C5-^-/5-/F. ■ /^^ -jrrs 10^' ESSA TR ERL 162-ITS 104 A UNITED STATES DEPARTMENT OF COMMERCE PUBLICATION ESSA Technical Report ERL 162-ITS 104 U.S. DEPARTMENT OF COMMERCE Environmental Science Services Administration Research Laboratories An Atlas of Oblique-Incidence High-Frequency Backscatter lonograms of the Midlatitude Ionosphere ROBERT D. HUNSUCKER BOULDER, COLO. MARCH 1970 ESSA RESEARCH LABORATORIES The mission of the Research Laboratories is to study the oceans, inland waters, the lower and upper atmosphere, the space environment, and the earth, in search of the under- standing needed to provide more useful services in improving man's prospects for survival as influenced by the physical environment. Laboratories contributing to these studies are: Earth Sciences Laboratories: Geomagnetism, seismology, geodesy, and related earth sciences; earthquake processes, internal structure and accvirate figure of the Earth, and distribution of the Earth's mass. Atlantic Oceanographic and Meteorological Laboratories and Pacific Oceanographic Laboratories: Oceanography, with empJiasis on ocean basins and borders, and oceanic processes; sea-air interactions: and land-sea interactions. (Miami, Florida) Atmospheric Physics and Chemistry Laboratory: Cloud physics and precipitation; chemical composition and nucleating substances in the lower atmosphere; and laboratory and field experiments toward developing feasible methods of weather modification. Air Resources Laboratories: Diffusion, transport, and dissipation of atmospheric con- taminants; development of methods for prediction and control of atmospheric pollu- tion. (SUver Spring, Maryland) Geophysiceil Fluid Dynamics Laboratory: Dynamics and physics of geophysical fluid systems; development of a theoretical basis, through mathematical modeUng and computer simulation, for the behavior and properties of the atmosphere and the oceans. (Princeton, New Jersey) National Severe Storms Laboratory: Tornadoes, squall Unes, thunderstorms, and other severe local convective phenomena toward achieving improved methods of forecasting, de- tecting, and providing advance warnings. (Norman, Oklahoma) Space Disturbamces Laboratory: Nature, behavior, and mechanisms of space disturb- ances; development and use of techniques for continuous monitoring and early detection and reporting of important disturbances. Aeronomy Laboratory: Theoretical, laboratory, rocket, and satellite studies of the phys- ical and chemical processes controlling the ionosphere and exosphere of the earth and other planets. Wave Propagation Laboratory: Development of new methods for remote sensing of the geophysical environment; special emphasis on propagation of sound waves, and electromag- netic waves at millimeter, infrared, and optical frequencies. Institute for Telecommunication Sciences: Central federtd agency for research and serv- ices in propagation of radio waves, radio properties of the earth and its atmosphere, nature of radio noise and interference, information transmission and antennas, and methods for the more effective use of the radio spectrum for telecommunications. Research Flight Facility: Outfits and operates aircraft specially instrumented for re- search; and meets needs of ESSA and other groups for environmental measurements for aircraft. (Miami, Florida) ENVIRONMENTAL SCIENCE SERVICES ADMINISTRATION BOULDER. COLORADO 80302 .> INSTITUTE FOR TELECOMMUNICATION SCIENCES J BOULDER, COLORADO ^ March 1970 For sale by the Superintendent of Documents, U. S. Government Printing Office, Washington, 0. C. 20402 Price $1.25 TABLE OF CONTENTS Page ABSTRACT 1 1. INTRODUCTION 1 2. RANGE -AZIMUTH AND RANGE-ELEVATION SCAN BACKSCATTER 5 3 2.1 Equipment Parameters 5 2. 2 Classification of Ech(;es 8 3. RANGE-AZIMUTH SCAN BACKSCATTER 29 4. RANGE-TIME BACKSCATTER 39 5. SWEEP-FREQUENCY BACKSCATTER 63 6. PPI ROTATING ANTENNA, FIXED FREQUENCY BACKSCATTER 87 7. ACKNOWLEDGMENTS 105 8. REFERENCES 105 APPENDIX 109 iii Digitized by the Internet Archive in 2012 with funding from LYRASIS IVIembers and Sloan Foundation http://archive.org/details/atlasofobliqueinOOhuns AN ATLAS OF OBLIOUE-INCIDENCE HIGH-FREQUENCY BACKSCATTER lONOGRAMS OF THE MIDLATITUDE IONOSPHERE Robert D, Hunsucker An atlas of data photographs of (jblique- incidence high-frequency (HF) backscatter ionograms of t±ie nnid- latitude ionosphere from the period 1952 - 1969 is pre- sented. Representative examples of data acquired by the range-azimuth scan, range- elevat icm scan, range- time, sweep- frequency and PPI backscatter techniques are displayed. No attempt is made to interpret the back- scatter "signatures", but publications which present analyses and interpretations of backscatter data are referenced . Key Words: Atlas, backscatter, data, high-frequency, ionograms, ionosphere, midlatitude, oblique -incidence, photographs. 1. INTRODUCTION The purpose of this report is to present representative examples of oblique incidence backscatter ionograms of the midlatitude ionosphere obtained by several different high-frequency (HF) backscatter sounding techniques. The atlas consists of five data photosections and an appendix. Each section contains a description of a particular technique, a listing of pertinent equipment parameters, a saniple data format and a collection of photographs of the particular cathode -ray-tube (CRT) data display. Other similar atlases have been published by Wright andKnecht (1957) and by Agy et al. (1959). The HF backscatter technique for oxploriiig tlie ionosphere was pioneered by Edwards and Jansky (1941), Benner (1949), Kono (1950), Hartsfield et al.(l950), Dieminger (1 951), Peterson (1^51), Abel and Edwards (1951), Villard and Peterson (1952), and Silber stein (1954). This technique continues to provide scientists with new and iniportant information on the physics of the ionosphere and the nature of the surface of the earth. Basically, the method utilizes an HF pulse trans- mitter and a suitable antenna to illuminate the ionosphere, and a sensi- tive receiver to detect the signal after it has been refracted in the ionosphere, backscattered from the earth and returned via the ionosphere to the receiving antenna. Direct backscatter from electron -density irregularities in the high-latitude ionosphere has also been described by Bates (I960, 1965), and applications of HF backscatter information for improving high -latitude HF predictions have been recently reported by Hunsucker and Bates (1969). No attempt will be made to interpret the backscatter data in this Atlas; instead, I hope that ionospheric physicists of the theoretical persuasion, while wandering through this menagerie, may be attracted to one or more of the exotic specimens and feel compelled to contrive a rigorous, elegant, qviantitative , and thoroughly satisfying explanation. For detailed analyses of various HF backscatter observations the reader is referred to publications by Croft (1965); Bates (1966); Croft (1967); Blair, Melanson^and Tveten (1969); Georges and Stephenson (1969); Hxinsucker (I969);and papers referenced in the backscatter bibliography by Hagn et al.(l961). The five-digit number on the lower left of each page of most of the ESSA. backscatter data is the number of the negative for that page, which is on file in the Photographic Laboratory at the ESSA Research Laboratories in Boulder, Colorado. Photographic prints of any figure or figures may be obtained at a nominal charge by writing directly to the Photographic Laboratory. Table 1 lists five of the most commonly used techniques for ob- taining HF backscatter information on the state of the ionosphere. It is intended to convey some idea of the general characteristics and capabilities of each of the listed techniques. -2- (U • tn o 0) &S2 u ^Q 5: X) r-H < ti a ^ (0 u •H •M OQ • H h 0) •M u (d h «J A U ^^ '^ 0) <^ O OjO CU (u • xi > y 3 £ 5^ P! O H < pq 'n" >-li! g^ •— < r; — S 3." • H O^ M ^t s H h Pi 4) O* •r! 1 Q> H ^ w a n) (U o CO a- :i: H H d: c:- TJ TJ •4-> i •1-1 o K^ tn ^K ^ :i fi bX) O •r-( d ■(-> nJ ^ 1 — 1 -Jd o GO m •iH H o O (0 o (U ^ M CU M fl CJ o (ti ■M ^^ T3 o (0 (U O ^4 o I O o o (1) U CiO Pi o CO (U o in r-< 13 O- *-> t— 1 o d — • CO • « ^ — c CO rt "^ ^4 in CO o ■J-J •rH f I d (4 • rH (7- (TJ o CU) ^ w r— ♦ CQ d) a. W d. >-< fl o o o Oh u -4-) :3 . .— 1 1— 1 u g) o CO (D C 0) > ^ a i-i o •iH ;3 a^ .3 r— 1 CO ^-1 c3 a s u o o c: a, Q) x: o c a. 82818 12 U O Q. 82819 13 82829 14 imirtw: ^^rr MIMItti. miiSfir M I ) i X tr I to » 82830 15 X "it to" CD CD > o C/) O O N X CO CO CD CO o CM to 82827 C o □Q 16 to O m CO 82821 17 82820 18 ■HiMiiit. mum MHIHttttti ttBifif -fc q: I ■ ■■■■■■ ■>: t iWf^i rau »■■»«««« J ti 'T 01 Q. (LI CO cr> — CO o LO O 13 Cn c >i«4<|'i.««'i-«>«« w>^s«^ftuk>^4i ,«lk* 1*ivM^l4fcW4' < • < I ; « ' i,\»^'tX4>^ tri i-»->J^ I IM I 82822 19 CD ^. t3 3 k. CO (U c 82823 20 T ^ a. I o (/) = 2 rO IT) O o o UJ I a> a> c o q: I w O 82824 il o o I ^^^^^^^^^^^^Be! X lO to to ?r C/) 82825 2Z o o I 82826 IS a> o sz o UJ ■D if) (/) O O c ID X a: I CD > o to CO O ro O 82831 24 X q: rsi X c -J 2i CO OJ in ro o X CO iT) — (/) CM o u •o (/> o u c Z5 X or fM X ih Q. Q) ro OJ t- co ro in X X to O — oo ro 82832 25 X a: I 00 Q. < = CO (/) 1^ o > o CD I- cn O in o 30 IHHHMi^lllliyL r^ in en ID I- o rO O CM CO CO CNI I If) — o CD CO fO I/) u O Q- CD 3 -3 CO o O O U3 CO If) CO «> >s «r — — 3 CO CO GO in O 83792 31 X CD D CD o CD X ID (D CD 3 00 CM CO to o CM 83795 (/> N X LO CD CD -3 r- (/) CM o CM Nl X in CD (J) >> o 0} h- co ro O 32 cri IT) -> o o I ■3 -3 CO o CD I in I ID 01 CM OO cri in CO '3- CD 83793 33 M I lO 1^ s — ^^ — ID K ^ iO a> o ^ «• > o z (M h- co 5 • 'T - »r> o OO U) -II- o ro r- N I CO ro ID 0} o > o q> 1- o — ir> r— O u V (A E OO a> o I c IT) ID > o 2 83794 35 ,__-,_(__■-_[ I^i N If) CD CO CvJ o -^ k o (A E o o X '--JU- a; £ 83791 36 X LO CO 00 O o OvJ u UJ •o (/> o u c 3 X IP CM CM 83796 37 4. RANGE -TIME BACKSCATTER The data in the first part of this section were provided by Professor I. Ranzi of Ccntro Radioelettrico Spcrimentale "G.Marconi", in Rome, who has also furnished the following information on the observing station: Latitude and longitude: 42.02° N; 1 1 . 84* E Peak pulse power: 2. 5 kW Pulse repetition frequency: 16. 66 pulses/ sec Pulse duration: 400 \i sec Type of antenna: Four-element horizontal Yagi; gain r 7 dB, beamwidth (-3dB)=56 , front -to- back gain ratios 33d B, height above the sea = 15 m (the antenna tower is on the coast, and all the first Fresnel zone of the reflected ray is on the sea for direction NNW.) On each of the records, time (15° east meridian time) increases from left to right, and slant range (in kiloinctcrs) increases from bottom to top. The operating frequency for all the data is 18, 6 MHz, and the antenna azimutli is indicated on tlie left end of each film strip. Photo- graphic negatives of each of the pages are on file at the ESSA Labora- tories photographic laboratory. The high resolution data photographs on pages 5 3-62 were obtained by the CRPL backscatter project group (R . Silberstein, W.L. Hartsfield and L. H. Tvctcn). These data were acquired during the period 1953-1954 with an oblique backscatter sounder located at Sterling, Virginia (Tveten, 1961). The salient system parameters are: Peak pulse power : 200 to 500 kW Pulse repetition frequency: 2 5 pulses/ sec Pulse duration: 40 \j sec Frequency: 13.7 MHz Antenna: Two 3-clcment vertically polarized Yagis spaced \/ 2 apart with the center oi the array -^^ - above ground. Now the Institute for Teleconununication Sciences, ESSA. 39 rJ 40 r 1 1 1 1 i 1 1 1 i 1 1 ~! 41 42 43 44 45 46 47 4 48 1 49 50 ii 51 52 CO 05 O o 'a- o rO I/) < CO (Dasoi) ^0|9Q auiii 53 o IT) I cs rsi S < ro LO 3 cn < ro ( 38SUU ) AD|9Q 9ai!_L 54 ^ rO in Q. 00 CD o o lO rO cr> x> E Q. ( Dasoi) AoiaQ aoiix 55 (oasLu) Ad|8(] 9uj!i 56 CSJ O o in Nl ro lO o u O cr> C3 ( 38SUJ ) A0|8Q 8UJIX 57 { D8SUJ ) Adisq aaijx 58 o ISI fO m o o O 1^ CO CVJ ( D8SUJ ) Ao|8Q aoiix 59 ( oasLu ) AoiaQ auiji 60 o o O < ID (J> o Li. C3 C3 (oasoi) Aoiag auj|^ 61 ( D9SUU ) ^D|9C 9UUI1 62 5. SWEEP-FREQUENCY BACKSCATTER These data were obtained at ESSA' s Erie, Colorado^field site during January through April 1963 using two different antennas. Pertin- ent equipment parameters are shown on page 65, along with the sample data fornnat. Pages 66-68 show soundings on the four cardinal geo- graphic azimuths using the rotatable log -periodic antenna. Various "signatures" obtained at different azimuths during winter and equinoctial months of 1963 are shown on pages 69 through 8 3. The multiple traces on the left of most of the data photos in this section are multiple vertical incidence (V-I) echoes. The oblique backscatter echo is observed to take off from the second-order vertical trace as explained by Peterson (1951). The distorted nature of the V-I traces in the region of 1 . - 6. 5 MHz is due to the nature of the frequency-determining cam used in this particular so\inder which resulted in transmission at a fixed fre- quency of 6. 5 MHz in this section of the ionogram. Pages 84-85 in this section display data obtained with the high-resolution system described in section 2. The "wide -beam" data were acquired using only one of the antennas of the 2 5-element horizontal array; the narrow-beam data were recorded using the entire array. These data arc included to illustrate how a narrow antenna beam shows the ionospheric "fine -structure" at midlatitudes. No attempt has been made to classify the echoes in this section as was done in section Z, since an excellent atlas of sweep-frequency backscatter data calibrated in amplitude has been compiled by Gilliland (1965). A listing of available sweep -frequency backscatter data obtained at the Eric, Colorado^site is included in the appendix of this atlas following the listing of range-a/.imuth and range- elevation scan back- scatter data. 63 The two records en page 86 of this section show examples of simultaneous oblique sweep -frequency backscatter, forward pulse propagation, and vertical incidence sounding data. The HF propagation path was from Sterling, Virginia to Boulder, Colorado (2370 km) and the experiment was described in detail by Silberstein (1958). Page 120 in the appendix lists the 35-mm film data on hand at Boulder from this experiment. 64 SWEEP-FREQUENCY DATA FORMAT 4000- c ^ 1000 85177 Frequency ( MHz) Location - Boulder, Colorodo Time - Mountain Standard Time (MST) Output Power a; 50 kw Pulse Repetition Frequency = 12.5 Pulses/Second Pulse Length = 250 /xsec j RHA b.) Rotatabie Log-Periodic — LPA Antennas: a.) Rtiombic Directed Toward 1 14 Geograptiic Azimutti 65 „.--.,- _ . -_ Z3 o in -:r" :■> --:- .. ;? ; M«^ :->! -_io IT) in CM lO o C a -3 00 ijkT »4m^ ~ — - — — I- « - « ■-— T '- . - g^ ^^y I (~ 1— wm^ .-4 CO < pMB9 ^^jfS'''^ i- UJ 4*°!^ *t^ aksss ■ -X^^- ■ ^SSRBSffMl y^^''% < Q. in ra^s-: 85175 66 ID CM col u M r% -1 ' 1 • "• ' ■ - • r ^^ - f «»i«« ;- CO < UJ t r fr^TST'^te^ ^'j;:: ■^ttt" *~ 1^ ro >» w O 3 C O -3 (0 < Q. 85174 b7 ■^ ' ' i in o C3 C5 o <=> o <=> C3 lO lO LO ur> i>o «VJ o o CD CD 0^ Q. < CVJ mm vmtm. mu imti§. H- o h ' ■■ m \ , ,:_\ - : : 4^ •t I r .«. ..-( i. 00 ID CM lO IT) < Q. 85173 68 o C o (T) CD rO O _1 L o O If) o C O 00 C\J C\J o < OL -I o C o CD CJ) O O 85176 69 ma inHU- to lo o (U m o 3 (D N- o o O in WIS?- -If *»'' ■* — f r 1 — &^ . . .^_ o O in < Q_ < Q. o m in 85163 70 - CVJ -h -1- 1 _-4. C3 _ "^ CD — LO (X) ro 00 ro o i_ JQ a> (D iT) >N o O '- iD o 3 X) t Li_ < O Q- OJ _J 85164 71 1 C5 1 1 1 O o o o LO LO lO lO ro CVJ 0} CD CD o o o JO Ll CM ro o O lO < CL _1 85165 72 1 o 1 C3 1 o 1 o o O o o> tn LO lO lO ro CVJ — o O in o 3 u. 00 O O o 'a- < Q. < CL 85166 O 3 CO 00 If) »_ o o o 3 lO jO ~- U- 00 CM (D o o O ro ro o O IT) < Q. o Zi ro O < CL o 00 CM ro O tS"^T^"^ 85167 74 en 00 O I 85171 ro CD o CO o o in < a. ._.« .■•. . > ro 1- o — < Q. o 3 O 00 CM t < CL CM _l o CM 75 1*5 IO«N1t O O < V- O in 00 CVJ o <=> a <=> ^ o <=> <=> lO lO to to ro CNJ — o O C\J u 00 o — < Q. _l IMS VekKk. < a. sz o lO CO ro 85168 76 o in ro o O < Q. m» ii4fl» lr^-^1 \ — — — r ift ^ L , IT It" i ^•' •*-'^ T» X 3V11 .=_ .-j= ^. H -•5 a i\ • ■»■■ i 1-1 ~ v-\ if • «■ ^ ■■? ^ ^?5S riilflBK .n ■ ■ ' 1 \A - .1 -^ ■sitia 9UIS : i : ■ • — : a^ 1 « > - . -. •-•1 ^^ r —i -— - I-. 19 m m O (D f^ (Ti OJ M o 2 < CD Q. -1 ro 85169 77 laiz dSw. 0} o CM 2 lO O - 1 'T >l ! 1 1 i i i i I 1 ; - 1 <:» ro 1 esj 1 1 o o to o < X q: f^^PPPf 4 -. ^. -... TT — i- .-i. — .4. — rT- 4 ■ o o CM CM I o NiB SiSpM mil2 IIBM* < x: o o O 1- h- o CM ^ , 1 00 CM < ^ a. ID _i o CM ro 85162 78 4 o O < CL CM CM o O o < Q. SI o o - t ro (\J lO < X q: ' ' • I o O CM » f ro < a. 85170 79 o Q. < IT) O O -t-H^r^M- t -i f- i - ^-^ ♦■-— t o CO CM CM < Ql JUS IM«M«. "1-: Q. < 00 o < Ql 85172 80 o O Q. < o O < Q- Q. < in o C\J Q. < in lO < CL 85159 81 "csj -4*^ — ^rjiirifja^ -^-; ; ;. O u. '^r a. < — ^ 11 00 < C\J Q_ in _l < CL _J Q. < ^ h- O L. N Q. (\J < CO . (0 ro <. h- LL 85160 82 i 1 o 1 o 1 «=> o o LO LO LO OJ Q. < CM CM o O 00 < 0. < Q. Q. < 00 O O Q. < CVJ ro 85161 83 NARROW-BEAM SWEEP- FREQUENCY BACKSCATTER BOULDER, COLORADO - MARCH 1969 9 10 12 14 16 18 20 22 24 Frequency (MHz) 26 28 85157 84 WIDE- beam/narrow -BEAM SWEEP-FREQUENCY BACKSCATTER BOULDER, COLORADO MARCH 1969 Narrow-Beam Wide Beam I I I I I I I { I I I I I I I { I I I 7 9 II 15 15 17 19 21 2i 25 Frequency (MHz) 25 85158 Wide Beam siiiill Narrow Beam Wide Beam Narrow Beam [ , g , I * !■'■ iiiSiiiiiill m MnHIII 85 Simultaneous Vertical - Incidence, Oblique - Incidence Backscatter and Forward Pulse Sounding Data 10 12 1344 CST March 18, 1955 24 MHz km 3000- 2000- 1000- ■ * 4 1 * " , 1 : i \ Liil ■1 IWPii Ml -.1- r iTirin 1^ 1 6 8 10 12 14 16 18 20 1240 CST November 22, 1954 22 24 MHz 86 6. PPI ROTATING ANTENNA, FIXED FREQUENCY BACKSCATTER This section contains representative examples of PPI''' back- scatter data obtained during winter 19 52-1953 at the Central Radio Propagation Laboratory (CRPL.) , Sterling, Virginia, field site. The PPI data format is shown ( 0402 EST 28 Dec. 1952 1531 EST 28 Dec. 1952 83564 97 0523 EST 1 Jan. 1953 1522 EST 1 Jan. 1953 83565 98 1741 EST 1 Jan. 1953 1854 EST 1 Jan. 1953 83566 99 1952 EST I Jan. 1953 0122 EST 2 Jan. 1953 83567 100 1^27 EST 5 Jan. I'Jbi 1 628 LSI .^ Jon I Obi 83568 101 1355 EST 22 Jan. 1953 1817 EST 22 Jan. 1953 83569 102 0307 EST 23 Jan. 1953 0941 EST 24 Jan. 1953 83570 103 7. ACKNOWLEDGMENTS I would like to express my appreciation to several of my colleagues at ITS for aiding and abetting me on this project. To Mr. L. A. Berry, Mr. L. H. Tvcten, Mr. R. K. Salaman, Dr. W. H. Hooke and Dr. T. M. Georges I ann indebted for many stimulating and challenging discussions concerning the makeup of this atlas. Professor 1. Ranzi of the Centro Radioelettrico Sperimcntale "G. Marconi" in Rome, Itlay provided good examples of range -time back- scatter data for section 4 of this alias. Special thanks are also due to Mr. L. H. Tveten ^or making available to me vast quantities of backscatter film data and providing essential information needed to identify and catalog these data. My thanks also go to Mr. R. G Kirby, (Director) and Dr. W. F. Utlaut (Deputy Director) of ITS for their support of this project. 8. REFERENCES Abel, W. G. , and L. C. Edwards (1951), The source of long-distance backscatter, Proc. Inst. Radio Engrs, i9_, 1538-1541. •^gy» Vaughn, Kenneth Da vies and Roger Salaman (1959), An Atlas of oblique -incidence ionograms, NBS Tech. N( te 31. Bates, H. F. (I960), The height of F -layer irregularities in the arctic ionosphere, J. Gcophys. Res. 64, 1257-1264. (Also see correction, J. Gcophys. Res. 65 , No. 4, 1304, b^oO.) Bates, H. F. (1965), Some effects of dense E clouds on high latitude HF backscatter observations, J. Geophys. Ros. 70 (23), 5895-5905. Bates, H. F. (1966), Results of the HF forward and backscatter program at College since 1963, Final Report, UAG-R-178, Geophysical Institvitc, University of Alaska, College, Alaska. 105 Benner, A. H. (1949), Predicting maximum usable frequency from long-distance scatter, Proc. IRE, 37, No. 1, 44-47. Blair, J. C. , L. L. Melanson and L. H. Tveten (1969), HF iono- spheric radar ground -scatter map showing land-sea boiondaries by a spectral -separation technique. Electronics Letters 5, No. 4, 75-76. Croft, T. A. (1965), The synthesis of sweep -frequency grovmd back- scatter by digital computer. Tech. Rept. No. 84, Radioscience Laboratory, Stanford University, Stanford, Calif. Croft, Thomas A. (1967), The interpretation of HF sweep -frequency backscatter soundings to deduce the structure of localized ionospheric anomalies, Tech. Rep. No. 116, Radioscience Laboratory, Stanford University, Stanford, Calif. Dieminger, W. (1951), The scattering of radio waves, Proc. Phys. Soc. (London) B, ^, 142-158. Edwards, C. F. , and K, G. Jansky (1941), Measurements of the delay and direction of arrival of echoes from nearby shortwave trans- mitters, Proc. Inst. Radio Engrs. 29, 322-329. Fitzgerrell, R. G. , L. L. Proctor and A. C. Wilson (1966), An HF antenna array electronically scanned in elevation, ESSA Tech. Rept. lER 11-ITSA 11. Georges, T. M. , and Judith J. Stephenson (1969), HF radar signatures of traveling ionospheric irregularities -3D ray -tracing simula- tion. Radio Sci. 4, No. 8. Gilliland, C. R. (1965), Sweep -frequency backscatter with calibrated amplitude. Tech. Rept. No. 11, Radio Science Laboratory, Stanford Univ. , Stanford, Calif. Hagn, George H. , Donald L. Nielson and Frances H. Smith (1961), Backscatter literature survey, SRI Report on Contract SD-66, Stanford Research Institute, Menlo Park, Calif. 106 Hartsfield, W. L.. , S. M. O s trow and R. Silberstein (1 950), Backscatter observations by the Central Radio Propagation Laboratory - August 1947 to March 1948, J. Res. NBS _44, 199-^14. Hunsucker, R. D. , and H. F. Bates (1969), Survey of polar and auroral region effects on HF propagation. Radio Sci. ^ , No. 4, 347-365. Hunsucker, Robert D. (1969), Remote sensing of the nnidlatitude ionosphere with a narrow-beam high-frequency radar, Ph.D. Dissertation, Univ. of Colorado. Hunsucker, R. D. , and L. H. Tveten (1967), Large travelling- ionospheric -disturbances observed at midlatitudes utilizing the high-resolution hf backscatter technique, J. Atmos. Terr. Phys. 29, 909-916. Kono, Tetsuo (1950), Experimental study on scattered echoes, Nos. 1 and 2, Report of Ionosphere Research in Japan, 4^, No. 3, 127-135 and 4, I^o. 4, 189-199. Peterson, A. M. (1951), The mechanism of F-layer propagated back- scatter echoes, J. Geophys. Res. 56, 221-237. Peterson, A. M. , R, D. Egan and D. S. Pratt (1959), The IGY three- frequency backscatter sounder, Proc. IRE, 4]7, 300-314, Ranzi, I., and P. Dominici (1963), Backscatter sounding during ionospheric storms, The Effect of Disturbances of Solar Origin on Coinmunications , Edited by G. J. Gassn-iann, AGARDograph 59, 143-154. Silberstein, R. (1954), Sweep-frequency backscatter -some obser\'ations and deductions, IRE Trans. Ant. Prcip. AP-2 , 56-63. Silberstein, R. (1958), The use of sweep-frequency backscatter data for determining oblique -incidence ionospheric characteristics, J. Geophys. Res. 63, No. 2, 335-351. 107 Thomas, J. A., and R. W. E. McNichol {i960), A highly directive rotating array for 16 Mc/ s, Nature, 187 , 398. Tveten, Lowell H. (1961), Ionospheric motions observed with high frequency backscatter sovmders. Radio Propagation, J. Res. NBS, 65D , No. 2, 115-127. Tveten, Lowell H. , and Robert D, Hunsucker (1969), Remote sensing of the terrestrial environment with an HF radio high -resolution azimuth and elevation scan system, Proc. IEEE 5_7 No. 4, 487-493. Villard, O. G. , Jr., and A. M. Peterson (1952), Scatter sounding: A technique for study of the ionosphere at a distance, IRE Trans. Ant. Prop, PGAP- 3 , 186-201. Wright, J. W., and R. W. Knecht (1957), Atlas of ionograms (unpublished report). 108 APPENDIX The tabulations on the left side of pages 1 10 through IZZ in this appendix arc listings of some backscatter sounding data which are available at the Boulder ESSA Research Laboratories. Sequences of the temporal behavior of two of the "signatures" observed with the narrow-beam azimuth and elevation scan radar are shown on the right side of pages 110 through 1 iZ , The data were acquired every two minutes and some idea of the irregularity motion may be obtained by rapidly flipping the pages. The upper photos show the time behavior of the "patch" signature^and tlic lower photos illustrate apparent motion of the "bands" signature. 109 Range -Azimuth and Range -Elevation Scan Backscatter - 16 mm Film Data Date Start End Type of "Signatures" Roll #64/ 65-01 MST 1964 Oct. 16 1050 1500 MSB, FS 19 0645 1800 MSB, FS, T, P 19 1830 2400 MSB, FS, P 20 0000 0600 MSB, P, : FS 21 0600 1815 MSB, FS, T 22 0715 1730 MSB, FS, P, LB, T 23 0800 1130 MSB, FS 23 1200 1600 MSB, FS, B Nov. 5 0830 1530 MSB, FS 9 0715 1845 MSB, FS, T, LB 11 0615 0700 MSB, T U 1700 1743 P 13 0620 0725 T, MSB, ; FS 13 1700 1800 MSB, FS 17 0612 0654 T, MSB 17 1600 1715 B 18 0615 0907 MSB, FS 19 1650 1740 P 21 1555 1700 LB, FS 23 1130 1600 LB, MSB Dec. 8 0930 Dec. 9 0347 MSB, FS, H 10 1508 1640 LB, MSB, FS 11 1316 1455 MSB, FS 14 1223 1334 MSB, FS 15 0715 2040 MSB, FS, B, H, P 15 2055 2400 P, LB 16 0000 -1600 MSB, FS, T 29 -1000 1635 MSB, FS, T 30 1000 1135 MSB, FS 31 1010 1100 MSB, FS, T 1965 Jan. 4 0920 1320 LB, MSB, FS 6 1005 1507 MSB 7 0805 1145 MSB, FS, T 7 1223 2200 MSB 82817 8 0023 1530 MSB, FS, T, P 0843 1300 110 Range -Azimuth and Range -Elevation Scan Backscattcr - 16 mm Film Data Date Start End Type of "Signature" Roll II 64/ 65-01 MST 1965 Jan. 11 1045 1110 MSB 13 1545 1615 MSB, FS 14 1216 - -1300 20 0920 162 5 MSB 23 0830 0920 MSB 25 0920 1000 Feb. 11 1735 1850 MSB, FS Roll No. 65-01 May 4 0900 1800 MSB, FS, T 5 1830(6 )0630 MSB 17 1100 18 50 P, MSB, FS, LB 7 2205 1445(1 9)P,MSB, FS, LB, T, U Roll No. 65-02 June 2 1030 2400 MSB, T, P, LB 3 0000 1515 MSB, P, T, FS 7 0925 1330 MSB, LB, P 8 1125 1445 MSB, LB 9 1000 2400 T, MSB, P 10 0000 1430 U, P, LB , MSB, FS, T 21 1100 1300 MSB, FS Roll No. 65-03 June 2 5 0905 1040 MSB, FS, P 28 1145 2400 LB, MSB, FS 29 0000 2400 LB, MSB, FS 30 0000 1100 LB, MSB Roll No. 65-04 July 1 1255 1450 LB, MSB, FS 2 0900 1045 MSB, FS 6 0950 2400 LB, MSB, T 7 0000 2400 LB, P, T , MSB, FS 8 0000 1315 MSB, T Roll No. 65-05 July 8 1410 1545 LB, MSB, FS 12 0925 1010 MSB, FS ..... 13 0020 0135 MSB. FS 0845 Li II 1302 82816 HI Range -Azimuth and Range -Elevation Scan Backscatter - 16 mm Film Data Date Start End Type of "Signature" Roll No. 65-05 MST July 14 0900 2400 MSB, FS, P, T 15 0000 2400 MSB, FS, P, T, H 16 0000 1335 MSB, FS, P Roll No. 65-06 July 19 0730 1030 MSB, FS 19 1820 1944 MSB, FS, P 20 0850 2400 MSB, FS, LB, P, T 21 0000 1520 MSB, LB, P, T 22 0000 1520 MSB, FS, T Roll No. 65-07 July 27 0905 2400 LB, MSB, FS, T, P, U 28 0000 2400 FS, MSB, P, T 29 0000 -1430 FS, MSB, LB, P 0847 1966 Roll No. 66-01 Jan. 24 1110 1620 LB, MSB, FS 25 1110 1650 MSB , FS, B 26 1210 1625 MSB , FS, P Roll No. 65-08a Aug. 3 1045 2400 MSB , FS, T 4 00 00 2400 MSB , FS, T, U, LB 5 0000 0400 MSB , FS Roll No. 65-08b Aug. 10 1115 2400 MSB , LB, P, FS, T 11 0000 2400 MSB , T, LB Roll No. 66-02 Aug. 17 2000 2400 LB, P 18 0000 2400 MSB T B, H 19 0000 2400 FS, MSB, T 20 0000 FS, MSB, T, P Roll No. 66-03 Sept. 12 1725 2400 FS, MSB, T 13 0000 2400 FS, MSB, T 14 0000 2400 FS, MSB, T R7Rm ■*• -* 0000 2400 FS, MSB, T, LB 1304 112 Range -Azimuth and Range -Elevation Scan Backscatter - 1 6 mm Film Data Date Start P:nd Type of "Signature" Roll No. 66-03 MST Sept. 16 0000 2400 FS, MSB, T, LB 17 0000 1730 Roll No. 66-04 Oct. 10 2015 2400 T, P, H, MSB, FS 11 0000 2400 LB, MSB, FS, B 12 0000 2400 U, LB, MSB, FS, B 13 0000 2400 LB, MSB, FS, B 14 0000 2400 U, MSB, FS, B 15 0000 1000 MSB, FS Roll No. 66-05 Nov. 15 1350 1900 U, MSB, H 15 2030 2400 P, LB, MSB 16 0000 1130 U, H, P, B 16 1930 2400 U, H 17 0000 2400 FS, B, U, P 18 0000 1300 LB, U, P, FS 19 0130 1740 U, P, FS, B Roll No. 66-06 Dec. 14 1637 2400 MSB, H, FS 15 0000 2400 B, P, MSB, FS 16 0000 2400 FS, H, MSB, FS, B, T, P 17 0000 1730 H, MSB, FS, B 1967 Roll No. 67-01 Jan. 18 1820 2400 MSB, FS, LB, B 19 0803 1910 H, FS 19 1918 2400 LB, MSB 20 0745 -1700 T, H, MSB, FS 20 1758 2400 T, H, MSB, FS 21 0025 0441 T, MSB, FS. H 21 0524 1701 T, MSB, FS, B Roll No. 67-02 UT Feb. 14 1430 2400 MSB, FS, T, B 15 2149 2400 MSB, FS, B 16 0038 2400 MSB, FS, T, B 82814 1'^ 0000 2400 MSB, FS, B 18 0000 2400 MSB, FS, B, 11 0849 1306 113 Range -Azimuth and Range -Elevation Scan Backscatter - 16 mm Film Data Date Start End Type of "Signature" Roll No. 67-03A UT Mar. 14 1538 2400 U, FS, B 0851 15 0000 2400 U, FS, B 16 0000 2400 U, FS, B 17 0000 2400 U, FS, B 18 0000 2400 U, FS, B, MSB Roll No. 67-03B Mar. 14 1420 2400 B 15 0000 2400 B 16 0000 2400 B, T 17 0000 2400 T, LB, B 18 0000 2400 B, LB Roll No. 67-04 Apr. 11 0515 2400 MSB, T, U, FS 12 0000 2400 U, FS, MSB, T 13 0000 2400 U, FS, MSB, T, B 14 0000 2400 U, FS, B 15 0000 2400 U, FS, T, P Roll No. 67-05A May 9 0115 2400 B, U, MSB, FS, P 10 0000 2400 U, FS, H, P, T, MSB 11 0000 2400 MSB, LB, T, P 12 0000 2400 MSB, LB, FS, H, T, P 13 0000 2400 LB, MSB, FS, P, T RoU No. 67-05B May 22 2030 2240 FS, T, MSB 23 1530 1830 U, FS, T 23 2030 2130 FS, T 24 1520 2300 MSB, FS, T, P 1308 25 1500 2100 B, FS, P, MSB, T Roll No. 67-06 Jime 13 0345 2400 LB, MSB, FS, P, B 14 0000 2400 U, FS, MSB, P, H 15 0000 2400 P, H, T, MSB, LB 16 0000 2400 U, MSB, P, FS 17 0000 2400 P, MSB, P, FS m „ «tm .-. ■f m^ 1 82813 114 Range -Azimuth and Range -Elevation Scan Backscattcr - 1 6 mm. Filnn Data Date Roll No. July 18 19 20 21 22 Roll No. Aug. 15 16 17 18 19 Roll No. Sept. 19 20 21 22 23 Roll No. Oct. 24 25 26 27 28 Roll No. Nov. 14 15 16 17 18 Roll No. Dec. 12 13 14 15 16 82812 Start End Type of "Signature" 67-07 0630 0000 0000 0000 0000 67-08 0020 0000 0000 0000 0000 67-09 0000 0000 0000 0000 0000 67-10 1500 0000 0000 0000 0000 67-11 0130 0000 0000 0000 0000 67-12 1030 0000 0000 0000 0000 0853 UT 2400 MSB, T, P, FS 2400 MSB, P, FS 2400 MSB, FS, P, H, T 2400 MSB, FS, P 1030 MSB, FS, LB 2400 MSB, FS, T, P, B 2400 P, T, MSB, FS, B 2400 MSB, FS, LB, T 2400 MSB, FS, T 2400 MSB, FS, P, H 2400 U, FS, MSB, B, P, T 2400 MSB, LB, FS, T 2400 U, FS, P, B, LB, H, T, MSB 2400 U, FS, P, MSB 2400 LB, FS, MSB, B, U 2400 U, MSB 2400 U, FS, MSB, P 2400 U, FS, MSB 2400 U, FS, B 2400 U, FS, MSB 2400 B 2400 U, FS 2400 U, FS, MSB 2400 U, FS, MSB 1310 2400 2400 U, FS, MSB, B 2400 B, U, MSB, B 2400 MSB, FS, B 2400 MSB, T, U, FS 2400 U, MSB, FS, B M 115 Range -Azimuth and Range -Elevation Scan Backscatter - 16 mm Film Data Date Start End Type of "Signature" FS, MSB, P, T, U, B MSB, FS, T, B MSB, FS, B MSB, LB, FS, B MSB, LB, FS, T MSB, FS MSB, FS, LB, B, T T, MSB, FS, B T, FS, MSB, P, B P, MSB, FS, B, LB MSB, FS, T, LB MSB, FS, B, T MSB, FS, T, LB MSB, FS, T, LB MSB, FS, T, U U, FS, T, MSB U, FS, MSB, P U, FS, T MSB, FS, U, P MSB, FS, LB, P T, FS, P LB, P, MSB, T P, FS, MSB P, LB, T, MSB, U, B U, MSB, FS, P, T MSB, FS, H, T, P MSB, FS, T, P, H MSB, FS, P MSB, P, T, B Roll No. 68-01 UT Jan. 1 6 0445 2400 17 0000 2400 18 0000 2400 19 0000 2400 20 0000 2400 Roll No. 68-02 Feb. 20 0100 2400 21 0000 2400 22 0000 1800 23 0007 2400 24 0000 2400 Roll No. 68-03 Mar. 12 0325 2400 13 0000 2400 14 0000 2400 15 0000 2400 16 0000 2400 Roll No. 68-04 Apr. 16 0700 2400 17 0000 2400 18 0000 2400 19 0000 2400 20 0000 2400 Roll No. 68-05 May 14 0535 15 0000 2400 16 0000 2400 17 0000 2400 18 0000 2400 RoU No. 68-06 J\m.e 12 0000 2400 13 0000 2400 14 0000 2400 15 0000 2400 MM ittMW 1312 ti. 82811 116 Year Sweep-Frequency Backscatter 16 mm. Film Data Month Days 1954 December lllh 1955 February 9 th 1963 January 2-10 1963 February 13-28 19 63 March 1- 5 1963 March 8-31 1963 April 1-30 1963 May 1-31 1963 June 4-21 0857 82810 1314 fc<^ V * 117 PPI - Rotating Antenna, Fixed -Frequency- Backs catter - 1 6 mm Film Data Date Start End 1952 Roll No. Dec. 4 7 1 0900 0537 Roll No. Dec. 7 10 2 0946 0822 Roll No. Dec. 10 13 3 0833 0152 Roll No. Dec. 13 15 4 0255 1913 Roll No. Dec. 15 18 5 1922 -1200 Roll No. Dec. 12 6 0744 Roll No. Dec. 21 23 7 0751 2318 Roll No. Dec. 23 26 8 2326 0640 Roll No. Dec. 26 29 9 1923 1308 Roll No. Dec. 29 Jan. 1, 1953 10 1313 0026 0901 '^"'»**^ ■Mi ^Wl 1316 1^ lb' I***- -"^ 82809 118 PPI - Rotating Antenna, Fixed-Frequency Backscatter - 16 mm Film Data Date Start End 1953 Roll No. Jan. 1 3 1 0035 17 54 Roll No. Jan. 3 6 2 1802 0625 Roll No. Jan. 6 9 3 632 0112 Roll No. Jan. 9 11 4 0941 2356 Roll No. Jan. 12 19 22 5 0009 1740 0414 0212 Roll No. Jan. 22 24 6 0222 1745 Roll No. Jan. 24 27 7 1753 1013 Roll No. Jan. 27 30 8 1020 0438 Roll No. Jan. 30 Feb. 2 9 0604 0055 0903 1318 Bf^ ki..» ^-^ 82808 11^ Simulta-neous oblique sweep -frequency backscatter, forward pulse propagation and vertical-incidence sounding - 35 mm fil m data Date 22- -23 Sept. ] L954 29 Sept. ] L954 15, 19 Oct. : L954 22- -23 Nov. : L954 29 Nov, 1 L954 7- -21 Dec. ] L954 18- -21 Dec. ] L954 3- - 4 Jan. 1 L955 11- -12 Jan. ] L955 17- -18 Jan. ] L955 24- -25 Jan. 1 L955 31 Jan. ] L955 1- - 2 Feb. 1 L955 7- - 8 Feb. ] L955 17- -18 Feb. ] L955 21 Feb. ] L955 24- -25 Feb. ] L955 1- - 2 Mar. 1 L955 8- - 9 Mar. 1 L955 15- -16 Mar. 1 L955 22- -23 Mar. 1 L955 29- -30 Mar. 1 L955 5- - 6 Apr. ] L955 12- -13 Apr. ] L955 19- -20 Apr. ] L955 26- -27 Apr. ] L955 29 Apr. ] L955 10- -11 May ] L955 0905 1320 82807 120 High -Re solution Range -Time Backscatter Large Negative Filna Data 1953 Day Month 2- 3 June 4- 5 August 11-13 13-14 '.' 20-21 25-26 26-27 31 Aug . 1 Sept. 9-10 September 10-11 15-16 16-17 17-18 22-25 29 Sept. - 2 Oct. 5-13 October 21-23 II 26-29 II 2- 3 November 12-13 " 17-18 II 17-18 Decennber Geographical Azimuth of Antenna Heading 150' 040* 150. 040 040 150 040 040 040 150 150 040 150 150 150 150 150 150 150 150 150 150 0907 1322 82806 Ul High -Re solution Range -Time Backscatter Large Negative Film Data 1954 Day Month 20-22 January 7- 9 February 19-25 March 1- 2 April 5- 7 8-13 14-15 19-20 23-30 30 April - 5 May 6- 9 May 10-19 II 21-25 It 1- 2 June 3- 4 II 7- 9 It 15-17 It 22-25 It 21-22 October Geographical Azimuth of Antenna Heading 150" 0909 1324 82805 122 091 Rll 1326 , it%n 82804 123 09!3 m-"^^ 1328 1 82803 124 82802 0915 V irr ■» 1330 . %t* 125 0917 HiiJ 1332 82801 126 82800 I r 0919 r-"^ 1334 , ^% 127 092! .., fclMl I 82799 1336 * V a^-*.*«i. «'^' ■^t^ 128 0923 l«* 1338 ^.. ^^^ 82798 129 0925 F*l ir: * -"m 1340 n€L /*-• 11'' i 82797 130 0927 P^'^ I I 1 mu 1342 82796 131 0929 t%*.. ,♦ •••• 1344 U*. ■u 82795 132 GPO 858-051 lipBr