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Articoli di riviste sul tema "Radio waves"

Autore: Grafiati

Pubblicato: 4 giugno 2021

Ultima modifica: 25 luglio 2025

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1

Hodkinson, Liam, and Elizabeth Stitt. "Radio Waves." Index on Censorship 39, no. 2 (2010): 49–50. http://dx.doi.org/10.1177/03064220100390021001.

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2

Apple, Jacki, Regine Beyer, and Richard Kostelanetz. "Making Radio Waves." TDR (1988-) 36, no. 2 (1992): 7. http://dx.doi.org/10.2307/1146189.

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3

Rakusen, Sam. "Making radio waves!" Primary Teacher Update 2013, no. 18 (2013): 53. http://dx.doi.org/10.12968/prtu.2013.1.18.53b.

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4

O'Sullivan, Mike. "Making radio waves." A Life in the Day 10, no. 2 (2006): 6–8. http://dx.doi.org/10.1108/13666282200600013.

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5

Dyson, Frances. "Radio Art in Waves." Leonardo Music Journal 4 (1994): 9. http://dx.doi.org/10.2307/1513174.

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6

Dixon, E. "Radio waves of progress." Engineering & Technology 4, no. 5 (2009): 40–41. http://dx.doi.org/10.1049/et.2009.0506.

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7

Wait, J. R. "Propagation Of Radio Waves." IEEE Antennas and Propagation Magazine 40, no. 2 (1998): 88. http://dx.doi.org/10.1109/map.1998.683546.

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8

Friebele, Elaine. "“Seeing” with radio waves." Eos, Transactions American Geophysical Union 78, no. 30 (1997): 310. http://dx.doi.org/10.1029/97eo00203.

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9

Storey, L. R. O. "Natural VLF radio waves." Planetary and Space Science 37, no. 8 (1989): 1021–22. http://dx.doi.org/10.1016/0032-0633(89)90058-5.

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10

Jones, Dyfrig. "Natural VLF Radio Waves." Journal of Atmospheric and Terrestrial Physics 51, no. 2 (1989): 151. http://dx.doi.org/10.1016/0021-9169(89)90116-5.

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11

DeWALD, ERICH. "Taking to the Waves: Vietnamese society around the radio in the 1930s." Modern Asian Studies 46, no. 1 (2011): 143–65. http://dx.doi.org/10.1017/s0026749x11000606.

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AbstractCompared with other public media, the colonial state showed a relative lack of interest in radio broadcasting, which developed in Vietnam in the 1930s under the aegis of two organizations based in Hanoi and Saigon, the Radio-Club de l'Indochine du Nord and Radio Saigon. These two groups were largely responsible for the new technology's expansion and for determining the content of broadcasting. The groups actively consulted the growing radio public, and that vocal audience played a role in determining not just what was heard but also in the social life of radio in late-colonial Vietnam.

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12

Bokoyo Barandja, Vinci de Dieu, Bernard Zouma, Auguste Oscar Mackpayen, Martial Zoungrana, Issa Zerbo, and Dieudonné Joseph Bathiebo. "Propagation of Electromagnetic Wave into an Illuminated Polysilicon PV Cell." International Journal of Antennas and Propagation 2020 (January 30, 2020): 1–7. http://dx.doi.org/10.1155/2020/6056712.

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The increasing cohabitation between telecommunication antennas generating electromagnetic waves and solar panels poses the problem of interaction between these radio waves and solar cells. In order to study the effect of radio waves on the performance of a polycrystalline silicon solar cell in a three-dimensional approach, it is necessary to assess the attenuation of the radio wave in the illuminated polysilicon grain and also to find the expressions of its components. This work investigated the attenuation of radio waves into a polycrystalline silicon grain by analyzing, firstly, the behaviou

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13

Lutfi Apriyadi, Sabila Sofyana Zahra, Sabrina Nadya Octaviani, and Diyajeng Luluk Karlina. "Analisis Pengaplikasian Medan Elektromagentik Terhadap Gelombang Radio Frekuensi Tinggi." Venus: Jurnal Publikasi Rumpun Ilmu Teknik 2, no. 6 (2024): 150–58. https://doi.org/10.61132/venus.v2i6.636.

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The electromagnetic field on high-frequency radio waves and its impact on signal transmission quality. High-frequency radio waves, used in wireless communication, can be affected by electromagnetic fields from various external sources, such as electronic equipment and building structures. This study analyzes the interaction between electromagnetic fields and radio waves, as well as their impact on transmission speed and signal range. The analysis results show that electromagnetic fields can cause distortion or interference in radio waves, affecting the quality of the received signal. This stud

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14

Lyubarskii, Yu E. "Generation of pulsar radio emission." International Astronomical Union Colloquium 177 (2000): 387–88. http://dx.doi.org/10.1017/s0252921100060073.

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AbstractThe generation of radio emission from plasma waves excited by two-stream instability in pulsar magnetospheres is considered. Induced scattering transforms the excited longitudinal waves into waves that escape freely in the form of transverse electromagnetic waves. It is shown that the spectrum and the luminosity of the generated radio emission are compatible with those observed.

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15

Vasilev, Dragomir. "PROTECTION AGAINST THE ELECTROMAGNETIC STRENGTH OF THE RADIO WAVES IN COMMUNICATION RADIO NETWORKS." Journal Scientific and Applied Research 22, no. 1 (2023): 50–55. http://dx.doi.org/10.46687/jsar.v22i1.340.

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In this paper presents protection methods against Electromagnetic straight of the radio waves in communication radio networks. Examples of personal protective equipment for monitoring EMF when working near transmitting devices. Personal Monitor. When an electric current flows through the human body, cells and tissues prevent the movement of charged particles. The value of the resistance depends on the type and condition of the cells, the value and frequency of the applied voltage and the duration.

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16

Shoji, Eiichi. "Development and Performance of a Battery-Free Disaster Prevention Radio “HOOPRA” Using the Energy Harvested from Radio Waves." Journal of Disaster Research 11, no. 3 (2016): 593–98. http://dx.doi.org/10.20965/jdr.2016.p0593.

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A battery-free radio receiver, HOOPRA (<span class=”underline”>hoop</span> type <span class=”underline”>ra</span>dio), is proposed for acquiring information using middle wave AM radio broadcasting during unexpected power failures or disasters, with emphasis on wide coverage, immediate information acquisition, and energy saving. The HOOPRA utilizes middle waves for energy harvesting. As this radio is intended for use during disasters, the protection methods, receiving performance, and the applications of energy harvesting are reported in this paper. The HOOPRA is ring-sh

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17

Farah, Wahaj, and Vinay M. "Electromagnetic Waves - Functionality, Types and Uses." Journal of VLSI Design and its Advancement 4, no. 3 (2022): 1–4. https://doi.org/10.5281/zenodo.6344058.

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<em>Radio waves are a form of electromagnetic radiation with wavelengths longer than infrared radiation in the electromagnetic spectrum. It consists of electromagnetic waves with the longest wavelengths, often at frequency of 300 gigahertz (GHz) or less. The corresponding wavelength at 300 GHz is 1 mm (shorter than a grain of rice), while the analogous wavelength at 30 Hz is 10,000 km (longer than the radius of the Earth). Radio waves, like other electromagnetic waves, travel at the speed of light in a vacuum and at a somewhat slower speed in the Earth's atmosphere. Charged particles under

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18

Chernov, Gennady, and Valery Fomichev. "On the Issue of the Origin of Type II Solar Radio Bursts." Astrophysical Journal 922, no. 1 (2021): 82. http://dx.doi.org/10.3847/1538-4357/ac1f32.

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Abstract Type II solar radio bursts are among the most powerful events in the solar radio emission in the meter wavelength range. It is generally accepted that the agents generating type II radio bursts are magnetohydrodynamic shock waves. But the relationship between the shock waves and the other manifestations of the large-scale disturbances in the solar atmosphere (coronal mass ejections, Morton waves, EUW waves) remains unclear. To clarify a problem, it is important to determine the conditions of generation of type II radio bursts. Here, the model of the radio source is based on the genera

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19

Ohtsuki, Tomoaki. "Monitoring Techniques with Radio Waves." IEICE Communications Society Magazine 11, no. 1 (2017): 24–29. http://dx.doi.org/10.1587/bplus.11.24.

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20

Lopez, Luciana. "Virtual Barcodes Use Radio Waves." JALA: Journal of the Association for Laboratory Automation 3, no. 2 (1998): 13–15. http://dx.doi.org/10.1177/221106829800300205.

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The wrong additive in a specimen vial, for example, could not only give completely invalid results, it could also waste a given sample. While the automation, robotics, and electronics industries have been consistently helping laboratories improve identification and classification problems over the years, there has always been room for improvement. Now, however, a new technology stands poised to take identification solutions to a new level: radio frequency identification.

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21

Lewis, Sian. "The power of radio waves." Nature Reviews Neuroscience 16, no. 10 (2015): 578. http://dx.doi.org/10.1038/nrn4031.

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22

Osborne, Ian S. "Going quantum with radio waves." Science 363, no. 6431 (2019): 1052.14–1054. http://dx.doi.org/10.1126/science.363.6431.1052-n.

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23

Chalmers, Matthew. "Radio waves measure body water." Physics World 16, no. 3 (2003): 26–27. http://dx.doi.org/10.1088/2058-7058/16/3/38.

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24

Barclay, L. W. "The Propagation of Radio Waves." Electronics and Power 32, no. 8 (1986): 610. http://dx.doi.org/10.1049/ep.1986.0365.

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25

Barr, R., D. Llanwyn Jones, and C. J. Rodger. "ELF and VLF radio waves." Journal of Atmospheric and Solar-Terrestrial Physics 62, no. 17-18 (2000): 1689–718. http://dx.doi.org/10.1016/s1364-6826(00)00121-8.

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26

Adawi, I. "Centennial of Hertz’ radio waves." American Journal of Physics 57, no. 2 (1989): 125–27. http://dx.doi.org/10.1119/1.16106.

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27

Cairns, R. A., A. Kay, and A. W. Taylor. "Absorption of radio-frequency waves." Plasma Physics and Controlled Fusion 30, no. 1 (1988): 11–19. http://dx.doi.org/10.1088/0741-3335/30/1/003.

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28

Bates, D. R. "The propagation of Radio Waves." Planetary and Space Science 34, no. 6 (1986): 573. http://dx.doi.org/10.1016/0032-0633(86)90097-8.

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29

Bougeret, J. L. "Radio waves in the heliosphere." Advances in Space Research 13, no. 6 (1993): 191–203. http://dx.doi.org/10.1016/0273-1177(93)90409-5.

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30

Misra, Sanjai, and K. K. Bajpai. "Radio Waves and Living world." Anusandhaan - Vigyaan Shodh Patrika 9, no. 1 (2021): 21–23. https://doi.org/10.22445/avsp.v9i1.4.

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Abstract (sommario):

Electromagnetic field and radio waves are produced by many daily used gazettes like Microwave, washing machine, mobile etc. It adversely affects the human health as well as other living organisms. Present paper discusses the Physiology and Mechanism of harmful effects caused by electromagnetic field and radio waves .

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31

Mann, G., C. Vocks, and A. Warmuth. "Type III radio bursts and excitation of Langmuir waves by energetic electrons." Astronomy & Astrophysics 660 (April 2022): A91. http://dx.doi.org/10.1051/0004-6361/202142804.

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Context. Solar activity occurs not only in terms of the well-known 11-year Sun spot cycle but also in terms of short-lived phenomena as radio bursts. For instance, type III radio bursts are the most common phenomenon of this activity in the Sun’s radio radiation. In dynamic radio spectra, they appear as short-lived stripes of enhanced radio emission rapidly drifting from high to low frequencies. They are regarded as the radio signature of beams of energetic electrons travelling along magnetic field lines in the corona. The radio emission is thought to be plasma emission, that is to say the rad

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32

Zhang, Ze-Lin, and Ruo-Yu Liu. "The Twisting of Radio Waves in a Randomly Inhomogeneous Plasma." Astrophysical Journal 975, no. 2 (2024): 260. http://dx.doi.org/10.3847/1538-4357/ad7d0a.

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Abstract Polarization of electromagnetic waves carries a large amount of information about their astrophysical emitters and the media they passed through, and hence is crucial in various aspects of astronomy. Here we demonstrate an important but long-overlooked depolarization mechanism in astrophysics: when the polarization vector of light travels along a nonplanar curve, it experiences an additional rotation, in particular for radio waves. The process leads to depolarization, which we call “geometric” depolarization (GDP). We give a concise theoretical analysis of the GDP effect on the transp

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33

Pleukhov, A. N. "Nonreciprocity of radio waves in a meteor radio channel." Radiophysics and Quantum Electronics 31, no. 5 (1988): 395–99. http://dx.doi.org/10.1007/bf01043601.

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34

Avdzeyko, V. I., V. I. Karnyshev, R. V. Meshcheryakov, and E. S. Paskal. "Patent analysis: revealing the promising trends in the advancement of radio electronic systems using the reflection or reradiation of radio waves." Radio industry 29, no. 1 (2019): 53–60. http://dx.doi.org/10.21778/2413-9599-2019-29-1-53-60.

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To identify the promising (breakthrough) trends in the advancement of radio electronic systems with the use of US Patents and Trademark Office database this paper examines the possibilities of patent analysis. This method is based on automatic time series generation of US patents for inventions and subsequent comparison of different technical solutions in specific International Patent Classification subgroups, and in their issuance dynamics for 2007-2017. In particular, the authors analyze several promising trends in the advancement of radio electronic systems using the reflection or secondary

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35

Mann, G., C. Vocks, A. Warmuth, et al. "Excitation of Langmuir waves at shocks and solar type II radio bursts." Astronomy & Astrophysics 660 (April 2022): A71. http://dx.doi.org/10.1051/0004-6361/202142201.

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Context. In the solar corona, shocks can be generated due to the pressure pulse of a flare and/or driven by a rising coronal mass ejection (CME). Coronal shock waves can be observed as solar type II radio bursts in the Sun’s radio radiation. In dynamic radio spectra, they appear as stripes of an enhanced radio emission slowly drifting from high to low frequencies. The radio emission is thought to be plasma emission, that is to say the emission happens near the electron plasma frequency and/or its harmonics. Plasma emission means that energetic electrons excite Langmuir waves, which convert int

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36

Füllekrug, M., C. Hanuise, and M. Parrot. "Simulating satellite observations of 100 kHz radio waves from relativistic electron beams above thunderclouds." Atmospheric Chemistry and Physics Discussions 10, no. 10 (2010): 23149–67. http://dx.doi.org/10.5194/acpd-10-23149-2010.

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Abstract. Relativistic electron beams above thunderclouds emit 100 kHz radio waves which illuminate the Earth's atmosphere and near-Earth space. This contribution aims to clarify the physical processes which are relevant for the spatial spreading of the radio wave energy below and above the ionosphere and thereby enables simulating satellite observations of 100 kHz radio waves from relativistic electron beams above thunderclouds. The simulation uses the DEMETER satellite which observes 100 kHz radio waves from fifty terrestrial Long Range Aid to Navigation (LORAN) transmitters. Their mean lumi

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37

Füllekrug, M., C. Hanuise, and M. Parrot. "Experimental simulation of satellite observations of 100 kHz radio waves from relativistic electron beams above thunderclouds." Atmospheric Chemistry and Physics 11, no. 2 (2011): 667–73. http://dx.doi.org/10.5194/acp-11-667-2011.

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Abstract. Relativistic electron beams above thunderclouds emit 100 kHz radio waves which illuminate the Earth's atmosphere and near-Earth space. This contribution aims to clarify the physical processes which are relevant for the spatial spreading of the radio wave energy below and above the ionosphere and thereby enables an experimental simulation of satellite observations of 100 kHz radio waves from relativistic electron beams above thunderclouds. The simulation uses the DEMETER satellite which observes 100 kHz radio waves from fifty terrestrial Long Range Aid to Navigation (LORAN) transmitte

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38

Chimeh, Jahangir Dadkhah, Saeed Bashirzadeh Parapari, and Seyed Mohmoud Mousavinejad. "Millimetric Waves Technologies: Opportunities and Challenges." Key Engineering Materials 500 (January 2012): 263–68. http://dx.doi.org/10.4028/www.scientific.net/kem.500.263.

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Providing an available wideband and better antenna beam forming are two good profits of millimeter wave (mmWave) technology. MmWave technology makes radio systems lighter and smaller and radars more precise. Today, commercial MmWave equipment work below 90GHz frequencies. MmWave radios work to transport Internat traffic in the backhaul of communication networks. There is a challenge in mmWave technology since the prices of equipment increases as the frequency increases. In this paper we study the applications of mmWave technology, its products, standards and compare it with other wireless tech

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39

Krasheninnikov, I. V., and V. N. Shubin. "Features of Forecasting the Operation of Ionospheric Radio Lines in Upper Rays Modes." Геомагнетизм и аэрономия 63, no. 4 (2023): 473–80. http://dx.doi.org/10.31857/s0016794023600096.

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The frequency dependence of transmitted information qualitative indicators is analyzed on theexample of two meridional radio links: single-hop (~2600 km) and dominant two-hop (~5100 km) for basicmodes of radio wave propagation in the ionosphere. It is shown that the presence of highly efficient receivingtransmittingantennas in a radio communication system leads to the need to take the existence of a priori energeticallyextremely weak modes into account in the problem of radio path specification statement. In thiscase, we consider those formed exclusively by the mechanism of radiation transfer

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40

FABRIKANT, A. L., V. Yu TRAKHTENGERTS, Yu G. FEDOSEEV, V. O. RAPOPORT, and V. A. ZINICHEV. "Radio-acoustic sounding of the troposphere using short radio waves." International Journal of Remote Sensing 15, no. 2 (1994): 347–60. http://dx.doi.org/10.1080/01431169408954078.

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41

Sugimoto (Stray Cats), Norihiro. "Looking for radio waves with a simple radio wave detector." Physics Teacher 49, no. 8 (2011): 514–15. http://dx.doi.org/10.1119/1.3651739.

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42

Chandra, Isita, Arnab Ghosh, Ayan Chatterjee, and Rajiv Ganguly. "Tracking and analysis of solar radio waves using a low-cost Radio Telescope in urban areas." EPJ Web of Conferences 325 (2025): 01009. https://doi.org/10.1051/epjconf/202532501009.

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Radio telescopes are specialized instruments to detect radio-waves between 30MHz-300GHz from different astronomical sources. It has ability to capture radio signals from satellites effectively during high light pollution and cloudy weather. In Kolkata, light pollution being significant, radio telescopes offer an alternative to optical telescopes for signal tracking from different radio sources. Although radio telescopes are typically expensive devices, here the main objective is to develop a low-cost, user-friendly model by using dish antenna, connecting cables, low-cost satellite meter (SF720

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43

Cartlidge, Edwin. "Radio offers view of gravitational waves." Physics World 34, no. 2 (2021): 5. http://dx.doi.org/10.1088/2058-7058/34/02/05.

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44

Purwadi, A., and D. T. Utomo. "Radio waves-based landslide mitigation system." IOP Conference Series: Earth and Environmental Science 672, no. 1 (2021): 012081. http://dx.doi.org/10.1088/1755-1315/672/1/012081.

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45

Wilkie, Bill. "The Daintree Blockade: Making (radio) waves." Queensland Review 28, no. 2 (2021): 166–68. http://dx.doi.org/10.1017/qre.2022.13.

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Radio log 11/8/84D5 crossing creek under Timbertop’s tree … continues to fill the creek crossing … If he continues to fill it high enough the D10 should go through. Looks like a moonscape where the dozers are working.

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46

SHINOHARA, Naoki. "Energy Harvesting from Radio Waves（Rectenna）." Journal of the Surface Finishing Society of Japan 67, no. 7 (2016): 353–56. http://dx.doi.org/10.4139/sfj.67.353.

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Aydin, Ulkem. "From radio waves to gamma rays." Journal of Oral and Maxillofacial Radiology 1, no. 3 (2013): 93. http://dx.doi.org/10.4103/2321-3841.126676.

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48

Bradley, Richard. "The many uses of radio waves." Physics Today 72, no. 5 (2019): 60–61. http://dx.doi.org/10.1063/pt.3.4206.

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Warrington, E. M., and T. B. Jones. "Propagation of low-frequency radio waves." IEE Proceedings - Microwaves, Antennas and Propagation 147, no. 1 (2000): 35. http://dx.doi.org/10.1049/ip-map:20000172.

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Peterson, I. "Detecting Jupiter's Tug on Radio Waves." Science News 140, no. 19 (1991): 294. http://dx.doi.org/10.2307/3975910.

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