BACKGROUND OF THE INVENTION
1. Field of the Invention
[0001] The present invention relates to a dynodes arrangement for an electron multiplier.
In particular, the invention is utilized in scintillation gamma cameras for nuclear
diagnosis purposes.
2. Description of the Prior Art
[0002] It is known that the gain of photomultiplier tubes (PMT's), in particular those which
are utilized in scintillation gamma cameras, changes with time. Due to this, PMT's
have to be retuned from time to time.
[0003] The British Patent Application 2,067,281 describes a method and circuitry for retuning
by means of an automatic gain control (AGC) amplifier.
[0004] Further, the British Patent 977,827 illustrates a method and circuitry for retuning
by modifying the potential of the anode and some of the dynodes, when the total gain
of the photomultiplier exceeds a predetermined value, by directly connecting together
the anode and a number of dynodes which are closest to the anode.
[0005] Finally, the European Patent Application 0,066,763 delineates a method and circuitry
for retuning by means of varying the potential difference between to neighboring dynodes.
[0006] However, it is also possible to retune the gain of a photomultiplier by means of
varying the of high voltage.
[0007] The aforementioned two methods, namely controlling gain in a photomultiplier tube
for retuning by means of varying the interdynode potential differences or by means
of changing the high voltage are the easiest methods. However, these methods have
also some limitations. These limitations include for example
a) that the peak linear and peak saturated output current from the photomultiplier
tube is reduced in the reduced gain state;
b) that non-linear effects occur as the gain is decreased;
c) that the transit time of the photomultiplier tube is increased as the gain is decreased;
and
d) that the gain changes with the count rate (e.g., increased count-rate-shift effect
at decreased gain).
[0008] Page 3 of the brochure "Nucleonics Data", issued by Johnston Laboratories, Cockeysville,
Maryland 21030, Number JLI-605, illustrates a dynodes arrangement wherein a grid is
positioned between each two neighboring dynodes. The grid is always electrically connected
with one of the two neighboring dynodes.
[0009] The copending application Serial No. 343,207, filed January 27, 1982, by Dennis E.
Persyk, entitled "Radiation Detector Assembly for Generating a Two-Dimensional Image"
shows a radiation detector having a photocathode, an electron multiplier such as a
multichannel plate, and a grid positioned between the photocathode and the electron
multiplier. A first electrical field is provided between the photocathode and the
grid and a second electrical field is provided between the grid and the electron multiplier;
whereby the strength of the second electrical field is larger than the strength of
the first electrical field. Due to this the impingement area of a packet of photo
electrons on the electron multipier input is enlarged and thus, simultaneously, the
electron density is reduced, which in certain applications is a favorable result.
SUMMARY OF THE INVENTION
1. Objects
[0010] It is an object of this invention to provide a dynodes arrangement which allows improved
technically simple gain control of an electron multiplier.
[0011] It is a further object of this invention to provide an dynode arrangement which allows
improved technically simple gain control for a photomultiplier tube in a scintillation
gamma camera.
2. Sumary
[0012] According to this invention a dynodes arrangement for an electron multiplier is provided
which comprises:
a) a first dynode having a first voltage input;
b) a second dynode having a second voltage input; and
c) a control grid positioned between the first and second dynodes and having a control
voltage input separate from the first and second voltage inputs of the first and second
dynodes.
[0013] The control grid allows for tuning of the gain of a photomultiplier tube in a technically
simple manner, whereby all aforementioned limitations of the prior art do not any
longer influence the tuning process.
[0014] According to this invention also a photomultiplier tube is provided which conprises:
a) a photocathode;
b) an-anode; and
c) a dynodes arrangement between the photocathode and the anode including
cl) a first dynode having a first voltage input;
c2) a second dynode having a second voltage input; and
c3) a control grid positioned between the first and second dynodes and having a control
voltage input separate from the first and second voltage inputs of the first and second
dynodes.
[0015] Furthermore, according to this invention a scintillation gamma camera is provided
which comprises:
a) a scintillation crystal;
b) a number of photomultiplier tubes mounted behind the scintillation crystal, wherein
each photomultiplier tube having
bl) a photocathode;
b2) an anode; and
b3) a dynodes arrangement between the photocathode and
the anode including
b31) a first dynode having a first voltage input;
b32) a second dynode having a second voltage input; and
b33) a control grid positioned between the first and second dynodes and having a control
voltage input separate from the first and second voltage inputs of the first and second
dynodes.
[0016] The foregoing and other objects, features and advantages of the invention will be
apparent from the following more particular description of preferred embodiments of
the invention, as illustrated in the accompanying drawings.
BRIEF DESCRIPTION OF THE DRAWINGS
[0017] In the drawings:
Fig. 1 is a cross section of a photomultiplier tube comprising a dynodes arrangement
according to the invention;
Fig. 2 is an enlargement of a portion of the dynodes arrangement in the photomultiplier
tube of Fig. 1 comprising the invention; and
Fig. 3 is a cross section of a scintillation gamma camera including photonultiplier
tubes which comprise dynodes arrangements according to the invention.
DESCRIPTION OF THE PREFERRED EMBODIMENTS
[0018] In Fig. 1 a photonultiplier tube 10 comprises a housing 12 having an optical input
window 14. Behind the input window 14 is positioned a photocathode 16 with the high
voltage HV. The anode is generally designated-by 18.
[0019] Between photocathode 16 and anode 18 is placed a dynodes arrangement 20 according
to the invention. The dynodes arrangement 20 comprises a number n (e.g. at least n=4)
of dynodes DY1 to DYn.
[0020] Interposed between two dynodes, namely DY
i and DY
i+1 , are a first screen grid Gl, a control grid G2 and a second screen grid G3. The
dynodes DY1 to DYn and the screen grids Gl and G3 between dynodes DY
i and DY
i+1 are connected by means of an ohmic resistances voltage divider Rl to Rn with a voltage
supply source V. The control grid G2 is also connected with the voltage supply source
V by means of variable ohmic resistance (potentiometer) R
v.
[0021] According to the enlargement of Fig. 2 the dynodes are so-called venetian-blind dynodes
comprising each a transparent grid 22 across its top (electron-impinging surface)
as is customary to reduce electric field penetration from the preceding dynode. However,
it is understood that instead also other dynode types, such as box-and-grid, circular
cage, mesh dynodes, etc., can be utilized in connection with the invention. The spacings
between the grids Gl, G2, G3 and the neighboring dynodes DY
i and DY
i+1, are generally designated by dl,2; d2,3; d3,4 and d4,5.They are preferably equispaced
(dl,2 = d2,3 = d3,4 = d4,5).
[0022] The grids Gl, G2 and G4 have-an optical transparency of about 98% and similar electron
transparency. Photoetched grids would be satisfactory.
[0023] The potentials applied to dynodes DY
i, DY
i+1 and the grids G1, G2, G3 are designated VDY
i, VG1, VG2, VG3 abd VDY
i+1. Normally V
DY
i - VDY
i+1 = 100 volts. The potentials applied to Gl and G3 are given by the following equations:



[0024] Typical potentials are:
VDYi = -300 V
VDYi+1 = -200 V
VG1 = -300 V - (-100 V x 1/4) = -275 V
VG3 = -300 V - (-100 V x 3/4) = -225 V
[0025] The "normal" potential of G2 in the middle position of variable ohmic resistance
R
v is VG2 = -250 V.
[0026] Grids Gl and G3, acting as screen grids, do not perturb the electron optics of the
interdynode cavity because they are placed at the potential that would normally exist
in their respective planes or curved surfaces.
[0027] Now gain control is obtained by varying the potential of G2, the control grid, from
its "normal" potential of -250 volts to a value of -300 V, or even slightly more negative
than VDY
i. An electron created on dynode DY
i has a finite initial energy of 5 to 10 electron volts. Thus to obtain maximum cut-off,
G2 must be 5 to 10 volts nore negative than DY
i to account for initial energy effects.
[0028] It is known, that the space-charge limited current density between a planar cathode
and anode has a maximum of

[0029] While in normal PMT operation this equation does not apply, it does become important
in prior art gain control schemes. In particular, as the interdynode potential difference
is reduced, both the electron ballistics and the linearity of the photomultiplier
tubes are modified due to space charge effects. The results are the aforementioned
disadvantages of the prior art dynodes arrangements.
[0030] In a prior art dynodes arrangement with an interdynodes distance of for example d=4mm,
an interdynode potential reduction of Vr=50V from the normal interdynode potential
difference ΔV = 100V, Eo = 8.85 x 10
-12F/m,
e = 1.
6 x 10
-19C, and m
= 9.
11 x 10
-31kg the space-charge limited. current density is i = 5.15mA/cm
2. The dynamic range is 2:1.
[0031] In the dynodes arrangement according to this invention the space-charge region is
d2,3 = 1mm and Vr = 55 V for cut-off. The space-charge limited current density then
is i = 95 mA/cm
2. Thus the invention affords a far greater dynamic range of gain modulation (20:1
or more, contrasted to prior art 2:1 range), plus an 18-fold improvement in space-charge
limited (saturation) current.
[0032] The invention also decreases the device transit time shift as gain is modulated.
In prior art the -potential difference between two dynodes is decreased from 100 V
to for example 50 V with an acccnpanying transit time increase fron about 3 ns to
about 5 ns. According to this invention the drift space over which the gain is controlled
is very narrow, so that the change in transit time is much smaller, e.g., less than
1 ns. This is for example important in fast coincidence circuits of the kind used
in positron ECT.
[0033] The most novel aspect of this invention (which differentiates it from an ordinary
pentode) however, is that the count-rate-shift problem is overcome. Any change in
electron space current distribution within a photomultiplier tube causes the gain
to vary due to non-uniform dynode surfaces and non-uniform interdynode electron transfer
efficiencies. This is most serious in first-pass studies. According to this invention,
the current is altered in a narrowly confined region. Due to this the electron trajectories
are not altered significantly. Rather, some electrons simply do not transfer from
one dynode to another.
[0034] Another advantage of a dynodes arrangement according to this invention is that it
may be used to gate off a photomultiplier tube without changing gain in the period
following gating-on. This is important in certain procedures using short half-life
radioisotopes such as
95 Au. It may be desirable to protect the photomultiplier tube from initially-high anode
currents until the dose decays to a lesser intensity. With prior art the dynamic range
was too small (2:1) and a transistion period of varying gain would accompany a rapid
transition from "tube-off" to "tube-on".
[0035] The aforedescribed embodiment conprising one control grid and two screen grids is
only a preferred embodiment of this invention. Other implementations comprising different
number of grids, for example only one control grid or one control grid and one screen
grid, are also possible.
[0036] Photomultiplier tubes comprising a dynodes arrangement according to the invention
are particularly implemented in scintillation gamma cameras cf the Anger type. Such
a scintillation gamma camera is for example illustrated in Fig. 3. The camera 30 comprises
a scintillation crystal 32 which is connected with a light conductor 34 having pads
36. On each pad 36 is mounted a photomultiplier tube 10 according to Fig. 1. The canera
housing is generally designated by 38. The element 40 is an aluminum cover for the
scintillation crystal 32.
[0037] The dynodes arrangenent of this invention may also be implemented in single tube
scintillation cameras.
[0038] Having thus described the invention with particular reference to the preferred form
thereof, it will be obvious to those skilled in the art to which the invention pertains,
after understanding the invention, that various changes and modifications may be made
therein without departing from the spirit and scope of the invention as defined by
the claims appended hereto.
1. A dynodes arrangement for an electron multiplier, comprising:
a) a first dynode (DYi) having a first voltage input;
b) a second dynode (DYi + 1) having a second voltage input; and
c) a control grid (G2) positioned between the first and second dynodes (DYi; DYi + 1) and having a control voltage input separate from the first and second voltage inputs
of the first and second dynodes.
2. The dynodes arrangement according to claim 1, further comprising an additional
number of screen grids (Gl, G3) positioned between the first and second dynodes (DYi, DYi + 1) and the control grid (G2), each screen grid (Gl, G3) having a screen grid voltage
input.
3. The dynodes arrangement according to claim 2, further comprising voltage means
for supplying biasing voltages to the first and second voltage inputs of the first
and second dynodes, the control voltage input of the control grid and the screen grid
voltage inputs of the screen girds, wherein the location of the control grid and each
screen grid in the interdynode cavity between the first and second dynodes and the
values of the corresponding grid voltage are adjusted with respect to each other such
that each grid is placed at the potential that would normally exist in the respective
plane or curved surface of the grid location between the first and second dynodes.
4. The dynodes arrangement according to claim 3, further comprising means connected
with the control voltage input of the control grid for varying the biasing voltage
of the control grid.
5. The dynodes arrangement according to claim 2, wherein a control grid is placed
between a first and a second screen grid and all three grids are arranged between
the first and second dynodes.
6. The dynodes arrangement according to claim 1, comprising a plurality of additional
dynodes arranged in parallel to the first and second dynodes.
7. A photomultiplier tube, comprising:
a) a photocathode;
b) an anode; and
c) a dynodes arrangenent between the photocathode and the anode including
cl) a first dynode having a first voltage input;
c2) a second dynode having a second voltage input; and
c3) a control grid positioned between the first and second dynodes and having, a control
voltage input separate from the first and second voltage inputs of the first and second
dynodes.
8. A scintillation gamma camera, comprising
a) a scintillation crystal; and
b) a nunber of photomultiplier tubes mounted behind the scintillation crystal, wherein
each photomultiplier tube having
bl) a photocathode;
b2) an anode; and
b3) a dynodes arrangement between the photocathode and the anode including
b31) a first dynode having a first voltage input;
b32) a second dynode having a second voltage input; and
b33) a control grid positioned between the first and second dynodes and having a control
voltage input separate from the first and second voltage inputs of the first and second
dynodes.
9. The dynodes arrangement according to claim 6, wherein the control grid is positioned
between a first and second dynodes which are located one half way along the plurality
of dynodes.
10. The dynodes arrangement according to claim 6, wherein the combination of a control
grid and a number of screen grids is positioned between a first and second dynodes
which are located one half way along the plurality of dynodes.