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Model
SMM-1000 data sheet (download pdf file) High Resolution/Variable
Temperature LTS Magnetic Microscope
Model
SMM-770 data sheet (download pdf file)
HTS Magnetic Microscope (close gap - room temperature samples)
Model
SMM-601 data sheet (download pdf file) LTS Medium Resolution
/Room Temperature Sample Scanner

Microscope
Selection
Key
to deciding on the type of instrument to be used is the required
sensitivity and spatial resolution. Since these two features tend to be mutually
exclusive for a given device, the user needs to decide which
requirement is most critical. For example, micron resolution is
meaningless if there is not sufficient sensitivity to detect the
features being scanned.
The figures of merit used to assess these devices include:
¨The spacing between magnetic features
This is a key concern. A single dipole can be localized ten times better than
resolving two closely spaced dipoles. The smaller and closer the detection coil, the better.
¨How close
one can get to the magnetic feature
Getting much closer than a detection coil diameter gives no significant improvement in spatial resolution, especially for multiple sources.
In essence, the detectable feature size is a product of coil area and stand-off distance.
Tristan offers the following
types of scanning magnetic microscopes:
1)
Conventional LTS SQUID scanner - see Model SMM-601
2)
Scanning LTS SQUID Microscope - see Model SMM-1000
3)
Conventional HTS SQUID scanner - see Model SMM-701
4) Scanning
HTS SQUID Microscope - see Model SMM-770
¨
Model SMM-601
microSQUID LTS
SQUID scanner
This system uses a
niobium liquid helium (LTS) SQUID sensor and a separately wound
detection coil (or coils). It requires the detection coil to be
either immersed in liquid helium, or, alternatively, installed in
the vacuum space but thermally
anchored to a 4.2 K bath. Conventional coils can be wound to < 2 mm
diameter. Combined with a 2 mm stand-off, spatial resolutions (for a
single dipole) < 250 mm
are possible. The ability to use a three-dimensional structure for
the detection circuit allows significant external noise rejection.
Another advantage of niobium–based superconductors is the ability
of the detection coils to operate in tesla fields. This gives the
LTS microscope the ability to make susceptibility measurements on
the same spatial resolution scale. In addition, these systems can
operate in multi-gauss ac fields with dc – 50 kHz bandwidths for
eddy current measurements. The LTS SQUID scanner has the best field
sensitivity (< 20 x 10-15
T/ÖHz)
of any of the microscopes. Scanning areas can be tens of cm in both
x and y directions.
¨
Model SMM-1000
Scanning
Magnetic Microscope
This system uses a
monolithic array of SQUID sensors and LTS coils. Up to nine (linear
array) 14 mm
x 14 mm coils are at
the end of a cantilever that is suspended over the sample. The
sample is cooled to allow the detection coils to be within a few mm
of the sample, yielding 2 mm
spatial resolution. While that accuracy may not be sufficient to locate
a specific submicron transistor, it can place defects in the
vicinity so other tests can be performed. The use of superconducting
stepper motors allow 0.16 mm
X-Y resolution on the
scanning stage when covering a 5 mm x 5 mm scan area.
Since the sample and coils are both cooled, superconducting shielding can
be used to eliminate all external noise sources. Changing
samples requires the cryostat to be warmed and recooled; but, the use of load-locks may
allow SEM style sample handling. It is also possible to add field
generation coils to apply small dc and ac fields, useful for
susceptibility and eddy current measurements.
The LTS Scanning
Magnetic Microscope has a field sensitivity < 100 x 10-12 T/ÖHz.
A relatively mature technology, it has a low risk factor in terms of
technology development. One such system has been operating for
nearly ten years.
¨
Model SMM-701
HTS SQUID
Scanning System
The high temperature (HTS)
version of the microSQUID uses a YBCO HTS SQUID sensor that
operates at ~77 K, the boiling point of liquid nitrogen. The
inherent anisotropic nature of the HTS superconductors requires that
the planar detection coil be integral or inductively coupled to the
sensor, unlike the LTS microSQUID which uses 3-dimensional gradiometer
coils for improved noise rejection. Commercially available HTS
sensors have typically consisted of a single turn coil with an 8 mm
hole, and typical sensitivities ~ 30 x 10-15 T/ÖHz.
Decreasing the HTS coil size can improve spatial resolution, but at
a decrease in sensitivity (see below). Sensors can be made with 2 mm
standoff distances; the use of sapphire windows allow 50 mm
and smaller stand-off distances.
Unlike LTS SQUIDs, HTS
SQUIDs do not have the ability to operate in tesla fields. It is possible to operate a HTS microscope in up to 0.1 tesla fields. HTS
systems have been operated in milligauss ac fields with dc – 20
kHz bandwidths. This makes them the preferred (HTS) device for
susceptibility and eddy current measurements on macroscopic samples.
Like the LTS microSQUID, scanning areas can be tens of cm in both x
and y directions.
¨
Model SMM-770
HTS SQUID Microscope
Conceptually identical to
the Tristan LTS Scanning Magnetic Microscope delivered to NTT in
1995; this system uses HTS technology, with the detection coil having a
40 mm hole. With the sample
mounted in the
dewar vacuum space (but thermally anchored to the liquid nitrogen
bath or closed cycle refrigerator), stand-off distances < 100 mm
between detection coil and measurement sample are possible. The
SMM-770 system has a
sensitivity ~ 10-11 T/ÖHz.
Scanning areas can be up to 20 cm x 20 cm.
Unfortunately, its
magnetometer detection coil configuration makes the SMM-770 susceptible to
external noise sources. Operation in a shielded environment will improve noise immunity. By using phase sensitive detection
(injecting an ac current into the device under test), background
noise can be filtered out. The addition of external field coils make susceptibility measurements (dc or ac) possible.
One attractive use for
the SMM-770 system is the measurement of circuit board current traces. By overlaying
system images on a
CAD map of an IC or circuit board features, it is possible to locate
where actual faults occur. Under ideal conditions, a SQUID can
detect as little as 10 nA flowing in a conductor that is 100 µm
from the sensor.
Which to Choose?
The
choice of microscope system depends on the needed spatial
resolution and magnetic field sensitivity. Resolution (the minimum
separation between two magnetic features) is dependent on both the
distance from the sensor to the sample (stand-off) and the detection
coil size. If a SQUID microscope can place its sensor very close to
the sample (< 2 coil diameters), then the coil size is the
limiting factor to resolution.
Because
the flux sensitivity of SQUID sensors is roughly constant, there is
an inverse relationship between sensitivity and spatial resolution.
The figure below shows the trade off between sensitivity and spatial
resolution for a number of different SQUID based systems.
Sensitivity and Spatial
Resolution of a number of SQUID microscopes
The Table below shows the
capabilities of a number of Tristan magnetic microscopes.
|
System
|
Spatial
Resolution
|
Sensitivity
|
Scan
Area
|
Step
Size
|
|
1000
|
2
µm
|
100
pT/ÖHz
|
5 mm
x 5 mm
|
0.2
µm
|
|
770
|
<100
µm
|
20
pT/ÖHz
|
15 cm
x 15 cm
|
25
µm
|
|
601
|
2
mm
|
5
fT/ÖHz
|
30 cm
x 30 cm
|
25
µm
|
|
601S
|
0.5
mm
|
50
fT/ÖHz
|
30 cm
x 30cm
|
25
µm
|
|
660
|
0.5
mm
|
20
fT/ÖHz
|
Use
robot arm
|
25
µm
|
|
701
|
1
mm
|
30
fT/ÖHz
|
30 cm
x 30 cm
|
25
µm
|
Custom versions can be
supplied to achieve larger scan areas, smaller step sizes, etc.
Contact Tristan Technologies for additional information.
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