The FEI Nova 600 NanoSEM

The FEI Nova 600 NanoSEM Scanning Electron Microscope is a very versatile characterization instrument that produces enlarged images of a variety of specimens, achieving magnifications of over 500.000 times providing ultra high resolution imaging. At the time being this microscope is mainly designated for microstructural characterization using electron backscatter diffraction (EBSD) , Energy-dispersive X-ray spectroscopy (EDS) and forward scatter electron imaging by detectors recently bought from Bruker.

Who may operate the FEI SEM

Currently, Dr. Alice Bastos Fanta is co-ordinating all the activities that take place on FEI Nova 600 NanoSEM. So she must be informed about the planned activities before hand in the bi-weekly meetings which are held at DTU Nanolab. Alice makes the bookings in agreement with all the users. The rules of who may operate the FEI SEM and to what extent they may operate it are:

Only users who have been trained and approved by DTU Nanolab personnel may operate the instrument. Irregardless of their prior experience any new user with no official DTU Nanolab training or approval cannot operate the instrument, not even under close supervision by experienced users.

Users may only use the instrument to the extent they have been trained. This means that one should not try to operate the following options/capabilities without explicit training:
- Low vacuum
- EBSD capability
- EDX capability
- Backscatter detectors

How to operate the FEI Nova 600 NanoSEM

To find the basic instructions for operating the instrument, the reader is referred to the labmanager manual.

Processing guidelines on the FEI SEM

When one combines the 6 different detectors, 2 vacuum modes and 3 SEM modes with the traditional SEM parameters such as high voltage, working distance, spot sizes etc. it is clear that the FEI SEM has a huge number of different ways to be operated in. The number of ways that produce ultra high quality images is, however, limited. It is therefore crucial that the operators share their knowledge of how to obtain great images.

Steps to follow

There is no single general approach to taking good images on the FEI SEM. These points below are only guidelines.

What kind of images are needed

It is important to consider what kind of images are needed before you start. The different requirements/conditions could be some of the following:

High resolution at high magnification (above 10.000x) images are wanted: For conducting samples: Use TLD and mount the sample so that short WD's are possible.; For non-conducting samples: Mount the Helix detector and use short (app. 5 mm) WD.

Images of very thin (> 10 nm) metal films on low atom number materials: Use the backscatter detectors

Images with high resolution, large field of view and depth of focus are wanted: The TLD and Helix detectors do not provide large field of view and depth of focus when operated in SEM mode II.

Detectors on the FEI SEM

The FEI SEM has 6 electron detectors and 1 photon (X-ray) detector.

Tag	Name	Vacuum mode	Signal	SEM modes
ETD	Everhardt Thornley Detector	HiVac	SE, BSE (detector bias adjustable)	1 and 3
TLD	Through Lens Detector	HiVac	SE, BSE (detector bias adjustable)	1, 2 and 3
BSED	BackScatter Electron Detector	HiVac	BSE	1, 2 and 3
EBSD	Electron Backscatter Diffraction	HiVac	BSE	1 and 3
ARGUS	ARGUS(TM)	HiVac	BSE	1 and 3
LVD	Low Vacuum Detector	LoVac	SE + BSE	1 and 3
Helix	High resolution Low Vacuum detector	LoVac	SE	1, 2 and 3
GAD	Gaseous Analytical Detector	HiVac and Lovac	SE + BSE	1, 2 and 3
EDX	Energy Dispersive X-ray detector	HiVac and Lovac	X-ray photons	2 and 3

Equipment performance and process related parameters

Equipment		QFEG Cryo SEM FEI Quanta FEG 200
Purpose	Vizualization and Microanalysis	Vizualization of surfaces (topography and Z contrast) Vizualization of projected image (BF STEM image) Energy Dispersive X-ray analysis (EDS)
Performance	Resolution	The resolution of QFEG dependends on the sample and the operation mode!
Performance	Resolution	2 nm at 30 keV for Au on C sample with the ETD detector
Instrument specifics	Detectors	ETD- Everhart-Thornley for secondary electrons BSD- Solid state Back Scattered Detector LFD- Large Field Detector for secondary electrons GSED- Gaseous Secondary Electron Detector GBSD- Gaseous Backscattered Electron Detector GAD- Gaseous Analystical Detector STEM- right field Scanning Tramission Electron detector vCD- low voltage BSED CCD camera
	Electron source	Field Emission - Tungsten filament
	Stage (room temperature)	X, Y: 25 × 25 mm T: 0 to 60^o (Full tilt require removment of cryo cold trap.) R: 360^o
	Peltier stage	FEI Peltier stage -10^o to 22^o
	Cryo stage	Quorum PP2000 Cryo System
	EDS	Oxford Instruments 80 mm² X-Max silicon drift detector, MnKα resolution at 124 eV
	Operating pressures	High vacuum (10^-4 Pa), Low vacuum and Enviromental mode (up to 2700Pa)
Substrates	Sample sizes	No actual limit (limitted by stage movment and detector position).
	Allowed materials	Conductors, Semiconductors,Insulators,Wet Samples, Biological (not pathogents!)

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Characterization Techniques

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