PDF Designing High Power Arrays Using Maxi, Mini and Micro Family Dc-DC Converters

APPLICATION NOTE
Designing High-Power Arrays Using Maxi, Mini
and Micro Family DC-DC Converters
Introduction ................................................................1
PR Bus Architecture
PR Bus Architecture ....................................................1
Master / Slave Configurations................................1
Distribution Across Multiple Boards......................1
Master / Slave Configurations
One of the first decisions that must be made when
designing large arrays is to define the number of master
modules. Large numbers of possible masters will increase
redundancy but complicate PR and +S / –S line busing.
Initially it may be tempting to configure all modules in a
democratic array, but this may become cumbersome for
arrays of greater than three modules. For large arrays a
better choice is to define up to three modules as masters
and add additional slaves for more power. This provides
adequate redundancy for most applications.
Buffering .....................................................................2
Bypassing.....................................................................2
5 kW, 1,000 Amp Example Array ...............................2
Initial System Testing ..................................................6
PR Signal Fidelity ....................................................6
Input Ripple ............................................................7
EMI ..........................................................................8
Summary......................................................................8
Introduction
Vicor’s Maxi, Mini and Micro DC-DC converters are designed
for easy paralleling to increase output power. The unique
paralleling interface allows multi-kW capable designs to be
implemented with few external components. For information
on paralleling up to 12 modules, see the Application Note
“Converter PR Pin Facilitates Parallel Operation for Power
Expansion or Redundancy”. For very high-power arrays of
more than 12 modules, buffering of the PR signal is
required as the fan-out limit of the communication bus is
reached. This note describes how to use buffering to
increase the capability of the bus to drive large numbers
of converters, and gives an example of how to quickly
prototype a multi-kW system. This allows the benefits of
the Maxi, Mini and Micro family to be applied for systems
with output power into the multi-kW range.
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Distribution Across Multiple Boards
It is often necessary to break an array of converters into
multiple PC boards due to space and thermal requirements.
Separation between boards will introduce additional
impedance between the converters because of added
lead / trace length. To keep interconnect impedance
between boards from corrupting the control signals,
Vicor’s PR isolation transformer (Vicor P/N 29768) must be
used to isolate the PR bus. It is recommended that all
masters be located on the same board. This keeps noise
and line delay between the masters to a minimum. This is
especially important for very large arrays that will be
subject to high di / dts and dv / dts. If an application
requires redundancy between boards or between more
than 12 modules, a bidirectional buffer must be
implemented. This is beyond the scope of this note.
The PR signal should be bussed between boards with a
relatively lossy low-inductance connection. Twisted pair
works well while coaxial cable is not appropriate. Reflections
caused by the mismatch of PR bus source, load, and cable
impedance will not be damped by the low-loss coaxial
cable and result in reduced quality of the PR pulse.
Applications Engineering: 800 927.9474
Page 1
Buffering
High-speed buffering may be required with large arrays or
if the distance between modules is greater than a few
inches. This is because all modules, except the one that’s
talking, are in the listening mode. Each listener presents a
load to the master (talker) of approximately 500 Ω shunted
by 30 pF; see Figure 1. Long leads for the interconnection
introduce losses and parasitic reactance on the bus that can
attenuate and distort the sync-pulse signal. The bandwidth
of the bus must be at least 60 MHz.
Maxi, Mini or Micro DC-DC Converter
+IN
supply gives sufficient headroom for the followers. It is a
low-power rail that can be derived from a higher voltage
using a linear regulator. A separate auxiliary supply must be
derived on each board so that PR bus isolation is
maintained. The high frequency bypassing directly at each
buffer is essential.
Because of the high speed of the PR signal careful attention
must be paid to the signal fidelity of the PR bus. Locations
for both series and shunt damping resistors or ferrite beads
should be included in the layout as shown in Figures 2 and 3.
Populating all of these components may not be necessary
for all arrays depending on the geometry of the PR bus.
Both master and slave modules should have reverse-polarity
protection diodes (D1) on the PR pins.
6 V (Limited to < 150 mA)
Q1
PC
PR Logic
PR
Pulse Detector
Cint
Rint
30 pF (typ.)
500 Ω (typ.)
–IN
Figure 1 — PR pin equivalent circuit
One simple and robust PR buffer scheme is shown in
Figures 2 and 3. The system is separated into one master
board (Figure 2) and a number of slave boards (Figure 3).
The master board consists of five modules. Two of these are
configured in a democratic array with one trimmed down
by 2% relative to the other. These modules drive two
buffers. The first buffer (Q2) drives three additional slave
modules on the master board. The second drives the slave
boards. Each slave board contains five modules that are
configured as slaves by tying their SC pins to –S. There is a
PR isolation transformer on each slave board that isolates
the incoming PR signal. This signal is then buffered and fed
to each slave module.
The buffers are basic emitter followers that use generalpurpose NPN transistors. Transformers labeled T1 have 1:1
turns ratios and can be implemented by using Vicor’s PR
isolation transformer with one coil left open circuited.
Transformers labeled T2 have turns ratios of 2:1 to give
better matching to the PR distribution bus. The return path
for each transformer or buffer must be Kelvin connected to
the –IN pin of the appropriate converter. An 8 V auxiliary
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Bypassing
Selection of bypassing components has important
consequences for stability and EMI performance of highpower arrays. Common-mode bypassing for each converter
should be implemented as shown in the Design Guide and
Application Manual for the Maxi, Mini and Micro family.
Differential-mode bypassing can be considered in two
parts. Low-frequency bypassing that keeps source
impedance low and stabilizes the converter’s voltage loop
and high-frequency bypassing that reduces switching
related EMI. Low-frequency bypassing should be done
according to the Design Guide. Array input impedance is
the individual converter negative input impedance divided
by the number of converters in the array. This can present a
challenge for very large low-input-voltage arrays where
impedances must be kept very low.
5 kW, 1,000 Amp Example Array
The following prototype was implemented with modules
placed on evaluation boards and connected as shown in
Figures 2 and 3. It uses 25 modules with part number
V300B5C200B operating in parallel. The array has a 300 V
input, 5 V 1000 A output, and is connected in a 5 x 5 array.
Output leads must be very heavy gauge so as to have
sufficient ampacity to safely carry the high output currents.
To reduce the chance of noise causing the masters to swap
control, R5 is configured for 2% trim down. When using
Micro family converters in parallel arrays it is imperative that
the output voltage of each master is trimmed a minimum
of 2% apart.
Applications Engineering: 800 927.9474
Page 2
+8 V aux._M
C1
200 nF
2N2222
Q1
3
5
NP
1
R2
T2
8 V RTN_M
–PR Bus
Ferrite Bead
33 Ω @ 100 MHz
R1 75 Ω
2
+ Board Output
F1
+ Board Input
4
6
+PR Bus
Bypassing Not Shown (See Figure 4)
1:2
8 V RTN
Z1
R4
430 Ω
R4
+OUT
+IN
D2
PC
1N4148
430 Ω
PR
Master 1
(V300B5C200B)
–IN
+S
SC
–S
–OUT
– Board Input
– Board Output
+8 V aux._M
F1
C1
200 nF
2N2222
Q2
8 V RTN_M
R1 75 Ω
NP
Ferrite Bead
33 Ω @ 100 MHz
Z1
R4
430 Ω
R2
D1
D2
PC
1N4148
PR
R4
+OUT
+IN
Master 2
(V300B5C200B)
+S
SC
R5
49 k
–S
–IN
–OUT
+IN
+OUT
1N4148 430 Ω
R6
0Ω
F1
D2
PC
1:1
4
6
3
5
1N4148
Z1 10 Ω
R3
430 Ω
T1
PR
D1
Slave 1
(V300B5C200B)
–OUT
+IN
+OUT
1N4148
D2
PC
1:1
4
3
5
1N4148
Z1 10 Ω
R3
430 Ω
T1
PR
D1
Slave 2
(V300B5C200B)
+IN
+OUT
1N4148
PC
5
–S
–OUT
D2
1:1
+S
SC
–IN
F1
6
–S
–IN
F1
6
+S
SC
4
3
1N4148
Z1 10 Ω
R3
430 Ω
PR
D1
–IN
Slave 3
(V300B5C200B)
+S
SC
–S
–OUT
T1
1N4148
Group Enable / Disable
EN RTN
Figure 2 — Prototype array master board, one per system
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Applications Engineering: 800 927.9474
Page 3
Bypassing Not Shown (See Figure 4)
F1
+ Board Input
D2
+ Board Output
PC
+8 V aux._S1
1N4148
PR
R1 0 Ω
1:2
Q1
+OUT
+IN
Slave 1
(V300B5C200B)
– Board Input
–IN
+S
SC
–S
–OUT
4
+PR Bus
3
2
6
5
–PR Bus
T2
NP
R2
– Board Output
C1
R6
0Ω
200 nF
Z1 10 Ω
R3
D1
1N4148
430 Ω
1
F1
+OUT
+IN
D2
PC
8 V RTN_S1
6
4
5
3
1N4148
Z1 10 Ω
R3
PR
D1
1N4148
430 Ω
Slave 2
(V300B5C200B)
+S
SC
–S
–IN
–OUT
+IN
+OUT
T1
F1
D2
4
5
3
R3
D1
1N4148
430 Ω
Slave 3
PR
(V300B5C200B)
1N4148
Z1 10 Ω
1:1
6
PC
+S
SC
–S
–IN
–OUT
+IN
+OUT
T1
F1
D2
PC
Z1 10 Ω
1:1
4
6
3
5
1N4148
R3
PR
D1
1N4148
430 Ω
Slave 4
(V300B5C200B)
+S
SC
–S
–IN
–OUT
+IN
+OUT
T1
F1
D2
PC
1:1
4
6
3
5
1N4148
Z1 10 Ω
R3
430 Ω
PR
D1
1N4148
–IN
Slave 5
(V300B5C200B)
+S
SC
–S
–OUT
T1
Group Enable / Disable
EN RTN
Figure 3 — Prototype array slave board, four per system
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Applications Engineering: 800 927.9474
Page 4
C5
C3
4.7 nF
4.7 nF
+OUT
+IN
C1
0.15 µF
film
C2
33 nF
ceramic
PC
+S
DC-DC Converter
SC
PR
R1
–S
6.8 Ω
–IN
–OUT
C6
C4
4.7 nF
4.7 nF
Figure 4 — Differential-mode and common-mode bypassing for 5 kW array, each module
The PC pins of the converters have been diode OR’d to
provide group enable / disable for the array. An external
control circuit such as a microprocessor can provide this
signal. At a minimum, group undervoltage / overvoltage
lockout is required, see the Vicor application note
“Undervoltage / Overvoltage Lockout”. Because of voltage
drops between input leads of individual boards an
optocoupler must be used to correctly drive the PC pins.
Differential and common-mode bypass capacitors were
added close to each converter as shown in Figure 4. In
addition, a 24 µF capacitor in series with 6.8 Ω damping
resistor was added across the input of the entire array. See
Page 7 for information on how these values were chosen.
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Note: The high-power capability of the array’s input
source make proper safety precautions vital.
Individual fusing is required for each converter as
directed by the Design Guide and Applications
Manual. If the array is supplied by an offline source
an isolated scope should be used when making input
side measurements. Never apply power to an array
without connecting the output of the master board
and all slave boards to the same point. Failure to do
so will cause a destructive output overvoltage condition.
Applications Engineering: 800 927.9474
Page 5
Initial System Testing
Even the best array design will not predict all parameters
that will impact performance. Thorough testing during the
prototyping phase is recommended so that optimal
component values can be determined and potential issues
avoided. Tests may include dynamic loading, checking input
and output ripple, phase gain analysis, and PR bus signal
fidelity. For safety and to simplify testing, initial power up
should be performed on a subset of modules. For example,
the master board of the above array was tested first and the
system was subsequently checked as each new slave board
was added.
PR Signal Fidelity
Optimal component values for damping the PR bus were
found by testing the master board and one slave board (ten
modules total). The PR bus should always be checked with
an oscilloscope even if the array appears to behave properly.
Figure 5 — PR pin with insufficient damping, farthest
from master
Figure 5 shows the initial PR signal with series damping
resistors / ferrite beads (Z1), and shunt damping (R3, R4)
removed. This displays undesirable ring up due to parasitic
L and C. This pulse violates the 7 V absolute maximum
rating on the PR pin. Insufficient damping may cause the
pulse to make multiple transitions through the 2.5 V latching
threshold. This can cause extra power pulses to be
generated and should be avoided to prevent
module damage.
Figures 6 and 7 show the PR waveform on the primary
master and on the most distant slave module after the
damping is added. Both are examples of well-damped PR
pulses. The damping values shown are good starting values
for other array configurations.
Figure 6 — PR pin, primary master
The peak amplitude of the PR pulse should be at least 4 V
at every module for the pulse to be reliably detected, so
more damping is not always better. The forward voltage
drop associated with each emitter follower will add to PR
signal attenuation.
Figure 7 — PR pin, farthest from master
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Applications Engineering: 800 927.9474
Page 6
Figure 8 — 5 kW array input, full load
Figure 9 — 5 kW array input, full load, 24 µF bypass
Input Ripple
For the 25 module prototype, using a high input voltage
meant little low frequency bypassing was required. Input
impedance was low since the array was supplied with short
leads from Vicor’s 5 kW 3-Phase front end (Vicor P/N VITRY6-ICX). However, testing at full load uncovered a 2 kHz
oscillation on the DC input bus due to distribution inductance,
see Figure 8. This high-frequency ring is undesirable and
will increase the output ripple of the DC-DC converters. The
360 Hz ripple is from the rectified 3-Phase 60 Hz AC line.
To dampen this parasitic resonance, the following steps
were taken. First the nominal line input impedance for this
array was calculated:
Zin =
(VNL)2 η
Pconverter x N
=
(300 V)2 x 0.82
200 W x 25
Film or ceramic capacitors must be used due to the high
peak-to-peak ripple voltage on the DC input bus. The
lightly filtered bus has the advantage of keeping the power
factor of the supply high and minimizing inrush current.
Figure 9 shows the result of adding this capacitance
across the input terminals of the array.
The original ringing is gone but the added capacitors have
caused a lower frequency ring. This suggests series
damping resistance to reduce the Q of the added
capacitors. Adding about 10 Ω of damping in series with
these capacitors results in the input waveform in Figure 10.
This resistance was determined experimentally to give
optimal damping for the capacitor value chosen.
= 14.8 Ω
Where:
VNL is the nominal input voltage of the array
Pconverter is the output power of each converter
η is the minimum efficiency of the V300B5C200B modules.
N is the number of modules in the array
Solving for a capacitor with roughly five to ten times lower
impedance at 2 kHz gives about 24 μF.
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Figure 10 — 5 kW array input, full load, 24 uF bypass,
10 Ω damping
Applications Engineering: 800 927.9474
Page 7
Figure 11 — Input switching noise with two modules no
external differential bypass capacitors
Figure 12 — Input switching noise with two modules with
0.15 µF film differential bypassing
EMI
High-frequency bypassing at the input of each module in
the array can cut down on conducted noise before it can
escape to the rest of the system, greatly reducing the
demand for EMI filtering. Testing with several modules is
the easiest method to arrive at optimal input bypassing. For
example, Figure 11 shows the input waveform of two
modules with no bypassing.
This waveform shows significant undesirable switching
noise. To reduce it a 0.15 μF film capacitor was added at
the input of each module, Figure 4. The resulting waveform
is shown in Figure 12. Film capacitors were used because of
their moderate Q relative to ceramics.
Much of the high-frequency noise has been eliminated but
the ringing is undesirable. Series damping was added to
attenuate this ringing. A starting value for the damping
resistor can be found by calculating the characteristic
impedance of the 200 kHz ring wave:
Zchar =
1
2πf C
=
1
2π(200 kHz) 0.15 µF
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More information on high frequency bypassing can be
found in the Design Requirements section of the Maxi,
Mini and Micro Design Guide and Applications Manual.
= 5.3 Ω
Based on this result a 6.8 Ω damping resistor was added in
series with the 0.15 uF capacitor. This involved a tradeoff
because the resistor reduces attenuation of the highest
frequency components of switching noise. To regain low
impedance bypassing at high frequency a 33 nF ceramic
capacitor was added directly across the input of each
converter, see Figure 4. This was chosen because it
represents roughly one-fifth the value of the larger
capacitor and can thus be neglected at low frequency. The
effect of the final bypassing network is shown in Figure 13.
10/2013
Figure 13 — Input switching noise with two modules with
0.15 µF film differential bypassing, 6.8 Ω series damping
resistor, 33 nF ceramic differential bypassing
Summary
The techniques demonstrated in this example allow high
power arrays using Maxi, Mini and Micro converters to be
implemented with a minimum of design effort. With
nominal input voltages from 24 V to 375 V and outputs
from 2 V to 52 V this family of converters offer exceptional
versatility, reliability and ease of use. Vicor’s experienced
technical support can assist you in applying the benefits of
these converters to your high power application.
For more information, please contact Vicor’s Applications Engineers at
1-800-927-9474 or www.vicorpower.com/contact-us for worldwide
assistance.
Applications Engineering: 800 927.9474
Rev 1.1
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