Now boasting a 100% brighter screen, increased processing power, and faster graphics engine, the Tiger Touch II is the most specified Titan console.
The Avolites Tiger Touch II represents the perfect combination of power and portability. This third-generation console is packed with enough power for complex shows, yet small and light enough to fly in standard hold luggage. The console features SMPTE timecode support and a redesigned button layout to match the entire Titan range.
In order to update the console to version 12 of the Titan, it will be necessary to purchase and install a USB dongle called AVOKEY.
Serial 02006 - 03065
You need to order:
- AVOKEYINT
- 1x5 way to USB-A Cable (spare part code 8000-6102)
Once you've received your AVOKEYINT and 1x5 way to USB-A Cable, you will be required to connect the USB-A Cable to the motherboard. This cable will provide an additional USB port for the AvoKey.
Click here to view the installation guide: https://www.avolites.com/Portals/0/Downloads/Manuals/AvoKey/8000-6102 TT2-2-3K AVOKEY upgrade with 1808-0028.pdf
Serial 03066 - 4020
You need to order only AVOKEYINT
Once you've received your AVOKEYINT, you will be required to connect this directly to the available (Blue) USB port inside the console (on the motherboard).
Click here to view the installation guide: https://www.avolites.com/Portals/0/Downloads/Manuals/AvoKey/8000-6101 TT2 AVOKEY no cable.pdf
Serial 04021 - 05001
You need to order only AVOKEYINT
Once you've received your AVOKEYINT, you will be required to connect this directly to the available (Red) USB port inside the console (on the motherboard).
Serial 5001 and above include a factory fitted AvoKey.
Therefore, you do not need to purchase an AvoKey.
: Mathematical tools like partial differential equations and tensors are introduced only when required by the physical topic being discussed.
: Covers wave mechanics, vibrations, and a concluding section on the theory of relativity derived from first principles.
Many modern "Mathematical Methods" textbooks have ballooned to 1,200+ pages, filled with glossy diagrams and historical anecdotes that distract from the core mathematics. Menzel’s book, by contrast, is lean, dense, and direct. Doctoral students searching for a of a Green’s function often reject newer texts in favor of Menzel.
: Available on the Internet Archive and Open Library .
: Covers advanced dynamics, potential theory, and hydrodynamics. It introduces critical mathematical tools like vector analysis within this physical context. Waves and Vibrations
Before diving into the text, it is critical to understand the author. Donald Howard Menzel (1901–1976) was not merely a textbook writer; he was one of the most influential astrophysicists of his generation. A Harvard University professor and director of the Harvard College Observatory, Menzel made groundbreaking contributions to the study of solar physics, nebulae, and the chemistry of stars.
: Mathematical tools like partial differential equations and tensors are introduced only when required by the physical topic being discussed.
: Covers wave mechanics, vibrations, and a concluding section on the theory of relativity derived from first principles.
Many modern "Mathematical Methods" textbooks have ballooned to 1,200+ pages, filled with glossy diagrams and historical anecdotes that distract from the core mathematics. Menzel’s book, by contrast, is lean, dense, and direct. Doctoral students searching for a of a Green’s function often reject newer texts in favor of Menzel.
: Available on the Internet Archive and Open Library .
: Covers advanced dynamics, potential theory, and hydrodynamics. It introduces critical mathematical tools like vector analysis within this physical context. Waves and Vibrations
Before diving into the text, it is critical to understand the author. Donald Howard Menzel (1901–1976) was not merely a textbook writer; he was one of the most influential astrophysicists of his generation. A Harvard University professor and director of the Harvard College Observatory, Menzel made groundbreaking contributions to the study of solar physics, nebulae, and the chemistry of stars.
