal processing</subject><subject>software‐defined radar</subject><subject>System effectiveness</subject><issn>0048-6604</issn><issn>1944-799X</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2019</creationdate><recordtype>article</recordtype><recordid>eNp90MFKw0AQBuBFFKzVmw-w4NXozO5mN3ssrbWFgtAoeAubZEJbarZuUkpuPoLP6JMYqQdPnmYOH_8MP2PXCHcIwt4LwGSZAmhj5AkboFUqMta-nrIBgEoirUGds4um2QCgirUaMD2q-WzKU1-1Bxfo6-NzQtW6ppIvXekCbz1P233Z8XZFfO5r3-xWFOiSnVVu29DV7xyyl-nD83gWLZ4e5-PRIipU_1FUxBopRpk76je0xtkcyGJu8jwha4zCQlosY3SuSgitRltJV8ZAMreFkEN2c8zdBf--p6bNNn4f6v5kJiQYicYa6NXtURXBN02gKtuF9ZsLXYaQ_TST_W2m5-LID-stdf_abDlJBSRSyG8sgWMX</recordid><startdate>201909</startdate><enddate>201909</enddate><creator>Bostan, Salih Mehmed</creator><creator>Urbina, Julio V.</creator><creator>Mathews, John D.</creator><creator>Bilén, Sven G.</creator><creator>Breakall, James K.</creator><general>Blackwell Publishing Ltd</general><scope>AAYXX</scope><scope>CITATION</scope><scope>7SP</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope><orcidid>https://orcid.org/0000-0003-2209-6966</orcidid><orcidid>https://orcid.org/0000-0002-5416-7039</orcidid></search><sort><creationdate>201909</creationdate><title>An HF Software‐Defined Radar to Study the Ionosphere</title><author>Bostan, Salih Mehmed ; Urbina, Julio V. ; Mathews, John D. ; Bilén, Sven G. ; Breakall, James K.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c4102-c561e513bae561197a9b0e91b7bb8e97741c391d51aaf8e19619f3ad50e3b9c23</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2019</creationdate><topic>Antennas</topic><topic>Circular polarization</topic><topic>Data acquisition</topic><topic>Ionosphere</topic><topic>Ionospheric disturbances</topic><topic>Ionospheric sounding</topic><topic>Open source software</topic><topic>Radar</topic><topic>Radar equipment</topic><topic>radar system design</topic><topic>remote sensing</topic><topic>Signal processing</topic><topic>software‐defined radar</topic><topic>System effectiveness</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Bostan, Salih Mehmed</creatorcontrib><creatorcontrib>Urbina, Julio V.</creatorcontrib><creatorcontrib>Mathews, John D.</creatorcontrib><creatorcontrib>Bilén, Sven G.</creatorcontrib><creatorcontrib>Breakall, James K.</creatorcontrib><collection>CrossRef</collection><collection>Electronics & Communications Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Radio science</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Bostan, Salih Mehmed</au><au>Urbina, Julio V.</au><au>Mathews, John D.</au><au>Bilén, Sven G.</au><au>Breakall, James K.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>An HF Software‐Defined Radar to Study the Ionosphere</atitle><jtitle>Radio science</jtitle><date>2019-09</date><risdate>2019</risdate><volume>54</volume><issue>9</issue><spage>839</spage><epage>849</epage><pages>839-849</pages><issn>0048-6604</issn><eissn>1944-799X</eissn><abstract>In this paper, a novel design and implementation of a software‐defined high‐frequency ionospheric radar, the Penn State Ionospheric Radar Imager (PIRI), is described. Furthermore, preliminary results produced by the system (located at 40.71° N, 77.97° W) are presented. PIRI is designed to be a modest and low‐cost radar system, which is composed mostly of commercial‐off‐the‐shelf products and utilizing open‐source software to perform pulse generation, pulse coding, downconversion, data acquisition, and signal processing. It is designed to be mobile, as it can easily be deployed at temporary locations to study local ionospheric disturbances. For the results presented herein, the radar operating frequency was 5.125 MHz. However, as the system is software defined and short active receive antennas are used, only the transmit antenna needs to be changed to operate over the entire high‐frequency (HF) band. The two orthogonal receive antennas enable both linear and circular polarization measurements. Peak transmit power of the system is 500 W. PIRI is designed to be a modest and cost‐effective alternative to the current standard HF ionospheric sounding systems and can be readily replicated.
Key Points
Implementation of a low cost, software‐defined HF radar for ionospheric research is explained
Open‐source software and commercial‐off‐the‐shelf products are used
The system allows comprehensive analysis of events such as sporadic E and spread F</abstract><cop>Washington</cop><pub>Blackwell Publishing Ltd</pub><doi>10.1029/2018RS006773</doi><tpages>11</tpages><orcidid>https://orcid.org/0000-0003-2209-6966</orcidid><orcidid>https://orcid.org/0000-0002-5416-7039</orcidid><oa>free_for_read</oa></addata></record> |
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subjects | Antennas Circular polarization Data acquisition Ionosphere Ionospheric disturbances Ionospheric sounding Open source software Radar Radar equipment radar system design remote sensing Signal processing software‐defined radar System effectiveness |
title | An HF Software‐Defined Radar to Study the Ionosphere |
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