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Oxford Instruments Jupiter Discovery AFM
Asylum Research large-sample AFM: <25 pm noise floor, 5–20× faster scans, granite bridge and LVDT sensors — atomic resolution with a workflow a new user can finish in minutes.
Key specifications
- Noise floor
- <25 pm on a large-sample AFM
- Scan rate
- 5–20× faster than other large-sample AFMs
- Stage
- Ultra-rigid granite bridge; ultra-low-noise LVDT sensors
- Ease of use
- Pre-mounted probes, side-view camera, FFM Autopilot
- Configured to your application by our specialists
- Installed and commissioned on site
- Training and after-sales support across Jordan, the GCC and MENA
Oxford Instruments Jupiter Discovery AFM
Request a quoteOverview
Product overview
Jupiter Discovery is Asylum Research’s large-sample atomic force microscope: a granite bridge and ultra-low-noise LVDT sensors specified for a noise floor below 25 pm and scan rates 5–20× faster than other large-sample AFMs. Pre-mounted probes, a side-view camera, and FFM Topography with Autopilot take a new user from load to an image without a week of cantilever folklore. Core modes cover contact, tapping, force mapping, KPFM, MFM, PFM, and lithography; options add conductive AFM (ORCA), SCM, AM-FM viscoelastic mapping, blueDrive, liquid, CoolerHeater, and ±150 V nanoTDDB.
Al-Shaker specifies Jupiter Discovery versus a smaller-sample Asylum frame, which electrical and environmental options the proposal actually needs, and whether blueDrive belongs in the first cabinet — then installs, trains, and supports the AFM. Probes, holders, and heaters are supplied as consumables and accessories.
Specifications
Technical specifications
4 parameters
- Noise floor
- <25 pm on a large-sample AFM
- Scan rate
- 5–20× faster than other large-sample AFMs
- Stage
- Ultra-rigid granite bridge; ultra-low-noise LVDT sensors
- Ease of use
- Pre-mounted probes, side-view camera, FFM Autopilot
Features
Key features
- 01
Noise floor under 25 pm
Granite bridge and LVDT sensors specified for molecular and atomic resolution on a large sample.
- 02
Faster than the large-sample class
Electronic and mechanical bandwidth for scans 5–20× quicker than the AFMs this stage size usually implies.
- 03
Autopilot for the first image
Pre-mounted probes and a side-view camera so a core-facility user is not a two-day course.
From order to operation
We stay with the instrument after it arrives
Al-Shaker specifies the configuration, documents the system, and supports it across Jordan, the GCC, and MENA.
- 01
Consult
- 02
Plan
- 03
Supply
- 04
Install
- 05
Train
- 06
Support
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Talk to the technical team
Tell us the application. We will specify the system.
Share the workflow, capacity, and compliance constraints. We respond with a recommended configuration, not a generic catalogue list.