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Studio monitor due
vie con woofer da 38cm mod. F2235H, medio-alto mod. F2421A con tromba
biradiale - freq. crossover 1000Hz - effic. 93dB - dimensioni
556x908x480mm - peso 79.5kg
Dal sito:
http://www.audioassembly.com/jblstory.htm
Un
marchio con un inizio veramente tormentato, James Lansing alla fine del
1949 aveva un debito per circa 20.000$ e Robert Arnold cercò di
aiutare James Lansing continuando a fornire Alnico V essendo J.Lansing
un grande sostenitore nell'utilizzo dell'alnico per i suoi altoparlanti.
Uno dei primi componenti ad utilizzare tale meteriale fu il woofer D101,
un poderoso 15 pollici con cupola in alluminio e foro posteriore per la
ventilazione, quasi immediatamente sostituito con il D130, sviluppato
con Robert Arnold utilizzando appunto l'Alnico V. Grazie a Lansing
questo materiale si affermò nell'industria e venne utilizzato sempre più
spesso.
Purtroppo nel settembre de '49 la tragica fine di J.B.Lansing...si
suicidò con un colpo di pistola. Fu grazie alla sua assicurazione di
10.000$ precedentemente sottoscritta ...che la JBL sopravvisse a tale
catastrofe finanziaria, William Thomas rilevando anche la parte che
James Lansing lasciò alla moglie, divenne nel 1950 unico proprietario
della James B. Lansing Sound. Lo scontro con la Altec durato diversi
anni portò al cambio definitivo del nome, ossia: JBL
Piccola industria che velocemente
conquistava clienti e appassionati, grazie a prodotti di notevole
qualità. Grande successo venne con la mitica Hartsfield e con alcuni
driver che hanno fatto veramente la storia dell'hi-fi e sonorizzazione
in generale. Thomas entrando in possesso di alcuni disegni del driver
WE594 e sostituendo data la qualità del progetto l'elettromagnete con l'alnico
V nacque il driver 375. Questo componente consentì alla JBL di entrare
nel grande mercato della sonorizzazione, sviluppando quasi
immediatamente lenti acustiche e trombe radiali. Il grande successo
arrivò con le "Paragon" del 1957, riferimento che rimase per oltre un
ventennio.... Oggi sono ricercati i grandi
monitor da studio che per anni hanno regnato incontrastati in
meravigliosi studi di registrazione.
Alcuni modelli tra i più ricercati per qualità sonora e costruzione -
foto - (
quotazione nel mercato dell'usato in
euro)
il valore nel mercato dell'usato varia a seconda delle condizioni, stato
del mobile, tele originali, loghi, crossover non modificato e non
ricablate, altoparlanti in ottime condizioni...deve essere assolutamente
tutto originale - riportiamo un minimo ed un massimo.
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JBL 4350A - 4350 WXA
(4800-6800)
|
Prima
produzione 1978 - doppio woofer da 38cm mod.2231A, mid-basso da 30cm
mod.2202A, driver medio mod.2440 con tromba mod.2311 e lente mod.2308,
tweeter mod.2405 -
risposta in freq. 30Hz/20KHz 3dB - freq. crossover 250Hz 1100Hz
9000Hz - effic. 95.5dB - dimensioni 1210x889x508mm - peso 110kg |
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JBL 4350BWX
(5000-6900)
|
Studio
monitor con doppio woofer da 38cm mod.2231H, mid-basso da 30cm mod.2202H,
driver medio mod.2440 con tromba mod.2311 e lente mod.2308, tweeter
mod.2405 -
risposta in freq. 30Hz/20KHz 3dB - freq. crossover 250Hz 1100Hz
9000Hz - effic. 95.5dB - dimensioni 1210x889x508mm - peso 118kg |
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JBL 4345
(4700-6000) |
Studio
monitor con woofer da 46cm mod. F2245H, medio-basso da 25cm mod.2122H,
medio mod.2421 con lente mod.2308, tweeter mod.2405 - risposta in
freq. 32Hz/20KHz 3dB - freq. crossover 320Hz 1300Hz 10000Hz - effic.
95dB - dimensioni 1096x765x470mm - peso 112kg |
|
JBL 4343 BWX
(4500-5800) |
Studio monitor tre vie con woofer da 38cm mod. F2231, medio-basso
mod. 2121, medio-alto mod.2420 con tromba mod.2307, lente mod. 2308,
tweeter mod.2405 - freq. crossover 300Hz/1250Hz/9500Hz - effic. 93dB
- dimensioni 635x1051x435mm - peso 85kg |
|
JBL 4333 BWX
(1900-2500) |
Studio monitor tre vie con woofer da 38cm mod. F2231, medio-basso
mod. 2121H, medio mod. 2420 con lente mod. 2307, tweeter mod.2405 -
freq. crossover 800Hz/8500Hz - effic. 93dB - dimensioni
619x778x497mm - peso 60kg |
|
JBL 4435
(2200-3200) |
Studio monitor due vie con doppio woofer da 38cm mod. 2234H,
medio-alto mod. 2421A con tromba biradiale - freq. crossover 1000Hz
- effic. 96dB - dimensioni 965x908x515mm - peso 114kg |
|
JBL 4430
(1900-2600) |
Studio monitor due vie con woofer da 38cm mod. F2235H, medio-alto
mod. F2421A con tromba biradiale - freq. crossover 1000Hz - effic.
93dB - dimensioni 556x908x480mm - peso 79.5kg |
Dal sito:
http://www.audioheritage.org/html/profiles/jbl/4430-35.htm
The
4430 and 4435 Bi-Radial Studio Monitors were amongst the most successful
professional loudspeakers ever produced by JBL. They were in production
longer than any other JBL main studio monitor, being introduced in 1981
and not discontinued until 1996 for the 4435 and 1999 for the 4430.
David Smith was the engineer responsible for the system design of these
monitors. The following is his account of the background and design of
these systems.
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2, 3
or 4 way?
A lot of the systems
that preceded the 4430/35 were 3 or even 4 way designs. Adding an 8”
lower midrange would certainly improve power handling and also clean
up the sound at high levels where the woofer’s excursion gets
significant. Putting a crossover between the main horn and a small
super tweeter type horn is problematic, though. The main horn
usually had a lot of depth whereas a super tweeter (such as a 2207)
would be considerably shorter. There would be several wavelengths of
separation if they are both front mounted on the cabinet, leading to
comb filtering in the crossover region. Pushing the supertweeter
back to the point where the voice coil planes are aligned can remove
the comb filtering although it isn’t always practical and doesn’t
work over much of a vertical range of angles. If your main horn has
the bandwidth then you are better off equalizing a bit than crossing
over to a super tweeter at a high frequency. (This is just my
opinion and I do realize that a lot of great JBL speakers were
designed contrary to this.) |
I came to JBL in
September of 1980. It was my second job in the industry. I had started
out in an obscure OEM speaker company called Essex Cletron in Cleveland.
When Essex announced that they were moving the engineering department to
Indiana I thought it was a good time to move on. Interestingly, soon
after their move they were bought by Harman and turned into
Harman-Motive, a long lasting and highly profitable sister company for
JBL.
At the time
JBL had a good line of studio monitors including the 4350, the 4343 and
the 4315 (a product I much admired). The 4343, and especially the 4350,
were very large and were sometimes referred to ironically as "Japanese
bookshelf speakers". This is not a slur on their quality, but more
reflected their great popularity in the Asian market. As a practical
issue their sheer size made them a little over the top. Studios
typically build their main monitors into soffets over the control window
and the 4350 was just too big. The biggest problem, though, was that
UREI was stealing market share with their 811 and 813. These were based
on an Altec 604, always a popular unit, with a "time aligned" network
and some enhancements to the horn. The sound was good enough and the
size was reasonable and it had a good story in the time aligned network.
Don Keele
had just gotten his constant directivity horn design software going. You
might know that he had really pioneered the first constant directivity
horns while at EV. He also patented their design. Altec made thinly
veiled copies with their "Manta Ray" horns. Don, now at JBL, was to
develop a line of horns and at the same time needed to change the design
enough to get around the other patents. The biradial horns were the
answer and they were extremely good. One of the first units he developed
was a 100 by 100 degree horn. The larger 90 by 40 and 90 by 60 horns
were more for theater applications but this smaller, wider angle horn
was a natural for a studio monitor. If you look at the polar patterns
that are in the AES paper we wrote you can see that the polars are
incredibly uniform from 1000Hz to 16,000 Hz.
|
Why does the 4430’s horn roll off?
It doesn’t, actually. All
compression drivers have an inherent roll off related to their
diaphragm mass. This “mass breakpoint” usually occurs around 3 kHz.
In the lab we would measure a compression driver on a terminated
tube. In practice this is a long pipe (perhaps 4 to 6 ft long) with
a thin fiberglass wedge in it. A small microphone is inserted into
the side of the pipe near the compression driver. This presents the
compression driver with a resistive acoustical load so that pressure
in the tube represents what the output of a perfect horn would have.
Measured in this way most of the JBL compression drivers would have
flat response from several hundred Hz to about 3kHz. At 3k they
would start a gentle rolloff at 6dB per octave until phase plug
design and diaphragm modes took over above 10kHz. You may know that
Fanchur Murray did all the compression driver design at JBL in the
80’s. In my opinion his greatest achievement was the diamond
surround and getting the 2” and 4” compression drivers to have
smooth response out well beyond 15kHz.
Anyhow, this rolled off
response is the raw response that is presented to the horn. The
horn then modifies this response via its acoustic load at the low
end its and via its directivity index at the high end. (Directivity
index represents the on axis gain. It is essentially the
“beaminess” of the horn expressed in dB.) Prior to the constant
directivity horns most people assumed that horn/compression driver
combinations should have inherently flat response. Horns were
evolved that in effect “equalized” the compression driver. This
ignored the fact that the combinations could only be flat, and only
on axis, if the horn exhibited a great amount of high frequency
beaming.
With the 100 by 100 horn
the polars are so consistent and the directivity index so flat that
the on and off axis response looks just like the terminated tube
measurement of the compression driver. It is up to the crossover
network to take this rolled off response and makes it flat. |
To explain
the biradial name, there were a lot of radial horns at the time.
Probably the best known examples were the Altec 511 and 811. They took a
vertical cross section designed for exponential area growth and rotated
this cross section around an apex back in the throat (in effect a radial
swing). Slice such a horn from front to back at any angle (through the
vertex) and the cross section would be the same. Designing a horn in
this way gave good extension to its theoretical cutoff, but poor polar
response and a lumpy frequency response that contributed to “horn
colorations”. Two independent variables were at play here. The first,
the rate of area growth, defines the acoustic load that governs the
radiated power curve for the first octaves above cutoff. Independently,
the wall contours determine the polar pattern versus frequency. It works
out that the side wall angles near the compression driver primarily
determine the high frequency directivity. Contours farther out the horn,
as the dimensions grow, progressively set the polar curves for lower and
lower frequencies. Don developed a sidewall contour that gave a great
polar pattern for a wide range of frequencies. These contours (or one
contour used twice in the case of a 100 by 100 degree horn) were then
used for the horizontal and the vertical shape. With his new designs the
special contours were rotated twice around two radial points, hence the
name biradial.
One part of
the mechanical development of the 4430/35 was of the 100 by 100 horn
castings. I remember working with Mark Gander on their construction.
First samples were from a low tech molding process (reaction injection
molding?) and always a little warped. The back surface that would have
to seal to the cabinet tended to bow forward. General quality was much
improved by the time production rolled around.
As an aside,
a lot of the evolution of horns has been tied to their construction
processes. Early horns were usually of a multicell design because a
tinsmith could solder them up. More complex horn shapes wouldn’t become
practical without molding techniques. Horns that were expected to sell
in volume could be cast in aluminum, such as the Altec 511 and 811. Don's
big theater horns would have been cost prohibitive (and heavy) if
aluminum diecast due to their large size and relatively low projected
sales volume. They ended up being made in fiberglass with reinforcement
panels molded in. The 4430 horn was a little tricky because it needed
side extraction of the tool for the lateral pockets. It also had a
separate sand cast throat section that was bolted on from behind and
linked the front to the compression driver. Getting the cross section
and the juncture between the two just right impacted the response so we
played with that variable a fair bit.
Don had
just started on a crossover network when I took over the project. I
remember that there was a lot of work to get the midrange and tweeter
controls to work sensibly. Also a lot of work to get the octave to
octave balance right and also to insure the balance of the 4430 and 4435
were identical even though the 4435 was three dB more sensitive. There
were a number of listening sessions with Gary Margolis and John Eargle
which I, as a young engineer, found very instructional. They had good
ears and could identify what octave needed to go up or down a dB to get
the balance just right and I wanted to be able to do that!
|
How to improve the 4430/35
The only real negative
of the biradial horn designs was that the concentration on great
polar response sometimes was at odds with the ideal of exponential
area growth. This resulted in some ripple to the first couple of
octaves of the horn’s response.
The bottom end of a horn/compression
driver combo is largely determined by the rate at which the horn’s
area grows. Back in the acoustical gramophone days mathematicians
had figured out that Exponential area growth gave the most extended
acoustical load to the transducer. Exponential growth simply means
that the cross sectional area grows a constant percentage for a
fixed unit of length along the horn. The slower the area grows the
lower the cutoff frequency. For example a 500 cycle cutoff would
dictate that horn area should double every 38 millimeters. A 250
cycle horn would grow half as fast with area doubling every 76 mm.
For a horn to work well to a certain frequency it will need
appropriate exponential growth and also a certain minimum mouth
area. You must have both. Having a low flare rate but with
inadequate mouth area will lead to choppy response in the horns
first octaves.
In the original biradial
horns the only truly exponential part was the short section from the
exit of the compression driver to the gap that fed the horizontal
flare. Making the gap narrow gave great horizontal polars up to a
high frequency but pushed the exponential cutoff frequency down to
the point that the area didn’t support it. The consequence was a
periodic ripple in frequency response. It wasn’t real bad…about 2 dB
total ripple.
If you look at the
impedance curve you see impedance peaks that correspond to the
response peaks. This gave a challenge in the network design. You
needed to keep the networks driving impedance low otherwise the
voltage at the compression driver would start to follow the ripple
of the impedance curve and make the response worse.
With the 4430 network
the driving voltage had a ripple of about 1 dB and so the horn’s
total ripple was about 3 dB. The consequence of the ripple was a
slight coarsening of the sound of the midrange, most noticeable on
pink noise. I always thought that biamping would help a little here
(directly coupling the amplifiers low output impedance to the
compression driver) but what would be really neat would be to drive
it with and amplifier with a slightly negative output impedance.
This is can be achieved with various amplifier feedback schemes.
Then for every frequency where the impedance bumps up the amplifier
output voltage would actually drop. A negative output impedance
amplifier would act to equalize the first couple of octaves of the
horn’s response to something really smooth. Any experimenters out
there up to the task?? |
Equalization of the horn/compression driver was the only
out-of-the-ordinary issue for the 4430/35 network. As mentioned above
the high frequency section will have an inherent 6dB per Octave rolloff
above 3kHz. A passive network can equalize that as long as the inherent
sensitivity stays high enough to the highest frequency needed. The
sensitivity of the 2425 compression driver on the 100 by 100 horn was
about 108 dB from 1000 Hz up until its rolloff above 3K. By 16K the
response had dropped to about 94dB, just enough for the 93dB target of
the 4430 and near enough for the 96dB 4435.
The upper
section of the network started out as a second order filter followed by
an L-Pad for overall treble level and with a first order bypass (a small
capacitor around the L-Pad) to give the highest frequencies a path
around the L-Pad. Basically the L-Pad would pull the lower treble down
about 16dB, the bypass would push the highs back up and equalize the
horn.
A couple of
issues needed to be dealt with: First, the first order bypass approach
still lost a couple of dB at 16kHz, leading to a softer top end than was
desired. Secondly, it would be nice to have sensible response controls
for the system. The L-Pad, because it was bypassed, would only have
effect from 1 to 5kHz. It would become a “lower treble” control. I
wanted separate controls for both the lower treble and upper treble,
more in keeping with our other 3 and 4 way systems.
A solution
for both was to use a series resonant bypass network. 1 microfarad in
series with about .08 milihenries would resonate around 15K and give
about 2 dB more output for the highest frequencies. It also gave a
little less around 5k where the 2425/biradial combo was a little hot. A
variable resistor in series the resonant leg gave a nice “upper treble”
adjustment so we now had a pair of controls with really useful control
centers and range.
After
getting the horns working the woofer section was tackled. The woofer
section was a straight second order network with a conjugate to flatten
out the woofer’s inductance. Using a conjugate lets you achieve a more
“classic” looking second order rolloff since the network inductor and
the woofer’s inductance wouldn’t be interacting. Most of the work in
this network was in getting the best blend between woofer and horn.
When the woofer and network shape looks about right you have to see how
the sections add. Do they add well in phase? Or in reverse phase? At
what axis do they sum best, and is that where you want them to sum
best? It turns out that with the crossover slopes used and the relative
depths of the woofer and horn that the units gave best summing connected
in phase (++ we would say) on a measuring axis that was straight out or
slight rising. The 0 degree and 15 degree up curves were both about
equally good. This would work well if the system was floor standing or
even if inverted and mounted over a studio window.
At this
point we now have a system with all the sections working and giving a
reasonable response curve. We still aren’t done though. At this point
you call over the marketing guys with the golden ears and everyone has a
listen. The curve will be massaged a dB here and a dB there until the
group (primarily Gary Margolis and John Eargle for this product) is
happy.
I was keen
to give a paper on the monitors. Since they were the first to use a
constant directivity horn there was some merit to a paper and so I
received permission to write it. I did most of the writing, although
John Eargle corrected a lot of my grammar and finessed the introduction
and my wife captioned the illustrations! If you read between the lines
of the paper you can see that we were taking some potshots at the UREI
product.
I was
pleased that the products were well respected by the Pro community and
stayed in the line for a long time. The 4400 series grew after these
models. I designed a 4401 and 4411 and after I left JBL Greg designed a
baby 4430, the 4425. One thing that was amusing at the time was how
people reacted to the shape of the new biradial horns. I remember more
than one studio engineer referring to them (affectionately!) as the
“Dolly Parton” horns or “Baboon butt monitors”.
©





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Il filtro per la
biamplificazione: |



Diffusori davvero
magnifici , precisi , dettagliati e sopratutto cattivi !!!!
http://www.jblpro.com/pub/technote/tn_v3n01.pdf
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punto vendita di : |
E tanto Altro
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