IEEE TRANSACTIONS ON MICROWAVE THEORY AND TECHNIQUES, VOL. 49, NO. 6, JUNE 2001
1077
Ultra-Broad-Band Doubly Balanced Star Mixers
Using Planar Mouw’s Hybrid Junction
Chi-Yang Chang, Member, IEEE, Ching-Wen Tang, and Dow-Chih Niu
Abstract—Ultra-broad-band star mixers using planar Mouw’s
hybrid junction [1] are presented in this paper. The planar
Mouw’s hybrid junction is realized by coplanar waveguide (CPW)
to coplanar strip (CPS) or CPW to CPW T-junctions. A new
explanation of Mouw’s theory based on coupled transmission
lines and including the transmission line losses is presented. The
modified theory is more suitable for ultra-broad-band mixer
design. Some prototype mixers with CPW to CPS or CPW to
CPW T-junctions are fabricated with
2 3 substrate. The
prototype mixers show a bandwidth of greater than 20 : 1 if the
even-mode resonance has been damped out. Method for damping
out the even-mode resonance is also presented. All of the prototype
circuits show much broader bandwidth than that of conventional
star mixer.
Al O
Index Terms—Doubly balanced mixer, hybrid junction, star
mixer, ultra-broad-band mixer.
I. INTRODUCTION
U
LTRA-BROAD-BAND, typically greater than 10 : 1
bandwidth, microwave mixers are an important component in the applications such as instrumentation, electronic
warfare (EW), electronic support measures (ESMs), electronic
counter measures (ECMs), and electronic counter-counter
measures (ECCMs), etc. For example, a mixer for instrument
application is common to cover a frequency of 1–18 GHz or
even to 26.5 GHz. The most popular ultra-broad-band mixer is a
ring-type doubly balanced mixer. A ring-type doubly balanced
mixer uses two single baluns for RF and local oscillator (LO)
ports, and is usually realized by a soft-board and three-dimensional (3-D) structure. The star mixer is an alternative doubly
balanced configuration. There are many advantages of the star
mixer comparing to that of a ring mixer. One of them is that
the IF/RF or IF/LO diplexing circuit, which is essential in most
ring mixers, is eliminated. The IF signal can be directly picked
out from center of the star diode quad. However, the reported
star mixers do not show ultra-broad-band performance.
Two dual baluns are required to feed the balanced signals
to the diode quad in a star mixer. The conventional star
mixer [2]–[4] uses a modified Marchand-type dual balun [5].
A coaxial line, 3-D parallel-plate transmission line, coplanar
waveguide (CPW), or microstrip can realize the Marchand-type
Manuscript received August 4, 2000. This work was supported in part by the
Ministry of Education under Grant 89-E-FA06-2-4.
C.-Y. Chang and C.-W. Tang are with the Department of Communication Engineering, National Chiao Tung University, Hsinchu, Taiwan, R.O.C.
D.-C. Niu is with the Chung-Shan Institute of Science and Technology, LungTang, Taiwan, R.O.C.
Publisher Item Identifier S 0018-9480(01)03998-9.
dual balun. A pair of perpendicularly oriented Marchand-type
dual baluns [2]–[4] can realize a conventional star mixer.
The diode quad is placed at the center of two dual baluns.
The bandwidth of a conventional star mixer, typically 2 : 1
bandwidth, is mainly limited by this Marchand-type dual
balun. When performing the ultra-broad-band measurement,
the conventional star mixer periodically shows passband and
stopband. The stopbands of the conventional Marchand-type
star mixer are very wide and cannot be eliminated by the
method proposed in this paper because the stopbands of
the conventional star mixer are not caused by the resonant
phenomenon as the proposed Mouw’s star mixer does.
In this paper, we propose a star mixer using a planar Mouw’s
hybrid junction [1], which can achieve ultra-broad-band performance. The theory of original Mouw’s hybrid junction cannot
realize an ultra-broad-band mixer because the theory in Mouw’s
paper is based on lossless transmission lines. As the transmission line loss is introduced into the hybrid junction properly, this
newly proposed star mixer could be an ultra-broad-band mixer.
The hybrid junction proposed by Mouw [1] comprises a pair of
perpendicularly placed T-junctions. A single T-junction may be
considered as a dual balun. The bandwidth of a single T-junction dual balun is unlimited as long as the impedance is matched.
However, when the second T-junction dual balun is connected
to form a Mouw’s hybrid junction, the even-mode resonance,
as will be explained in the following section, occurs periodically. Theoretically, this resonant phenomenon causes conversion loss dips near the resonant frequencies. The Mouw’s star
mixer also shows multiple numbers of passbands and stopbands
due to this resonant phenomenon. According to the theory in
the following section, the stopbands can be quite narrow if the
even-mode characteristic impedance is much higher than the
odd-mode characteristic impedance. Therefore, the stopbands
(the resonant dips) can be removed by increasing the damping
factor of the resonance. An effective method to damp out the
resonance is proposed in this paper.
The suspended substrate coplanar strips (SSCPSs), the
conductor-backed coplanar strips (CBCPSs), and the absorber-backed coplanar strips (ABCPSs) are three proposed
transmission-line structures to realize a Mouw’s star mixer and
to compare their ultra-broad-band performance. The conversion loss dips can be found in the Mouw’s mixers realized by
SSCPSs or CBCPSs. The Mouw’s mixers realized by ABCPSs,
however, show very good ultra-broad-band performance because the absorber damps the resonant dips out. The theoretical
analysis for damping out the resonant dips is discussed in the
following section.
0018–9480/01$10.00 ©2001 IEEE
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IEEE TRANSACTIONS ON MICROWAVE THEORY AND TECHNIQUES, VOL. 49, NO. 6, JUNE 2001
(a)
(a)
(b)
Fig. 1. (a) Mouw’s hybrid junction with each transmission lines represented
by a pair of coupled lines. (b) Equivalent circuit of the Mouw’s hybrid junction
as it is excited from port 1.
II. THEORY OF MOUW’S HYBRID JUNCTION
TRANSMISSION-LINE LOSSES
WITH
The Mouw’s hybrid junction, as shown in Fig. 1(a), is
a broad-band magic-T-type hybrid [1]. In Fig. 1(a), nodes
11 represents port 1, nodes 22 represents port 2, nodes 33
represents port 3, and nodes 44 represents port 4. Ports 1 and
and ports 3 and 4 are terminated with
2 are terminated with
, respectively. This hybrid junction had been analyzed in
[1] based on lossless transmission-line theory. Mouw’s paper
suggested that the coaxial line, waveguide, double-sided strip
line, or lumped circuit transformer could realize the hybrid
junction. Here, we propose a planar circuit Mouw’s hybrid
junction, which is realized by two CPW to CPS T-junctions.
The CPS can be considered as a pair of coupled transmission
lines, as shown in Fig. 1(a). Assume that the coupled lines
and
are with the even-mode characteristic impedance of
the odd-mode characteristic impedance of
. The CPS
. If the coupled
characteristic impedance should be
lines are with loss, the equations presented in [1] should be
modified. Assume that the coupled lines are with even-mode
and odd-mode propagation constant
propagation constant
, respectively. When the circuit is excited from port 1, the
hybrid junction can be equivalent to a circuit shown in Fig. 1(b).
The terminating resistance of ports 3 and 4 are divided into
, respectively, for symmetry. The center points
two of
of the resistors should be RF virtually grounded. Therefore,
resistors can be connected,
the center point of the four
as shown in Fig. 1(b). Suppose that all the physical lengths of
(b)
Fig. 2. Calculated performances of Mouw’s hybrid junction with different
values. (a) Insertion loss. (b) Return loss.
the CPS transmission lines are equal to . Using the even- and
odd-mode excitation at ports 3 and port 4 and the property of
reciprocity, the scattering parameters of the hybrid junction can
be obtained. The 16 scattering matrix elements are given in
(1)–(4), shown at the bottom of the following page, where
is
, is or ,
represents the attenuation constant,
and represents the phase constant. The cases of
and
had been discussed in [1] with the condition of
. The analysis in [1] was focused on the first passband
only. As the ultra-broad-band performance is concerned,
the multiple numbers of passbands and stopbands should be
considered. The passbands’ center frequencies are defined as
, and the stopbands’ center frequencies
are defined as
, where
. The
impedance matching condition should hold at center frequency.
This implies that
(5)
can be chosen arbitrarily. However, it influences bandwidth of the stopbands. Our mixer is designed with
and
. Therefore,
should be 50 . Fig. 2
CHANG et al.: ULTRA-BROAD-BAND DOUBLY BALANCED STAR MIXERS
shows the calculated responses according to different
with
and
. The frequency in Fig. 2 is
normalized with the center frequency of the first passband. The
stopbands are located at the even multiples of the center frequency, as shown in Fig. 2. These transmission dips and reflection peaks could be explained as follows. From the equivalent circuit shown in Fig. 1(b), if the circuit is excited at port
1, the CPW-CPS T-junction at the upper left-hand side of the
figure forms a dual balun. The second CPW–CPS dual balun
in Fig. 1(b), at the bottom right-hand side of the figure, is just
loaded to ports 3 and port 4 as a ring circuit with ring char. The midpoint of the ring is RF
acteristic impedance of
virtually grounded and the port 2 connected to this point could
be removed without influencing the excitation. If the excitation
is from port 2, the situation is the same as the former case, except that the phase of outgoing waves between ports 3 and 4 are
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in-phase in this case and out of phase in the former case. The
circuit is just like a notch filter of order one when we look at
Fig. 1(b). The property of the filter in Fig. 1(b) is that the higher
, the narrower the stopband. As
and
are both high
enough, the stopband can be damped out, as shown in Fig. 2.
in Fig. 2 are 0.25, 0.5, 1.0, and 2.0 dB/in, reThe values of
spectively. When increases to 2 dB/in, the return losses of the
hybrid junction is better than 18 dB with insertion loss of 4.2 dB
(it should equal to 3 dB for an ideal hybrid junction) at the center
frequencies of the stopbands. This performance is good enough
for ultra-broad-band mixer application. According to the (1) and
(2), the return loss of ports 3 and 4 is equal to that of ports 1 and
. The return loss of ports 3
2 only for the case of
and 4 will not be equal to that of ports 1 and 2, especially at the
is not equal to
and
stopband center frequencies if
is not equal to zero.
(1)
(2)
(3)
(4)
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IEEE TRANSACTIONS ON MICROWAVE THEORY AND TECHNIQUES, VOL. 49, NO. 6, JUNE 2001
TABLE I
CPS PARAMETERS
(a)
III. MIXER DESIGN AND PERFORMANCES
(b)
Fig. 3. Cross-sectional view and E -field lines of the ABCPS. (a) Even mode.
(b) Odd mode (CPS mode) (substrate dielectric constant " = 9:8, substrate
thickness h = 25 mil, suspended height (absorber thickness) d = 200 mil).
An ABCPS, shown in Fig. 3, could realize a coupled line with
, very high
, very low , and very high . The
cross-sectional view and -field lines of an ABCPS is shown
in Fig. 3. In Fig. 3, almost no -field lines of the odd mode (or
CPS mode) go through the absorbing material if the substrate
is thick enough. However, most of the -field lines of the even
mode go through the absorbing material. The field penetrating
into the absorber causes much higher than . A general-purpose rubber-type absorber is used in the proposed mixer. Better
performances may be obtained if it uses an absorber that is designed for absorbing microwave energy especially near the resonant frequency.
Two methods are proposed in this paper to increase the
even-mode impedance. Using a very thin line and suspending
the substrate much higher than the substrate thickness is
the first method to achieve high even-mode impedance.
Three cross-sectional structures, namely, ABCPS, SSCPS, and
CBCPS, of the mixers are presented in this paper to compare
and gap widths
of
their performances. The linewidths
the CPS lines and the corresponding line parameters are listed
in Table I. The values listed in Table I correspond to CBCPS
and SSCPS with a suspended height that is the same as the
absorber thickness. An electromagnetic (EM) simulator (Microwave Office, Applied Wave Research Inc., El Segundo, CA)
is used to calculate the line parameters. The line parameters
of ABCPS are not calculated because the detailed material
parameters are not available. The spiral structure described in
[6] is the second method to increase the input impedance of the
even mode. The spiral has very little effect to the CPS mode,
but it acts as a lumped-circuit spiral inductor for the even
mode. The effect of this spiral CPS is equivalent to a straight
CPS line with very high even-mode characteristic impedance.
However, as with most of the lumped-circuit spiral inductors,
the spiral CPS has the problem of self-resonance. Both of
the ABCPS and spiral CPS methods for increasing the mixer
bandwidth are discussed and the results are explained in the
following section.
substrate and
Table I is based on a 25-mil-thick
200-mil suspended height.
Three different layouts with CPS width and spacing corresponding to nos. 1–3 in Table I are realized. The CPS length
in all three layouts equals 370 mil from the T-junction to
diode quad (including extra 30-mil length for connecting the
quad). A planar ultra-broad-band Mouw’s mixer is shown in
Fig. 4(a). It is the layout of the no. 3 mixer with CPS width
mil and spacing
mil. Fig. 4(b) is the photograph of the mixer [same as Fig. 4(a)]. The mixer diode used
in the mixers is DME3178 (the new part number is DME2178)
-band silstar quad from Alpha Inc., Woburn, MA. This is a
icon beam-leaded Schottky diode star quad with maximal
of 16 and typical
of 0.1 pF for each diode. The bottom
right-hand-side CPW-CPS T-junction dual balun has two CPS
jumps, as shown in Fig. 4(a). The left-hand-side CPS jump is required for crossing the upper left-hand-side CPW-CPS T-junction dual balun, as can be seen in Fig. 4(a). However, the righthand-side CPS jump in Fig. 4(a) is for balancing of the electrical
length of the right-hand-side CPS arm to the left-hand-side CPS
arm. Each jump can be realized by a pair of bonding wire, a
pair of gold ribbon, or a pair of air bridges [for monolithic microwave integrated circuits (MMICs)]. The coupling between
two CPS lines through the jump wires has been studied using
EM simulation. The coupling is negligible because the -fields
in two CPS lines are perpendicular to each other. The IF signal
is picked up from center of the star quad via a CPW line at
upper right-hand side of Fig. 4(a). The IF DC return is through
four CPS lines and grounded at the T-junctions. These dc return paths limit the IF bandwidth because the CPS lines, which
are in even-mode operation for the IF signal, become an open
. Therefore, the IF bandcircuit at the diode end when
width of this star mixer cannot overlap the RF bandwidth. The
IF signal of the lower left-hand-side mixer diode in the diode
quad is grounded through one more CPS loop than the other
three diodes. Theoretically, a bonding wire connects the lower
left-hand-side diode and the peripheral ground plane can balance the IF grounding path. This bonding wire works as an RF
choke and as an IF dc return path simultaneously. However, the
measured IF performance changes very little when the mixer is
with this bonding wire. The length of the CPS can be decreased
to get higher IF frequency. Consequently, the RF bandwidth
shrinks at the low-frequency end due to smaller CPS length. A
mil
mixer with shorter CPS length of 190 mil and with
mil is designed for comparing the RF and IF bandand
width.
in Fig. 1(a) is chosen to be 100 because it shows
The
the best return loss of the hybrid junction near the resonant
CHANG et al.: ULTRA-BROAD-BAND DOUBLY BALANCED STAR MIXERS
1081
(a)
(a)
(b)
Fig. 5. Measured performances of the mixer with CPS length of 370 mil and
CPS parameters corresponding to no. 1 in Table I. (a) Conversion loss versus
RF frequency. (b) Conversion loss versus IF frequency.
(b)
Fig. 4. (a) Layout and (b) photograph of mixer with 370-mil CPS length and
with W = 2 mil and S = 1:8 mil.
frequencies under a high
situation. As each diode in the
diode quad has the equivalent RF resistance of 50 , the hy. Usubrid junction will meet the condition of
ally, the equivalent RF resistance of a Schottky diode is approximately inversely proportion to the LO power level. Therefore,
can be met
the impedance matching condition of
if the diodes are properly pumped.
Figs. 5–7 show the measured performances of the mixer with
CPS length of 370 mil and CPS parameters corresponding to
nos. 1–3 in Table I, respectively. A mixer with shorter CPS
length of 190 mil and CPS width of 5 mil and spacing of 4 mil
is measured for comparing of the IF/RF performances. Figs. 5
and 8 depict two mixers, which are to be compared (the only
difference being their CPS length). The measured results are described as follows. The IF 10-dB conversion-loss bandwidth is
dc to 0.75 GHz for the mixer with 370-mil CPS length and dc to
1.8 GHz for the mixer with 190-mil CPS length. The RF 10-dB
conversion-loss bandwidth starts from 1.3 GHz for the mixer
with 370-mil CPS length and stars from 2.5 GHz for the mixer
Fig. 6. Measured conversion loss of the mixer with CPS length of 370 mil and
CPS parameters corresponding to no. 2 in Table I.
with 190-mil CPS length. The first resonance occurs at about
6.7 GHz for the mixer with 370-mil CPS length and 13.7 GHz
for the mixer with 190-mil CPS length. The first resonance is occurred at the frequency of even-mode CPS length equals to half
. Higher order resonance can only be found in
wavelength
the CBCPS mixer due to much lower even-mode characteristic
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IEEE TRANSACTIONS ON MICROWAVE THEORY AND TECHNIQUES, VOL. 49, NO. 6, JUNE 2001
(a)
(b)
(c)
(d)
(e)
Fig. 7. Measured performances of the mixer with CPS length of 370 mil and CPS parameters corresponding to no. 3 in Table I. (a) Conversion loss of SSCPS and
CBCPS mixer under various IF frequencies. (b) Conversion loss of ABCPS mixer under various IF frequencies. (c) LO to IF isolation of the SSCPS and ABCPS
mixer. (d) LO to RF isolation of the SSCPS and ABCPS mixer. (e) SSB noise figure of the SSCPS and ABCPS mixer.
impedance comparing to that of the SSCPS mixer. The conversion loss peaks of the ABCPS mixers improve to about 10 dB
near the resonance frequency, as was expected. The conversion
loss of the mixer with no. 3 CPS parameters in Table I are measured under various IF frequencies, as shown in Fig. 7(a) and
(b). The conversion loss degrades gradually as the IF frequency
increases. The first resonant frequencies of all three types of the
mixers, namely, ABCPS, SSCPS, and CBCPS, are very close. It
can also be seen from the figures that the CBCPS mixer has the
widest stopband bandwidth due to its much lower even-mode
impedance. The RF bandwidths of mixers with CPS length of
370 mil are described as follows. The RF bandwidth is from 0.9
to 19.5 GHz with conversion loss less than 11.5 dB for the no.
1 ABCPS mixer, and it is from 0.9 to 29.9 GHz with conversion loss less than 10.5 dB for the no. 2 ABCPS mixer. The RF
bandwidth of the no. 3 ABCPS mixer is from 0.9 to 31.5 GHz
with conversion loss less than 10.8 dB. The RF bandwidth of the
mil
ABCPS mixer with 190-mil CPS length and with
CHANG et al.: ULTRA-BROAD-BAND DOUBLY BALANCED STAR MIXERS
1083
(a)
(a)
(b)
Fig. 8. Measured performances of the mixer with same CPS parameters
in Fig. 5, but shorter CPS length of 190 mil. (a) Conversion loss versus RF
frequency. (b) Conversion loss versus IF frequency.
and
mil is from 2.5 to 33.5 GHz with conversion loss less
than 11 dB. The conversion loss, which degrades gradually from
low to high frequency, is mainly due to the performance degradation of the mixer diodes. A GaAs diode quad with a higher
diode cutoff frequency may be required to reach higher frequencies. The diode quad used in this paper, however, is a commercially available star quad with the highest cutoff frequency. The
measured LO to IF and LO to RF isolation of the no. 3 SSCPS
mixer and ABCPS mixer are shown in Fig. 7(c) and (d). The
isolation is also degraded at the stopband frequencies. However,
the isolation of the ABCPS mixer is better than that of SSCPS
mixer at the stopband frequencies. The penalties of using an absorber to damp out the resonance are the degradation of the conversion loss and noise figure over the entire bandwidth, except
the stopband. The degradation of the conversion loss is typically
from 0.5 to 1 dB, as can be seen in the conversion-loss curves.
The measured singel-sideband (SSB) noise figure of the no. 3
SSCPS and ABCPS mixer is shown in Fig. 7(e). The noise figure
improves a lot near the resonance frequency, but degrades typically about 1 dB at other frequencies. The CBCPS mixers show
strong resonance phenomenon due to relatively low even-mode
impedance. The higher order resonant peaks of CBCPS mixers
are not damped out, as can be seen in the conversion loss curves.
(b)
Fig. 9. Layout and measured conversion loss of the spiral CPS star mixer with
CPS parameters the same as in Fig. 6. (a) Mixer layout. (b) Measured conversion
loss.
Moreover, the absorber underneath the substrate of the CBCPS
mixer is useless to damp these resonant peaks out due to the
ground plane between the substrate and absorber. Therefore,
CBCPS mixers can only be used in their passbands, especially
the first passband.
As mentioned in the previous section, a spiral CPS may increases the even-mode input impedance at the diode end. A
mixer with spiral CPS layout and with CPS parameters of
mil and
, as shown in Fig. 9(a), is realized to study
the effect of spiral design. The measured conversion loss of this
spiral CBCPS mixer is shown in Fig. 9(b). However, the mixer is
not an ultra-broad-band mixer, as can be seen in Fig. 9(b). This
is due to the self-resonance of the CPS spiral inductor. Nevertheless, in the case of a CBCPS mixer, this spiral layout should
be much more broad band than the straight layout, as predicted
in [6]. A 3-dB conversion-loss passband is defined to compare
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Fig. 10.
IEEE TRANSACTIONS ON MICROWAVE THEORY AND TECHNIQUES, VOL. 49, NO. 6, JUNE 2001
Measured conversion loss of a conventional FCPW star mixer.
the bandwidth between mixers in this paper. The 3-dB conversion-loss passband is defined as a frequency band between
two corner frequencies, in which the conversion losses at these
two corner frequencies are 3 dB worse than that of center frequency. The 3-dB conversion loss passband of the spiral CBCPS
mixer is from 1.25 to 4.95 GHz in the first passband, which
corresponds to a relative bandwidth of 119%. The 3-dB conversion-loss passband of the straight CBCPS mixer is from 2.3
to 5.8 GHz, as shown in Fig. 6(a). The relative bandwidth of
the straight CBCPS mixer is 86%. Indeed, the spiral design increases the first passband a lot. The spiral CBCPS is a good
choice for the MMIC mixer design because the SSCPS and
ABCPS are both not usable in MMICs.
IV. DISCUSSIONS
According to original Mouw’s theory, many different kinds
of transmission lines can realize the Mouw’s hybrid junction.
A finite-ground-width coplanar waveguide (FCPW) is also a
good choice to realize the planar circuit Mouw’s hybrid junction. The hybrid junction theory developed in Section II is still
in (1)-(3) should equal
valid in the FCPW case, except
. An FCPW–FCPW T-junction type mixer has been fabricated, and the measured performance (not shown in this paper)
is not as good as a CPW–CPS T-junction type mixer. The relative 3-dB bandwidth of the suspended substrate FCPW (SSFCPW) mixer is 93.4%, which is less than that of the SSCPS
mixer (it is 124% in Fig. 6). Besides, the absorber-backed finiteground-width coplanar waveguide (ABFCPW) mixer shows serious performance degradation in the passbands. The reasons are
that the even-mode (suspended-stripline-like mode) characteristic impedance of a 100- FCPW line cannot be made high and
the odd-mode (CPW mode) electric field of the 100- FCPW
goes partially through the absorber because the total width of
the 100- FCPW is very large. Another issue for the star mixer
is the difference of RF performance between the conventional
star mixer described in [2]–[4] and the mixer proposed in this
paper. Authors have realized an FCPW conventional-type Marchand dual-balun star mixer [3] to see the behavior of passbands
and stopbands. The measured conversion loss of these conventional SSFCPW and ABFCPW star mixers is shown in Fig. 10.
The conversion-loss behavior of this conventional star mixer is
summarized as follows. The first 3-dB passband of this conventional star mixer is from 2 to 3.8 GHz, which corresponds to a
relative bandwidth of 62%. The first stopband with conversion
loss worse than 15 dB is from 5 to 8 GHz. The stopband and
passband performances of the ABCPW mixer are almost the
same as that of the SSCPW mixer, as can be seen in Fig. 10.
The passbands and stopbands of the conventional star mixer
appear periodically. Unlike this newly proposed Mouw’s star
mixer, the absorbing material cannot damp out the stopbands
of the conventional star mixer. This means that the conventional star mixer cannot be used as an ultra-broad-band mixer.
The Mouw’s hybrid junction is very useful in realization of an
ultra-broad-band star mixer. Moreover, it can also be used to realize a triply balanced mixer if a double-ring diode quad and an
extra IF balun are used. In fact, a triply balanced mixer that is
realized by Mouw’s hybrid junction faces the same even-mode
resonance problem. The methods to solve an even-mode resonance problem, which is developed in this paper, are also valid
in triply balanced mixer.
V. CONCLUSIONS
The ultra-broad-band star mixer using CPW-CPS planar
Mouw’s hybrid junction has been developed. The theory of the
elimination of the even-mode resonance has been developed.
Theoretically, a coupled transmission line with a lossy even
mode can damp out the resonance. The absorber-backed CPS
can damp out the resonance effectively. The penalties of using
an absorber to damp out the resonance are typically from 0.5to 1-dB degradation of the conversion loss and noise figure.
Higher even-mode impedance causes broader first passband
bandwidth. In case of a CBCPS, the even-mode resonance
cannot be damped out. The CBCPS mixer with a spiral CPS
layout has also been developed for increasing the first passband
bandwidth. The first passband bandwidth of this spiral CPS
mixer, approximately 4 : 1 bandwidth, was much broader than
that of a straight CPS mixer.
ACKNOWLEDGMENT
The authors wish to thank C. S. Wu, Chung-Shan Institute
of Science and Technology, Lung-Tang, Taiwan, R.O.C., for his
constant support and valuable suggestions.
REFERENCES
[1] R. B. Mouw, “A broad-band hybrid junction and application to the star
modulator,” IEEE Trans. Microwave Theory Tech., vol. MTT-16, pp.
154–161, Nov. 1968.
[2] B. R. Hallford, “A designer’s guide to planar mixer baluns,” Microwaves, pp. 52–57, Dec. 1979.
[3] S. A. Maas, “A broad-band, planar, doubly balanced monolithic
-band diode mixer,” IEEE Trans. Microwave Theory Tech., vol. 41,
pp. 2330–2335, Dec. 1993.
[4] Y. I. Ryu, K. W. Kobayashi, and A. K. Oki, “A monolithic broad-band
doubly balanced EHF HBT star mixer with novel microstrip baluns,” in
IEEE Microwave Millimeter-Wave Monolithic Circuit Symp. Dig., 1995,
pp. 155–158.
Ka
CHANG et al.: ULTRA-BROAD-BAND DOUBLY BALANCED STAR MIXERS
[5] N. Marchand, “Transmission line conversion transformers,” Electronics,
vol. 17, no. 12, pp. 142–145, Dec. 1942.
[6] S. Maas, M. Kintis, F. Fong, and M. Tan, “A broadband planar monolithic ring mixer,” in Microwave Millimeter Wave Monolithic Circuit
Symp. Dig., 1996, pp. 51–54.
Chi-Yang Chang (S’88–M’95) was born in Taipei,
Taiwan, R.O.C., on December 20, 1954. He received
the B.S. degree in physics and the M.S. degree in
electrical engineering from the National Taiwan University, Taiwan, R.O.C., in 1977 and 1982, respectively, and the Ph.D. degree in electrical engineering
from The University of Texas at Austin, in 1990..
From 1979 to 1980, he was a Teaching Assistant with the Department of Physics, National
Taiwan University. From 1982 to 1988, he was
an Assistant Researcher with the Chung-Shan
Institute of Science and Technology (CSIST), where he was in charge of
development of microwave integrated circuits (MICs), microwave subsystems,
and millimeter-wave waveguide E -plane circuits. He returned to CSIST, where
from 1990 to 1995, he was an Associate Researcher in charge of development
of uniplanar circuits, ultra-broad-band circuits, and millimeter-wave planar
circuits. In 1995, he joined the faculty of the Department of Communication
Engineering, National Chiao-Tung University, Hsinchu, Taiwan, R.O.C., where
he is currently an Associate Professor. His research interests include microwave
and millimeter-wave passive and active circuit design, planar miniaturized
filter design, and MMIC design.
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Ching-Wen Tang was born in Nantou, Taiwan,
R.O.C., on July 16, 1968. He received the B.S.
degree in electronic engineering from the Chung
Yuan Christian University, Chungli, Taiwan, R.O.C.,
in 1991, the M.S. degree in communication engineering from the National Chiao-Tung University,
Hsinchu, Taiwan, R.O.C., in 1996, and is currently
working toward the Ph.D. degree at the National
Chiao-Tung University.
In 1997, he joined the RF Communication Systems
Technology Department, Computer and Communication Laboratories, Industrial Technology Research Institute (ITRI), Hsinchu,
Taiwan, R.O.C., as a RF Engineer, where he currently develops RF passive components. His research interests include microwave and millimeter-wave mixer
design, and the analysis and design of thin-film passive components.
Dow-Chih Niu was born in Taipei, Taiwan, R.O.C.,
on August 28, 1956. He received the B.S. degree in
electrophysics and the M.S. degree in electronics engineering from the National Chiao-Tung University,
Hsinchu, Taiwan, R.O.C., in 1978 and 1982, respectively.
From 1982 to 1991, he was with the Chung-Shan
Institute of Science and Technology (CSIST), LungTang, Taiwan. From 1991 to 1993, he was with the
University of California at Los Angeles. He is currently with CSIST, where he is in charge of the development of microwave and millimeter-wave circuits and subsystems.