Длинноволновики всех стран объединяйтесь!LW-mans of all countries unite!
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Увы, архив Радио охватывает только старые номера, до 2000 года.
дойдёт до практической космической реализации
В статье показано, что сигналы диапазона 136 кГц могут распространяться сквозь ионосферу и выходить в космос в режиме свистовых волн (как свистящие атмосферики на сверхдлинных волнах).
Good morning...As some of you may be aware, Jim Hollander, W5EST, providedobservations and analysis of on air occurrences that were reported onmy 630 meter daily blog for several years. Much of that informationwas compiled into volumes (4 volumes now), organized by years to showthe progression on the band.While I've never tracked 2200 meter activity like I did for 630meters, Jim accepted the task of reviewing data found on the Internetand from email interviews and discussions with participants whowitnessed or were party to some amazing openings on 2200m. He has nowreleased a compilation for 2200 meters. The table of contents, withlinks, is listed below and is also posted in the bio on my QRZ.compage for future reference.Jim reads these email reflectors and I am sure would appreciatecomments and feed back for his efforts.73 and TOC to follow below,John Langridge KB5NJD*******YOUR 2200M 2015-2022 COMPILATION BOOKCompiled by James F. Hollander W5ESTTABLE OF CONTENTSPART I: START BY RECEIVING 2200M!Preface & Chapter 1: Distinguishing 2200 Meters Compared to 630 Metershttps://drive.google.com/file/d/1fb4L1nYUap_utJBsM4O6A7ROHORZ5qaX/view?usp=sharingChapter 2: Receiving Antennas for 2200 Meters, and Noise Reductionhttps://drive.google.com/file/d/1feolTRt-IaOpHCwVra_9eyzmcOjil_hb/view?usp=sharingChapter 3: 2200m Receivers and Decoders for 2200m Modeshttps://drive.google.com/file/d/1iqwnBhafobRQ0IrhluMpApTzIYOqyBFp/view?usp=sharing2200m Operating Modes and How to Receive ThemChapter 5.1: WSPR, FST4W, Opera(EU)https://drive.google.com/file/d/1fYLlmVOndwbHnCC4O6tSRDsOY41F7Adp/view?usp=sharingChapter 5.2: CW, DFCW, QRSShttps://drive.google.com/file/d/1IbmlvEp9OQIs7XSumyDRa5bPEW16hU-6/view?usp=sharingChapter 5.3: General QSO Operations, FST4, JT9, Theoryhttps://drive.google.com/file/d/1xz_TQ7vFOYZ4BRNP8eCe8Nwi8_55nc2E/view?usp=sharingChapter 5.4: EbNaut HW/SW, EbNaut Operationshttps://drive.google.com/file/d/1rdjzVJVWmVonoDNEWSpNh3mF8Nbiargi/view?usp=sharingChapter 6: Storm Safety, Band Noise, GMF & Space Weatherhttps://drive.google.com/file/d/11n4hhUwWv8lyBHlVjjBWo16Pl9SvnD1k/view?usp=sharingChapter 7: Common Darkness and 2200m Pathshttps://drive.google.com/file/d/1TYeZKZZ4KC3U7T3ncFcs4VeUHCoYXWYf/view?usp=sharingPART II: YOUR 2200M TRANSMITTING STATIONChapter 9.1: 2200m Paths – Short and Medium—Ops Experiencehttps://drive.google.com/file/d/1xwvyOsYPhK6MddWPF_Lv8XfAyO-NP8AS/view?usp=sharingChapter 9.2: 2200m Paths – Short and Medium—Theoryhttps://drive.google.com/file/d/1Ia_-miX5gE_YOD7BjhXmB7kW5q2JVmuA/view?usp=sharingChapter 10: 2200m Transmit Antennashttps://drive.google.com/file/d/1whgUO0JZGc7oytYpItfCzhiEd8uU-6tF/view?usp=sharingChapter 10.1: 4000m+ (Part 5) Operations and Antennashttps://drive.google.com/file/d/1hyeTyne4BROJjj9UFVMGUeLNNqOL7JOx/view?usp=sharingChapter 13: 2200m Transmitters, RF Power Amplifiers, ATUshttps://drive.google.com/file/d/1C2P8EufaRy1b9VZqENsrs2rPNQPtQgvN/view?usp=sharingChapter 15: 2200m Around Sunrisehttps://drive.google.com/file/d/1IDmlmj-ahfryzLFT68s-kyDHN_kelb07/view?usp=sharingPART IIIA: 2200m PROPAGATION, VARIABILITY, AND MYSTERIES2200m Propagation on Long Haul PathsChapter 17.1: N. America To/From Europe/Africa, Prop Conceptshttps://drive.google.com/file/d/1LafGot5DaNXGpuA5MNLW7cgiw6IMqRvr/view?usp=sharingChapter 17.2: Europe – East Asia/ VK/ ZLhttps://drive.google.com/file/d/1VH5PjIejSQFPzMuDLQ9f6A1iXEpy_fDA/view?usp=sharingChapter 17.3: VK/ZL To/From Asia Pacific & N.America, N.Am.-JA/E.Asiahttps://drive.google.com/file/d/1kYbq_qluQEdbyzeFLBV8mMKiIiJFDVZ0/view?usp=sharingChapter 17.4: To/From South America; To/From Africa/Indian Oceanhttps://drive.google.com/file/d/1DjM3180UyFzdFrwYwz523Z2K_OeSKXzO/view?usp=sharingChapter 18: 2200m Fading and QSB Measurementshttps://drive.google.com/file/d/1pvN_09_AbhiDO-vUU_PN6g6VU-J-BvrF/view?usp=sharing2200m Propagation During DaytimeChapter 19.1: 2200m Daytime: Sky Wave, Ground Wavehttps://drive.google.com/file/d/1EuWL21NExPHoRI7_dvWxnenv2xtPOaTU/view?usp=sharingChapter 19.2: 2200m During Solar Flares, Solar Eclipse, or Earthquakehttps://drive.google.com/file/d/1QTkCqXX2t_E7xG4xgND9PqZovyks3HG9/view?usp=sharingAppendicesAppendix I-A: 2200m SNR Sequenceshttps://drive.google.com/file/d/1a4XCJEN3nDcJ2PEYODUJV_UeVmthq1zK/view?usp=sharingAppendix I-B: 4000m SNR Comparisonhttps://drive.google.com/file/d/179tmU7BtFeS-SzAXWKS0gVN6h1YU_CNv/view?usp=sharingAppendix I-C: 2200m Flares, Eclipse, Earthquakehttps://drive.google.com/file/d/1a1S3SPrF7Tmua9TJhY_MuGFzny7yFyHK/view?usp=sharingAppendix II: Comparing 2200m with 630m and Other MF bandshttps://drive.google.com/file/d/1Ko6i9VHeYb7udKPqeQXncPWHfQN0Bivc/view?usp=sharingAppendix III: Some 2200m Active TX or RX Stationshttps://drive.google.com/file/d/1Q_tEXRRrHEsFaE2rSXUlcf0gjHXFsNp-/view?usp=sharing Appendix IV: Some Digimode Softwarehttps://drive.google.com/file/d/1uOlims03fEMZJZFNJUZ2oSnOg_uOdJae/view?usp=sharing
