Microwave EME by Al Ward W5LUA

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Transcription:

EME by Al Ward W5LUA Ham-Com June 8, 2007 WWW..ORG 1

The Bands Band Frequency Range Weak signal work in NA 33 cm 902 to 928 MHz 902 MHz 23 cm 1240 to 1300 MHz 1296 MHz 13 cm 2300 to 2310 MHz 2304 MHz 2390 to 2450 MHz 9 cm 3300 to 3500 MHz 3456 MHz 6 cm 5650 to 5925 MHz 5760 MHz 3 cm 10000 to 10500 MHz 10368 MHz 1.25cm 24000 to 24250 MHz 24192 MHz and 24048 MHz.6 cm 47000 to 47200 MHz 47088 MHz.35 cm 77000 to 81000 MHz allocation changing Not all countries have same allocation as us.. WWW..ORG 2

902 to 928 MHz Shared by Region 1 only Includes US and Canada 10 Stations operational over the years Station Requirements 3m Dish with dual dipole feed, 150 watts from 2C39s, or 150/300/600 watt solid state amplifiers Active stations include K5JL, WA5ETV, W5LUA, K2DH, W0RAP,WB0TEM, VE4MA, NU7Z, WA8WZG, AND AF1T Interference from ISM and part 15 devices is a real problem on this band Operation by appointment only! WWW..ORG 3

1240 to 1300 MHz World wide allocation Primary operation between 1296.0 and 1296.1 MHz CW and SSB 200+ stations operational Digital modes being explored JT-44 initially, however JT-65C is used presently Minimum Station Requirements 3m Dish with VE4MA or Septum type circular polarized feed and 150 watts from 2C39s or GS15b Big stations run 7 or 8 meter dishes and kw plus from TH-327/347 or YL-1050 This is an excellent random CW band WWW..ORG 4

OH3MCK on 1296 MHz JT-65C 4 Yagis 27 dbi 200 watts WWW..ORG 5

www.emeham.com/1296/ WWW..ORG 6

2300-2310 and 2390-2450 MHz Most operation between 2304.0 and 2304.150 MHz UK can only operate at 2320 MHz - no allocation at 2304 MHz Japanese operate at 2424 MHz - no allocation at 2304 MHz 2320 MHz is primary terrestrial frequency in Europe Crossband operation requires extra receive converters 50+ stations operational Station Requirements 3m Dish, circular polarization,100 watts WWW..ORG 7

Path Loss According to the Radar equation, the path loss increases by 6 db every time the frequency is doubled However dish gain also increases by 6 db every time frequency is doubled Since we gain the same 6dB on both receive and transmit and assuming we use the same power and the same NF as we go up in frequency, our echoes will improve as frequency is increased this is in fact what we see! WWW..ORG 8

WD5AGO 8ft Dish for 2304 MHz WWW..ORG 9

WA5WCP 10ft Dish for 2304 MHz WWW..ORG 10

3300 to 3500 MHz Most operation between 3456.0 and 3456.1 MHz Not a world wide allocation Operation from Germany and Luxembourg on 3456 MHz, UK coming soon Finland operation on 3408 MHz W5LUA worked OH2AXH on 3408 MHz Stations that have been operational include K2DH, W7CNK, K0KE, W5LUA, DL9EBL, VE4MA, NU7Z, OH2AXH, LX1DB, OK1CA, WA9FWD, AND G4NNS G3LTF and WW2R working towards being operational Station Requirements 3M Dish, 50 watts, linear polarity has been used horizontal in NA and vertical in Europe most active stations migrating to circular polarization to avoid spatial offset problem Activity must be coordinated as random activity is nil WWW..ORG 11

5650 to 5925 MHz Most operation between 5760.050 and 5760.150 MHz W, OE, VE, SM, OK, I, DJ, LX, JA, OH,RW, CT, ZS, F, G, VK Operation RW3BP operational on 5670 MHz W5LUA and OE stations worked RW3BP crossband 5760/5670 MHz using 5616 MHz LO and 54 MHz IF 25+ stations operational Station Requirements 3M Dish and 25 watts WWW..ORG 12

5.7 GHz Activity List WA5TNY, K2DH, W7CNK, K0KE, W5LUA, OE9PMJ, VE4MA, SM4DHN, OK1KIR, I6PNN, OE9ERC, DJ5FJ, LX1DB, NU7Z, JA7BMB, W5ZN, IK2RTI, OH2AXH, RW3BP, CT1DMK, VE1ALQ, ZS6AXT, WA5ICW, F2TU, F1ANH, WD5AGO, G4NNS, VK3NX Most use linear polarity but there is a strong migration towards CP mainly because of the spatial offset problem. CP has also been shown to reduce the spreading on 5.7 GHz signals WWW..ORG 13

10000 to 10500 MHz Most operation between 10368.050 and 10368.150 MHz W, GW, OE, VE, SM, OK, I, DJ, LX, JA, OH,CT, ZS, F, G, PA, VK, RW, S57, HB, SP, RW Operation JAs operational on 10450 MHz - another crossband challenge - JA7BMB has worked several stations 40+ stations operational Station Requirements 3m Dish, 25 watts WWW..ORG 14

10.3 GHz Activity List NA WA7CJO, WA5VJB, W5LUA, VE3ONT, VE7CLD, WA6EXV, K9KFR, AA5C, WA6PY, N4MW, NU7Z, VE4MA, W6HD, W7SZ, K6RE, W4AD ROW SM4DHN, G3WDG, OK1KIR, PA3CSG, F6KSX, DJ5FJ, CT1DMK, VK2ALU, RW3BP, DF0OVH, I4CHY, LX1DB, DL2LAC, IK5WJD, IW4BTG, S57UUU, HB9BHU, OK1UWA, DL0EF, OH2AXH, OK1CA, F2TU, PA0EHG, G4NNS, F3VS, F1BLL, I4TTZ, I5PPE, DJ5MN, DK7LJ, JA7BMB, GW3XYW, IQ4DF, DL0SHF, F5JWF, HB9SV, IK2RTI, SP7JSG, RW1AW, GW4DGU, DF9QX, F5JTA WWW..ORG 15

5 Meter Dish at W5LUA Used for EME on 902 MHz 1296 MHz 2304 MHz 3456 MHz 5760 MHz 10368 MHz May use on 222 and 432 MHz Also considered use as a 2.5M offset fed dish for 24 GHz WWW..ORG 16

AZ EL Mount for 5 Meter Dish Hydraulics for elevation drive Prop pitch rotor for azimuth drive US Digital Absolute Encoders for readout and K5GW tracking program WWW..ORG 17

Multi-Band Feed System 10368 2304 1296 5760 WWW..ORG 18

K0YW at KH7X on 23 & 13 cm WWW..ORG 19

10 ft Dish at WW2R WWW..ORG 20

At Midlothian EME Contest 2005 Sept Oct 2005 EM12lj WWW..ORG 21

WA5WCP Mobile 5,4,3,2,1 WWW..ORG 22

WA5WCP / 1 @ W1JJ RI WWW..ORG 23

WA5WCP/1 Four States on 1296 EME in 16 Days Aug 2006 WWW..ORG 24

24000 MHz Operation originally occurred at 24192.100 MHz migrating to 24048.1 MHz because of primary int l allocations W5LUA, VE4MA, RW3BP, AA6IW, VE7CLD became operational in 2001 and 2002 More recently OK1UWA, G4NNS, DF1OI and LX1DB have become operational Minimum station Requirements 3M prime focus or 2.4M offset fed dish and 20 watts WWW..ORG 25

3 Meter Dish at W5LUA WWW..ORG 26

Tracking the Moon at 24 GHz at W5LUA Antenna beam width less than 0.3 degree Moon noise meter such as GR-1216 and GR-1236 allows tenths of db to be measured Elevation - Multi-turn pot and direct drive gearing provides voltage to drive IBM A/D board and W9IP Realtrack software Azimuth Precision transducer in Andrews positioner provides voltage to drive IBM A/D board 8V=360 Degrees 0.1 degree readout and accuracy Update antenna position every 30 to 45 seconds WWW..ORG 27

47088 MHz Operation at 47088.100 MHz AD6FP, RW3BP, W5LUA, and VE4MA operational Station Requirements 1.8 or 2.4 M offset fed dish and W2IMU type feed and 30 watts minimum Required use of RW3BP software for averaging of cw transmissions to enhance S/N ratio WWW..ORG 28

47 GHz EME Software

2.4m Offset Fed Dish at W5LUA WWW..ORG 30

AZ-EL for W5LUA 2.4 Meter Dish WWW..ORG 31

Atmospheric & Weather Effects Normally rain does not have a major impact on EME conditions through 5760 MHz some effect on 10 GHz Humidity and heavy cloud cover cause increased absorption at 24 GHz best conditions occur on a cold crisp night in the middle of winter At 47 GHz oxygen absorption is major contributor there are no good times to operate! WWW..ORG 32

Doppler The doppler shift is a change in frequency of the signal reflected off the moon and received back on earth. Doppler scales with frequency and is an indication of the relative motion of the moon with respect to the earth. When the moon is rising the doppler will be positive and when the moon is setting the doppler will be negative. The doppler is at a maximum when the moon is on the horizon and at a minimum at zenith. While doppler may be several hundred Hz at 2M, it is over 3 khz at 1296 MHz and greater than 100 khz at 47 GHz WWW..ORG 33

Faraday Rotation According to Skolnik s Radar handbook.. The Faraday rotation of the plane of polarization can be 2 to 5 revolutions in the UHF range, but since it scales as 1/f 2, is negligible at and above L band L band is defined in Skolnik as 1000 MHz to 2000 MHz and UHF is defined as 300 to 1000 MHz If we scale from 144 to 432 MHz the effect is 1/9 If we scale from 432 to 1296 MHz it is another 1/9 We know that time between signal peaks on 6M can be about 5 minutes, and 15 to 20 minutes on 2M and up to hours or days on 432 MHz so. In terms of what we hear, does this scale the time in between max and min signal strength or the level in db between max and min or both? Most likely it is scaling the amount of rotation of a linear polarized signal and decreases significantly at 902 MHz and higher WWW..ORG 34

K5GW Tracking Software with Doppler Calculation & RX Tuning

F1EHN Tracking Software with Doppler Calculation & RX Tuning

EME Net Meets Saturday and Sunday Mornings at 9AM Central time on 14.345 MHz NET Control is K1RQG Also available via the internet courtesy of K0TAR Weekly NET notes also available from K1RQG by emailing Joe at k1rqg@aol.com Also informal activity during the week on 14.345 MHz starting at 9AM Central WWW..ORG 37

432 MHz and Above EME Newsletter Edited and distributed monthly by Al Katz, K2UYH since 1972 send reports to a.katz@ieee.org Available from Rein W6/PA0ZN via the internet at http://www.nitehawk.com/rasmit/em70cm.html Available from Warren Butler wbutler@comcast.net in.pdf format WWW..ORG 38

International EME Conference DF6NA and his group sponsored the 2006 Int l EME Conference in Wuerzburg, Germany in August. 140 amateurs from all over the world were in attendance The 2008 Int l EME Conference will be held in Florence, Italy WWW..ORG 39

Coordination of Activity Band by band activity weekends and many contests during the year best to stay tuned in to the newsletter, net notes, reflectors and the 20M net. Bands like 1296 and 10368 MHz have considerable activity each month. Improved random activity on 2304. Best to coordinate other bands with individual operators known to be active WWW..ORG 40

When is the Best MW EME Activity? Perigee when the moon is closest to the earth High declination best for northern hemisphere activity most hours of moon Perigee and High declination not always occurring at the same time of the month however as we approach 2007, the 2 conditions get pretty close Stay away from new moon Mainly weekend activity unless retired WWW..ORG 41

Moonbounce Reflectors Moon-Net - http://www.nlsa.com/nets/moon-nethelp.html EME-net - http://web.telia.com/~u37029479/ WWW..ORG 42

Websites for more Information VE1ALQ - http://www.ve1alq.com/ F1EHN - http://www.f1ehn.org/ W2DRZ - http://www.w2drz.ramcoinc.com/index.htm K2AH www.k2ah.com W1GHZ www.w1ghz.org WWW..ORG 43

Any Questions? 73 Al Ward W5LUA al.ward@avagotech.com WWW..ORG 44