Sounding of an artificially perturbed ionosphere by means of an ionosonde/position finder with chirp modulation of the signal
We describe the operation of an ionosonde/position finder with chirp modulation of the signal. The first results of measuring the characteristics of short-wave radio signals scattered by artificial small-scale inhomogeneities, which were obtained by means of an ionosonde/position finder on the IZMIR...
Ausführliche Beschreibung
Autor*in: |
Uryadov, V. P. [verfasserIn] Vertogradov, G. G. [verfasserIn] Vertogradov, V. G. [verfasserIn] Kubatko, S. V. [verfasserIn] Ponyatov, A. A. [verfasserIn] Cherkashin, Yu. N. [verfasserIn] Krasheninnikov, I. V. [verfasserIn] Valov, V. A. [verfasserIn] Komrakov, G. P. [verfasserIn] Makarov, A. V. [verfasserIn] Bredikhin, D. V. [verfasserIn] |
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Format: |
E-Artikel |
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Sprache: |
Englisch |
Erschienen: |
2009 |
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Schlagwörter: |
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Übergeordnetes Werk: |
Enthalten in: Radiophysics and quantum electronics - New York, NY [u.a.] : Consultants Bureau, 1965, 52(2009), 4 vom: Apr., Seite 241-251 |
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Übergeordnetes Werk: |
volume:52 ; year:2009 ; number:4 ; month:04 ; pages:241-251 |
Links: |
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DOI / URN: |
10.1007/s11141-009-9136-9 |
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Katalog-ID: |
SPR017042496 |
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100 | 1 | |a Uryadov, V. P. |e verfasserin |4 aut | |
245 | 1 | 0 | |a Sounding of an artificially perturbed ionosphere by means of an ionosonde/position finder with chirp modulation of the signal |
264 | 1 | |c 2009 | |
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520 | |a We describe the operation of an ionosonde/position finder with chirp modulation of the signal. The first results of measuring the characteristics of short-wave radio signals scattered by artificial small-scale inhomogeneities, which were obtained by means of an ionosonde/position finder on the IZMIRAN—“SURA”—Rostov-on-Don path are presented. It was found that under certain ionospheric conditions, the angular and frequency selection of the scattered signals take place, in which case the signals are observed simultaneously in several frequency intervals (mainly, in three, namely, 6–9.5 MHz, 10–12 MHz, and 15–18 MHz) with different angles of incidence of radio waves in the vertical plane. In this case, the incidence angles were 20◦–35◦, 18◦–32◦, and 10◦–20◦ from the horizon for the first, second, and third frequency interval, respectively. Ionograms of oblique sounding were modeled allowing for the scattering of radio waves by artificial small-scale inhomogeneities. It is shown that at frequencies from 10 to 12 MHz, aspect conditions are fulfilled for the signals ducting along the high-angle beam (Pedersen mode). At frequencies 15–18 MHz (higher than the maximum observable frequency of the forward signal on the path IZMIRAN—Rostov-on-Don), aspect scattering conditions are fulfilled for the signals incident on a scattering area in the ascending part of the trajectory. At low frequencies 6–9.5 MHz (below the maximum observed frequency of the forward signal on the IZMIRAN—Rostov-on-Don path), the observable additional signals are caused by the scattering of radio waves by artificial inhomogeneities with subsequent relfection of the scattered signal from the Earth on the “SURA”—Rostov-on-Don path. | ||
650 | 4 | |a Radio Wave |7 (dpeaa)DE-He213 | |
650 | 4 | |a Electron Number Density |7 (dpeaa)DE-He213 | |
650 | 4 | |a Scattered Signal |7 (dpeaa)DE-He213 | |
650 | 4 | |a Linear Frequency Modulation |7 (dpeaa)DE-He213 | |
650 | 4 | |a Ionospheric Condition |7 (dpeaa)DE-He213 | |
700 | 1 | |a Vertogradov, G. G. |e verfasserin |4 aut | |
700 | 1 | |a Vertogradov, V. G. |e verfasserin |4 aut | |
700 | 1 | |a Kubatko, S. V. |e verfasserin |4 aut | |
700 | 1 | |a Ponyatov, A. A. |e verfasserin |4 aut | |
700 | 1 | |a Cherkashin, Yu. N. |e verfasserin |4 aut | |
700 | 1 | |a Krasheninnikov, I. V. |e verfasserin |4 aut | |
700 | 1 | |a Valov, V. A. |e verfasserin |4 aut | |
700 | 1 | |a Komrakov, G. P. |e verfasserin |4 aut | |
700 | 1 | |a Makarov, A. V. |e verfasserin |4 aut | |
700 | 1 | |a Bredikhin, D. V. |e verfasserin |4 aut | |
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773 | 1 | 8 | |g volume:52 |g year:2009 |g number:4 |g month:04 |g pages:241-251 |
856 | 4 | 0 | |u https://dx.doi.org/10.1007/s11141-009-9136-9 |z lizenzpflichtig |3 Volltext |
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2009 |
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10.1007/s11141-009-9136-9 doi (DE-627)SPR017042496 (SPR)s11141-009-9136-9-e DE-627 ger DE-627 rakwb eng 530 620 ASE 33.16 bkl 53.74 bkl 33.80 bkl 39.22 bkl Uryadov, V. P. verfasserin aut Sounding of an artificially perturbed ionosphere by means of an ionosonde/position finder with chirp modulation of the signal 2009 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We describe the operation of an ionosonde/position finder with chirp modulation of the signal. The first results of measuring the characteristics of short-wave radio signals scattered by artificial small-scale inhomogeneities, which were obtained by means of an ionosonde/position finder on the IZMIRAN—“SURA”—Rostov-on-Don path are presented. It was found that under certain ionospheric conditions, the angular and frequency selection of the scattered signals take place, in which case the signals are observed simultaneously in several frequency intervals (mainly, in three, namely, 6–9.5 MHz, 10–12 MHz, and 15–18 MHz) with different angles of incidence of radio waves in the vertical plane. In this case, the incidence angles were 20◦–35◦, 18◦–32◦, and 10◦–20◦ from the horizon for the first, second, and third frequency interval, respectively. Ionograms of oblique sounding were modeled allowing for the scattering of radio waves by artificial small-scale inhomogeneities. It is shown that at frequencies from 10 to 12 MHz, aspect conditions are fulfilled for the signals ducting along the high-angle beam (Pedersen mode). At frequencies 15–18 MHz (higher than the maximum observable frequency of the forward signal on the path IZMIRAN—Rostov-on-Don), aspect scattering conditions are fulfilled for the signals incident on a scattering area in the ascending part of the trajectory. At low frequencies 6–9.5 MHz (below the maximum observed frequency of the forward signal on the IZMIRAN—Rostov-on-Don path), the observable additional signals are caused by the scattering of radio waves by artificial inhomogeneities with subsequent relfection of the scattered signal from the Earth on the “SURA”—Rostov-on-Don path. Radio Wave (dpeaa)DE-He213 Electron Number Density (dpeaa)DE-He213 Scattered Signal (dpeaa)DE-He213 Linear Frequency Modulation (dpeaa)DE-He213 Ionospheric Condition (dpeaa)DE-He213 Vertogradov, G. G. verfasserin aut Vertogradov, V. G. verfasserin aut Kubatko, S. V. verfasserin aut Ponyatov, A. A. verfasserin aut Cherkashin, Yu. N. verfasserin aut Krasheninnikov, I. V. verfasserin aut Valov, V. A. verfasserin aut Komrakov, G. P. verfasserin aut Makarov, A. V. verfasserin aut Bredikhin, D. V. verfasserin aut Enthalten in Radiophysics and quantum electronics New York, NY [u.a.] : Consultants Bureau, 1965 52(2009), 4 vom: Apr., Seite 241-251 (DE-627)325573395 (DE-600)2037675-3 1573-9120 nnns volume:52 year:2009 number:4 month:04 pages:241-251 https://dx.doi.org/10.1007/s11141-009-9136-9 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_647 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.16 ASE 53.74 ASE 33.80 ASE 39.22 ASE AR 52 2009 4 04 241-251 |
spelling |
10.1007/s11141-009-9136-9 doi (DE-627)SPR017042496 (SPR)s11141-009-9136-9-e DE-627 ger DE-627 rakwb eng 530 620 ASE 33.16 bkl 53.74 bkl 33.80 bkl 39.22 bkl Uryadov, V. P. verfasserin aut Sounding of an artificially perturbed ionosphere by means of an ionosonde/position finder with chirp modulation of the signal 2009 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We describe the operation of an ionosonde/position finder with chirp modulation of the signal. The first results of measuring the characteristics of short-wave radio signals scattered by artificial small-scale inhomogeneities, which were obtained by means of an ionosonde/position finder on the IZMIRAN—“SURA”—Rostov-on-Don path are presented. It was found that under certain ionospheric conditions, the angular and frequency selection of the scattered signals take place, in which case the signals are observed simultaneously in several frequency intervals (mainly, in three, namely, 6–9.5 MHz, 10–12 MHz, and 15–18 MHz) with different angles of incidence of radio waves in the vertical plane. In this case, the incidence angles were 20◦–35◦, 18◦–32◦, and 10◦–20◦ from the horizon for the first, second, and third frequency interval, respectively. Ionograms of oblique sounding were modeled allowing for the scattering of radio waves by artificial small-scale inhomogeneities. It is shown that at frequencies from 10 to 12 MHz, aspect conditions are fulfilled for the signals ducting along the high-angle beam (Pedersen mode). At frequencies 15–18 MHz (higher than the maximum observable frequency of the forward signal on the path IZMIRAN—Rostov-on-Don), aspect scattering conditions are fulfilled for the signals incident on a scattering area in the ascending part of the trajectory. At low frequencies 6–9.5 MHz (below the maximum observed frequency of the forward signal on the IZMIRAN—Rostov-on-Don path), the observable additional signals are caused by the scattering of radio waves by artificial inhomogeneities with subsequent relfection of the scattered signal from the Earth on the “SURA”—Rostov-on-Don path. Radio Wave (dpeaa)DE-He213 Electron Number Density (dpeaa)DE-He213 Scattered Signal (dpeaa)DE-He213 Linear Frequency Modulation (dpeaa)DE-He213 Ionospheric Condition (dpeaa)DE-He213 Vertogradov, G. G. verfasserin aut Vertogradov, V. G. verfasserin aut Kubatko, S. V. verfasserin aut Ponyatov, A. A. verfasserin aut Cherkashin, Yu. N. verfasserin aut Krasheninnikov, I. V. verfasserin aut Valov, V. A. verfasserin aut Komrakov, G. P. verfasserin aut Makarov, A. V. verfasserin aut Bredikhin, D. V. verfasserin aut Enthalten in Radiophysics and quantum electronics New York, NY [u.a.] : Consultants Bureau, 1965 52(2009), 4 vom: Apr., Seite 241-251 (DE-627)325573395 (DE-600)2037675-3 1573-9120 nnns volume:52 year:2009 number:4 month:04 pages:241-251 https://dx.doi.org/10.1007/s11141-009-9136-9 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_647 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.16 ASE 53.74 ASE 33.80 ASE 39.22 ASE AR 52 2009 4 04 241-251 |
allfields_unstemmed |
10.1007/s11141-009-9136-9 doi (DE-627)SPR017042496 (SPR)s11141-009-9136-9-e DE-627 ger DE-627 rakwb eng 530 620 ASE 33.16 bkl 53.74 bkl 33.80 bkl 39.22 bkl Uryadov, V. P. verfasserin aut Sounding of an artificially perturbed ionosphere by means of an ionosonde/position finder with chirp modulation of the signal 2009 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We describe the operation of an ionosonde/position finder with chirp modulation of the signal. The first results of measuring the characteristics of short-wave radio signals scattered by artificial small-scale inhomogeneities, which were obtained by means of an ionosonde/position finder on the IZMIRAN—“SURA”—Rostov-on-Don path are presented. It was found that under certain ionospheric conditions, the angular and frequency selection of the scattered signals take place, in which case the signals are observed simultaneously in several frequency intervals (mainly, in three, namely, 6–9.5 MHz, 10–12 MHz, and 15–18 MHz) with different angles of incidence of radio waves in the vertical plane. In this case, the incidence angles were 20◦–35◦, 18◦–32◦, and 10◦–20◦ from the horizon for the first, second, and third frequency interval, respectively. Ionograms of oblique sounding were modeled allowing for the scattering of radio waves by artificial small-scale inhomogeneities. It is shown that at frequencies from 10 to 12 MHz, aspect conditions are fulfilled for the signals ducting along the high-angle beam (Pedersen mode). At frequencies 15–18 MHz (higher than the maximum observable frequency of the forward signal on the path IZMIRAN—Rostov-on-Don), aspect scattering conditions are fulfilled for the signals incident on a scattering area in the ascending part of the trajectory. At low frequencies 6–9.5 MHz (below the maximum observed frequency of the forward signal on the IZMIRAN—Rostov-on-Don path), the observable additional signals are caused by the scattering of radio waves by artificial inhomogeneities with subsequent relfection of the scattered signal from the Earth on the “SURA”—Rostov-on-Don path. Radio Wave (dpeaa)DE-He213 Electron Number Density (dpeaa)DE-He213 Scattered Signal (dpeaa)DE-He213 Linear Frequency Modulation (dpeaa)DE-He213 Ionospheric Condition (dpeaa)DE-He213 Vertogradov, G. G. verfasserin aut Vertogradov, V. G. verfasserin aut Kubatko, S. V. verfasserin aut Ponyatov, A. A. verfasserin aut Cherkashin, Yu. N. verfasserin aut Krasheninnikov, I. V. verfasserin aut Valov, V. A. verfasserin aut Komrakov, G. P. verfasserin aut Makarov, A. V. verfasserin aut Bredikhin, D. V. verfasserin aut Enthalten in Radiophysics and quantum electronics New York, NY [u.a.] : Consultants Bureau, 1965 52(2009), 4 vom: Apr., Seite 241-251 (DE-627)325573395 (DE-600)2037675-3 1573-9120 nnns volume:52 year:2009 number:4 month:04 pages:241-251 https://dx.doi.org/10.1007/s11141-009-9136-9 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_647 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.16 ASE 53.74 ASE 33.80 ASE 39.22 ASE AR 52 2009 4 04 241-251 |
allfieldsGer |
10.1007/s11141-009-9136-9 doi (DE-627)SPR017042496 (SPR)s11141-009-9136-9-e DE-627 ger DE-627 rakwb eng 530 620 ASE 33.16 bkl 53.74 bkl 33.80 bkl 39.22 bkl Uryadov, V. P. verfasserin aut Sounding of an artificially perturbed ionosphere by means of an ionosonde/position finder with chirp modulation of the signal 2009 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We describe the operation of an ionosonde/position finder with chirp modulation of the signal. The first results of measuring the characteristics of short-wave radio signals scattered by artificial small-scale inhomogeneities, which were obtained by means of an ionosonde/position finder on the IZMIRAN—“SURA”—Rostov-on-Don path are presented. It was found that under certain ionospheric conditions, the angular and frequency selection of the scattered signals take place, in which case the signals are observed simultaneously in several frequency intervals (mainly, in three, namely, 6–9.5 MHz, 10–12 MHz, and 15–18 MHz) with different angles of incidence of radio waves in the vertical plane. In this case, the incidence angles were 20◦–35◦, 18◦–32◦, and 10◦–20◦ from the horizon for the first, second, and third frequency interval, respectively. Ionograms of oblique sounding were modeled allowing for the scattering of radio waves by artificial small-scale inhomogeneities. It is shown that at frequencies from 10 to 12 MHz, aspect conditions are fulfilled for the signals ducting along the high-angle beam (Pedersen mode). At frequencies 15–18 MHz (higher than the maximum observable frequency of the forward signal on the path IZMIRAN—Rostov-on-Don), aspect scattering conditions are fulfilled for the signals incident on a scattering area in the ascending part of the trajectory. At low frequencies 6–9.5 MHz (below the maximum observed frequency of the forward signal on the IZMIRAN—Rostov-on-Don path), the observable additional signals are caused by the scattering of radio waves by artificial inhomogeneities with subsequent relfection of the scattered signal from the Earth on the “SURA”—Rostov-on-Don path. Radio Wave (dpeaa)DE-He213 Electron Number Density (dpeaa)DE-He213 Scattered Signal (dpeaa)DE-He213 Linear Frequency Modulation (dpeaa)DE-He213 Ionospheric Condition (dpeaa)DE-He213 Vertogradov, G. G. verfasserin aut Vertogradov, V. G. verfasserin aut Kubatko, S. V. verfasserin aut Ponyatov, A. A. verfasserin aut Cherkashin, Yu. N. verfasserin aut Krasheninnikov, I. V. verfasserin aut Valov, V. A. verfasserin aut Komrakov, G. P. verfasserin aut Makarov, A. V. verfasserin aut Bredikhin, D. V. verfasserin aut Enthalten in Radiophysics and quantum electronics New York, NY [u.a.] : Consultants Bureau, 1965 52(2009), 4 vom: Apr., Seite 241-251 (DE-627)325573395 (DE-600)2037675-3 1573-9120 nnns volume:52 year:2009 number:4 month:04 pages:241-251 https://dx.doi.org/10.1007/s11141-009-9136-9 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_647 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.16 ASE 53.74 ASE 33.80 ASE 39.22 ASE AR 52 2009 4 04 241-251 |
allfieldsSound |
10.1007/s11141-009-9136-9 doi (DE-627)SPR017042496 (SPR)s11141-009-9136-9-e DE-627 ger DE-627 rakwb eng 530 620 ASE 33.16 bkl 53.74 bkl 33.80 bkl 39.22 bkl Uryadov, V. P. verfasserin aut Sounding of an artificially perturbed ionosphere by means of an ionosonde/position finder with chirp modulation of the signal 2009 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier We describe the operation of an ionosonde/position finder with chirp modulation of the signal. The first results of measuring the characteristics of short-wave radio signals scattered by artificial small-scale inhomogeneities, which were obtained by means of an ionosonde/position finder on the IZMIRAN—“SURA”—Rostov-on-Don path are presented. It was found that under certain ionospheric conditions, the angular and frequency selection of the scattered signals take place, in which case the signals are observed simultaneously in several frequency intervals (mainly, in three, namely, 6–9.5 MHz, 10–12 MHz, and 15–18 MHz) with different angles of incidence of radio waves in the vertical plane. In this case, the incidence angles were 20◦–35◦, 18◦–32◦, and 10◦–20◦ from the horizon for the first, second, and third frequency interval, respectively. Ionograms of oblique sounding were modeled allowing for the scattering of radio waves by artificial small-scale inhomogeneities. It is shown that at frequencies from 10 to 12 MHz, aspect conditions are fulfilled for the signals ducting along the high-angle beam (Pedersen mode). At frequencies 15–18 MHz (higher than the maximum observable frequency of the forward signal on the path IZMIRAN—Rostov-on-Don), aspect scattering conditions are fulfilled for the signals incident on a scattering area in the ascending part of the trajectory. At low frequencies 6–9.5 MHz (below the maximum observed frequency of the forward signal on the IZMIRAN—Rostov-on-Don path), the observable additional signals are caused by the scattering of radio waves by artificial inhomogeneities with subsequent relfection of the scattered signal from the Earth on the “SURA”—Rostov-on-Don path. Radio Wave (dpeaa)DE-He213 Electron Number Density (dpeaa)DE-He213 Scattered Signal (dpeaa)DE-He213 Linear Frequency Modulation (dpeaa)DE-He213 Ionospheric Condition (dpeaa)DE-He213 Vertogradov, G. G. verfasserin aut Vertogradov, V. G. verfasserin aut Kubatko, S. V. verfasserin aut Ponyatov, A. A. verfasserin aut Cherkashin, Yu. N. verfasserin aut Krasheninnikov, I. V. verfasserin aut Valov, V. A. verfasserin aut Komrakov, G. P. verfasserin aut Makarov, A. V. verfasserin aut Bredikhin, D. V. verfasserin aut Enthalten in Radiophysics and quantum electronics New York, NY [u.a.] : Consultants Bureau, 1965 52(2009), 4 vom: Apr., Seite 241-251 (DE-627)325573395 (DE-600)2037675-3 1573-9120 nnns volume:52 year:2009 number:4 month:04 pages:241-251 https://dx.doi.org/10.1007/s11141-009-9136-9 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_647 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.16 ASE 53.74 ASE 33.80 ASE 39.22 ASE AR 52 2009 4 04 241-251 |
language |
English |
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Enthalten in Radiophysics and quantum electronics 52(2009), 4 vom: Apr., Seite 241-251 volume:52 year:2009 number:4 month:04 pages:241-251 |
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Enthalten in Radiophysics and quantum electronics 52(2009), 4 vom: Apr., Seite 241-251 volume:52 year:2009 number:4 month:04 pages:241-251 |
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Radio Wave Electron Number Density Scattered Signal Linear Frequency Modulation Ionospheric Condition |
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530 |
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Radiophysics and quantum electronics |
authorswithroles_txt_mv |
Uryadov, V. P. @@aut@@ Vertogradov, G. G. @@aut@@ Vertogradov, V. G. @@aut@@ Kubatko, S. V. @@aut@@ Ponyatov, A. A. @@aut@@ Cherkashin, Yu. N. @@aut@@ Krasheninnikov, I. V. @@aut@@ Valov, V. A. @@aut@@ Komrakov, G. P. @@aut@@ Makarov, A. V. @@aut@@ Bredikhin, D. V. @@aut@@ |
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2009-04-01T00:00:00Z |
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author |
Uryadov, V. P. |
spellingShingle |
Uryadov, V. P. ddc 530 bkl 33.16 bkl 53.74 bkl 33.80 bkl 39.22 misc Radio Wave misc Electron Number Density misc Scattered Signal misc Linear Frequency Modulation misc Ionospheric Condition Sounding of an artificially perturbed ionosphere by means of an ionosonde/position finder with chirp modulation of the signal |
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530 620 ASE 33.16 bkl 53.74 bkl 33.80 bkl 39.22 bkl Sounding of an artificially perturbed ionosphere by means of an ionosonde/position finder with chirp modulation of the signal Radio Wave (dpeaa)DE-He213 Electron Number Density (dpeaa)DE-He213 Scattered Signal (dpeaa)DE-He213 Linear Frequency Modulation (dpeaa)DE-He213 Ionospheric Condition (dpeaa)DE-He213 |
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ddc 530 bkl 33.16 bkl 53.74 bkl 33.80 bkl 39.22 misc Radio Wave misc Electron Number Density misc Scattered Signal misc Linear Frequency Modulation misc Ionospheric Condition |
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ddc 530 bkl 33.16 bkl 53.74 bkl 33.80 bkl 39.22 misc Radio Wave misc Electron Number Density misc Scattered Signal misc Linear Frequency Modulation misc Ionospheric Condition |
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title |
Sounding of an artificially perturbed ionosphere by means of an ionosonde/position finder with chirp modulation of the signal |
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(DE-627)SPR017042496 (SPR)s11141-009-9136-9-e |
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Sounding of an artificially perturbed ionosphere by means of an ionosonde/position finder with chirp modulation of the signal |
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Uryadov, V. P. |
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Radiophysics and quantum electronics |
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Uryadov, V. P. Vertogradov, G. G. Vertogradov, V. G. Kubatko, S. V. Ponyatov, A. A. Cherkashin, Yu. N. Krasheninnikov, I. V. Valov, V. A. Komrakov, G. P. Makarov, A. V. Bredikhin, D. V. |
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530 620 ASE 33.16 bkl 53.74 bkl 33.80 bkl 39.22 bkl |
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Elektronische Aufsätze |
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Uryadov, V. P. |
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10.1007/s11141-009-9136-9 |
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530 620 |
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verfasserin |
title_sort |
sounding of an artificially perturbed ionosphere by means of an ionosonde/position finder with chirp modulation of the signal |
title_auth |
Sounding of an artificially perturbed ionosphere by means of an ionosonde/position finder with chirp modulation of the signal |
abstract |
We describe the operation of an ionosonde/position finder with chirp modulation of the signal. The first results of measuring the characteristics of short-wave radio signals scattered by artificial small-scale inhomogeneities, which were obtained by means of an ionosonde/position finder on the IZMIRAN—“SURA”—Rostov-on-Don path are presented. It was found that under certain ionospheric conditions, the angular and frequency selection of the scattered signals take place, in which case the signals are observed simultaneously in several frequency intervals (mainly, in three, namely, 6–9.5 MHz, 10–12 MHz, and 15–18 MHz) with different angles of incidence of radio waves in the vertical plane. In this case, the incidence angles were 20◦–35◦, 18◦–32◦, and 10◦–20◦ from the horizon for the first, second, and third frequency interval, respectively. Ionograms of oblique sounding were modeled allowing for the scattering of radio waves by artificial small-scale inhomogeneities. It is shown that at frequencies from 10 to 12 MHz, aspect conditions are fulfilled for the signals ducting along the high-angle beam (Pedersen mode). At frequencies 15–18 MHz (higher than the maximum observable frequency of the forward signal on the path IZMIRAN—Rostov-on-Don), aspect scattering conditions are fulfilled for the signals incident on a scattering area in the ascending part of the trajectory. At low frequencies 6–9.5 MHz (below the maximum observed frequency of the forward signal on the IZMIRAN—Rostov-on-Don path), the observable additional signals are caused by the scattering of radio waves by artificial inhomogeneities with subsequent relfection of the scattered signal from the Earth on the “SURA”—Rostov-on-Don path. |
abstractGer |
We describe the operation of an ionosonde/position finder with chirp modulation of the signal. The first results of measuring the characteristics of short-wave radio signals scattered by artificial small-scale inhomogeneities, which were obtained by means of an ionosonde/position finder on the IZMIRAN—“SURA”—Rostov-on-Don path are presented. It was found that under certain ionospheric conditions, the angular and frequency selection of the scattered signals take place, in which case the signals are observed simultaneously in several frequency intervals (mainly, in three, namely, 6–9.5 MHz, 10–12 MHz, and 15–18 MHz) with different angles of incidence of radio waves in the vertical plane. In this case, the incidence angles were 20◦–35◦, 18◦–32◦, and 10◦–20◦ from the horizon for the first, second, and third frequency interval, respectively. Ionograms of oblique sounding were modeled allowing for the scattering of radio waves by artificial small-scale inhomogeneities. It is shown that at frequencies from 10 to 12 MHz, aspect conditions are fulfilled for the signals ducting along the high-angle beam (Pedersen mode). At frequencies 15–18 MHz (higher than the maximum observable frequency of the forward signal on the path IZMIRAN—Rostov-on-Don), aspect scattering conditions are fulfilled for the signals incident on a scattering area in the ascending part of the trajectory. At low frequencies 6–9.5 MHz (below the maximum observed frequency of the forward signal on the IZMIRAN—Rostov-on-Don path), the observable additional signals are caused by the scattering of radio waves by artificial inhomogeneities with subsequent relfection of the scattered signal from the Earth on the “SURA”—Rostov-on-Don path. |
abstract_unstemmed |
We describe the operation of an ionosonde/position finder with chirp modulation of the signal. The first results of measuring the characteristics of short-wave radio signals scattered by artificial small-scale inhomogeneities, which were obtained by means of an ionosonde/position finder on the IZMIRAN—“SURA”—Rostov-on-Don path are presented. It was found that under certain ionospheric conditions, the angular and frequency selection of the scattered signals take place, in which case the signals are observed simultaneously in several frequency intervals (mainly, in three, namely, 6–9.5 MHz, 10–12 MHz, and 15–18 MHz) with different angles of incidence of radio waves in the vertical plane. In this case, the incidence angles were 20◦–35◦, 18◦–32◦, and 10◦–20◦ from the horizon for the first, second, and third frequency interval, respectively. Ionograms of oblique sounding were modeled allowing for the scattering of radio waves by artificial small-scale inhomogeneities. It is shown that at frequencies from 10 to 12 MHz, aspect conditions are fulfilled for the signals ducting along the high-angle beam (Pedersen mode). At frequencies 15–18 MHz (higher than the maximum observable frequency of the forward signal on the path IZMIRAN—Rostov-on-Don), aspect scattering conditions are fulfilled for the signals incident on a scattering area in the ascending part of the trajectory. At low frequencies 6–9.5 MHz (below the maximum observed frequency of the forward signal on the IZMIRAN—Rostov-on-Don path), the observable additional signals are caused by the scattering of radio waves by artificial inhomogeneities with subsequent relfection of the scattered signal from the Earth on the “SURA”—Rostov-on-Don path. |
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title_short |
Sounding of an artificially perturbed ionosphere by means of an ionosonde/position finder with chirp modulation of the signal |
url |
https://dx.doi.org/10.1007/s11141-009-9136-9 |
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author2 |
Vertogradov, G. G. Vertogradov, V. G. Kubatko, S. V. Ponyatov, A. A. Cherkashin, Yu. N. Krasheninnikov, I. V. Valov, V. A. Komrakov, G. P. Makarov, A. V. Bredikhin, D. V. |
author2Str |
Vertogradov, G. G. Vertogradov, V. G. Kubatko, S. V. Ponyatov, A. A. Cherkashin, Yu. N. Krasheninnikov, I. V. Valov, V. A. Komrakov, G. P. Makarov, A. V. Bredikhin, D. V. |
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doi_str |
10.1007/s11141-009-9136-9 |
up_date |
2024-07-04T01:59:22.471Z |
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score |
7.400276 |