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Basic Detector Operation 

Octane Basic User Guide 

Page 18 of 25 

 

4.5

 

LIGHT ELEMENT OPERATION 

1.

 

Check that the geometry is correct when collecting spectra. For example, an incorrect tilt used, 
giving an incorrect Take Off Angle, will affect the Quant results. You can also correct this after 
the data has been collected by editing the spectra file parameters. 

2.

 

Check that you are using a well-defined peak when quantifying. Avoid using peaks that are 
“buried” in the background. 

3.

 

Use one of the longer amp times when specifically looking for light energy elements. They 
typically provide better light element performance. 

4.

 

Use low accelerating voltage when specifically looking for light energy elements.  

3.

 

Make sure the samples are flat and homogeneous when possible. 

4.

 

Collect for sufficient time to improve the statics when the peaks are very small, for example 
when looking at Boron. 

 

4.6

 

FREQUENTLY ASKED QUESTIONS (FAQ) 

Q1. Should I leave the detector powered on all of the time? 
A1.
 In most laboratory conditions (stable power, temperature controlled), leaving the detector powered 
on all of the time is fine.  
 
Q2. Should I leave the detector cold all of the time? 
A2.
 The detector will reach operating temperature in about two minutes, so it does not need to be left 
cooled when not in use. Spectra can be collected after the detector reaches its operating temperature, 
but for optimal performance and stable peak positions, it may be best to wait about 60 minutes. It is 
okay to leave the detector cold when the microscope chamber is left under vacuum. There is a user 
preference option in the software to automatically turn the cooling off after inactivity, in case the user 
prefers to turn the cooling off automatically.   
 
Q3. The software displays a message that the detector temperature is not changing, or a 
communication problem with the detector. What should I do? 
A3.
 In this case, power off the detector using the switch on the small black power “brick” for the 
detector then reboot the PC.  Then power the detector back on after Windows has started. 
 
Q4.  How often should I calibrate? 
A4
.  Many labs only calibrate their systems during a regularly scheduled service preventative 
maintenance visit.  The detector will need to be calibrated in some cases when then spectrum peaks do 
not match the blue line modeled peaks.  For this case, a calibration will bring the peaks into alignment 
with the modeled line. In other cases, labs may want to set a regular calibration schedule any time from 
weekly to monthly.

    

 
Q5. What count rate should I use to calibrate? 
A5
.  We recommend using a copper and aluminum sample with a primary beam at ≥ 20 kV. Adjust the 
sample position so both Copper and Aluminum can be seen on the same screen. Set the position so the 
Copper and Aluminum Kα peaks are similar in height, but with the Al peak larger than the CuK peak by 
20 to 50%. Set the beam conditions so the Dead Time is ≤ 40% as you should use during normal use. 
 

Содержание Apollo XF Octane

Страница 1: ...Apollo XF XLT Octane Basic User Guide Rev 1 5 June 24 2016...

Страница 2: ...uide Page 2 of 25 The Apollo XF Apollo XLT and Octane detectors are manufactured by EDAX a business unit of Ametek Inc Materials Analysis Division 91 McKee Drive Mahwah NJ 07430 USA 201 529 4880 edax...

Страница 3: ...Do not expose the detector to extreme temperatures 10 2 6 8 Do not expose the SUTW to plasma 10 2 6 9 Windowless detectors 10 3 Installation and Environment Requirements 11 3 1 Power requirements 11...

Страница 4: ...Contents Octane Basic User Guide Page 4 of 25 This page is intentionally left blank...

Страница 5: ...r SEM Octane Plus 30 mm2 SUTW for SEM Octane Super 60 mm2 SUTW for SEM Octane Ultra 100 mm2 SUTW for SEM Apollo XF 60 mm2 SUTW for SEM Octane Prime1 10 mm2 SUTW for SEM Apollo XLT 30 mm2 SUTW for TEM...

Страница 6: ...Introduction Octane Basic User Guide Page 6 of 25 This page is intentionally blank...

Страница 7: ...hot swappable unless otherwise specified The power to the system must be turned off before inserting or removing any of the modules boards or any of the interconnecting cables If this precaution is n...

Страница 8: ...were introduced to the EDS market several years ago to improve the transmission of low energy X rays e g B C N O through the window The SUTW is constructed of a 300 nm thick polymer foil with an addi...

Страница 9: ...oose particles Avoid venting the sample chamber too quickly Specifically do not exceed 10 cm s gas velocity into the chamber as this can increase the risk of particle induced detector window damage Th...

Страница 10: ...indow or may cause the temperature at the window to exceed manufacturer s specifications This may occur during a microscope chamber bake or operation of a heat stage Recommendations If there is a poss...

Страница 11: ...5 watts 100 240 Volts 47 63 Hz 0 5 to 1 25 Amps Table 2 Power requirements 3 2 SPACE AND WEIGHT SPECIFICATIONS Workstation dimensions 17 5 H x 7 75 W x 19 5 in 44 x 20 x 49 5 cm Workstation weight 33...

Страница 12: ...Installation Requirements Octane Basic User Guide Page 12 of 25 This page is intentionally blank...

Страница 13: ...sis software By default there is an Administrator login set up for TEAM Figure 1 Detector Power Supply 4 2 DETECTOR COOLING By default detector cooling is Off until it is started by the user When the...

Страница 14: ...N Ramping GREEN At Operating Temp Blinks RED Warming Table 4 Status LEDs definitions When the detector is first powered ON both Status lights on the detector back panel will light RED There is a Yello...

Страница 15: ...EAM Status Indicator Green Red OK to Vent DU is warm OK to vent microscope DU is cold Not OK to vent microscope for Window less DU Ready DU is cold OK to collect spectra DU is not ready to collect spe...

Страница 16: ...e Some or all may simply be software buttons that the user must acknowledge that it is ok to cool the detector Toggle so each Safety Interlock is Green Figure 4 Detector control and detector status fo...

Страница 17: ...n This high count condition is normally set by the factory or installation service engineer The purpose is to protect the detector from high energy backscattered electrons in a TEM which can be harmfu...

Страница 18: ...ut for optimal performance and stable peak positions it may be best to wait about 60 minutes It is okay to leave the detector cold when the microscope chamber is left under vacuum There is a user pref...

Страница 19: ...5 1 TYPICAL WORKSTATION CONFIGURATION Figure 6 PC Workstation Connections Power Supply Air Flow Hard drive USB Restore SG 3 Board Fan Air Flow Internal Sync cable Sync Panel Network Board Card bracke...

Страница 20: ...Ie 2735 171 30939 IP 192 168 0 101 SYNC PCIe 5335 007 28300 SG 2 PCI 5335 007 20000 Mains 24V Power Supply 2735 171 31074 Microscope Octane IP 192 168 0 100 NIC IP Microscope PC IP Ethernet cable 2435...

Страница 21: ...l 5335 007 31700 SG 3 PCIe 5335 007 31400 Mains 24V Power Supply 2735 171 31074 Microscope Octane IP 192 168 0 100 NIC IP Microscope PC IP Ethernet cable 2435 072 44045R Sync cable 4035 008 10900 Ferr...

Страница 22: ...PCIe 2735 171 30939 IP 192 168 0 101 SYNC Panel 5335 007 31700 SG 3 PCIe 5335 007 31400 Mains 24V Power Supply 2735 171 31074 Microscope Octane IP 192 168 0 100 NIC IP Microscope PC IP Ethernet cable...

Страница 23: ...Basic System Cabling Octane Basic User Guide Page 23 of 25 This page is intentionally blank...

Страница 24: ...Basic System Cabling Octane Basic User Guide Page 24 of 25 This page is intentionally blank...

Страница 25: ...dware as shown below or display a message about DPP service failing to start Figure 10 TEAM Login RED Hardware Status In this case power off the detector using the switch on the small black power bric...

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