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user:kurser:ham_vt2023_l7 [2023/02/12 16:56] useruser:kurser:ham_vt2023_l7 [2023/04/11 08:44] user
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 [[user:kurser:ham_vt2023|Back to course information]] [[user:kurser:ham_vt2023|Back to course information]]
  
-Recommended reading: KonCEPT page 191-229 (chapter 7 + 8) +**Recommended reading: KonCEPT page 191-229 (chapter 7 + 8) **
  
 +Start with transmission line (TL), the most difficult component. 
 +
 +characterized by: Characteristic impedance, Z_0, a geometry and material parameter. Length and the speed of light in the transmission line. Two metal conductors that guide the fields. 
 +
 +Used for high frequency signals. Lambda = 300/f [MHz], Lambda similar to length in size. 
 +
 +Waves propagate along transmission lines. Reflections along a TL are similar to light in a glass/water. Explain transmission/reflection coefficients. 
 +
 +Reflections cause standing waves and non-optimal power transfer/losses 
 +
 +VSWR = Voltage Standing Wave Ratio = Z1/Z2 OR Z2/Z1 so a x:1 relation is formed. 
 +
 +We want to "match" the antenna, transmission line and radio to minimize losses. 
 +
 +Balanced/unbalanced (differential/single-ended) TL are important and difficult. Explain this in detail.  
 +
 +balanced TL folded out -> dipole antenna! Nice SWR achieved. L = lambda/2 = 300/(2*f) ~=(0,96*lambda/2)
 +
 +==Antennas==
 +
 +Antenna = two port that converts energy from propagating in a transmission line to propagation in free-space. 
 +
 +Characterized by: 
 +  * Input impedance, SWR, Z_in
 +  * Operation frequency, resonance frequency, f_0
 +  * Directivity D, antenna gain, dBi, dBd 
 +  * far field distance = d_f > 2*D^2/lambda, given d_f >> D, d_f >> lambda
 +  * Radiation efficiency, eta
 +  * radiation pattern, E & H patterns
 +  * Polarization and x-pol suppression and so on...
 +
 +We can only measure input impedance and operational frequency easily with a VNA/Antena analyzer ... so lets do that at ETA. 
 +
 +Different types
 +  * Dipole
 +  * Monopole
 +  * Small loop
 +  * Yagi
 +  * Quad
 +  * Patch
 +  * Bowtie
 +  * PCB/PIFA
 +  * Spiral/Helical
 +
 +Talk about polarization. 
 +
 +Common mode current on coax = bad!
 +
 +== Propagation ==
 +
 +**HF/short wave**
 +
 +  1) Ground wave (20-40 km typical)
 +  2) Space wave (global range)
 +    * Reflections from the ionosphere's D, E, F regions. Sunlight ionize the ionosphere.
 +    * Reflections affect polarization chaotically.
 +    * D = 60-90 km height. 
 +      * "Dämpningsskiktet" attenuates signals
 +      * Only daytime
 +      * Attenuate <10MHz
 +    * E = 90-110 km
 +    * F = F1 + F2 = 150-350 km - reflection. 
 +      * Reflect <30-50MHz depending on sun activity
 +      * Created during daytime, slow to unionize
 +
 +**3.5-7 MHz**
 +  * Attenuated by D
 +  * skyward wave/antenna can reflect back to local contacts (E/F)
 +  
 +**14-30 MHz**
 +  * Not really affected by D
 +  * skyward wave/antenna cannot reflect back to local contacts (E/F)
 +  * Sporadic-E might enable local connections
 +
 +DX -> 10 degree max antenna gain is best
 +
 +**VHF/UHF/...**
 +  * Penetrates the atmosphere, EME possible
 +  * Basically only local line-of-sight connections possible
 +  * Troposphere propagation possible. Heat and humidity gradients guide waves. Ex. hearing Danish FM radio in Göteborg. 
 +  * northern lights reflections >25 MHz. Distorts signals, phone sounds creepy.
 +  * Moon/meteor/satellite/airplane scatter
 +    * Reflect signals from big things
 +
 +**Microwaves**
 +  * Moon/meteor/satellite/airplane scatter
 +    * Reflect signals from big things
 +    * Also rain scatter
 +
 +Fading example with cellphone if possible 
 +
 +
 +Radio Antenna Fundamentals Part 1 1947
 +
 +https://www.youtube.com/watch?v=JHSPRcRgmOw&ab_channel=GerryTrenwith 
  
user/kurser/ham_vt2023_l7.txt · Last modified: 2024/02/13 18:08 by user