2. GZK Neutrino Spectrum

3. How the detection scheme words

5. Index of Refraction

6. Askaryan Pulse and Antenna Response

7. Some attenuation modeling

8. Besson-Gorham Attenuation---300 MHz

9. Bogorodsky Attenuation

10. Sade and Gorham Attenuation—Gorham (old) at 300 MHz

11. Sade Attenuation

12. Attenuation vs frequency and depth

13. Some Optics

14. 50 meter depth optics

15. 200 meter depth optics

16. A horizontal event at 1500 meter Cerenkov Radiation Pattern

17. Testbed---Surface listening post Frequency range 100-1000 MHz
Testbed---Surface listening post Frequency range MHz. Sensitivity to -114 dBm

19. Batwing/Discone Antennas

21. Optics in a conductive medium

24. Radio Wish List?
Pingers—Deployable--(air, water, ice interface) complicates optics.
Permanent dedicated antennas at various depths. Special boreholes to 1000 meters. (both items are perishable opportunities which vanish when the IceCube string deployments stop.
Ice Characteristics: Index, Absorption Lengths, with respect to temperature (depth), density, and frequency.
Testbed—surface and meters deep, test firn-drill technology

25. The End