and Bubbles |
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| Convenor: | Santimay Basu, AFB/NRL | Keith Groves, Hanscom AFB |
| Michael Kelley, Cornell University |
| Speakers: | |||
| 1:30 - 1:40 | NASA Report | Mary Mellott (NASA) | |
| 1:40 - 1:50 | Physics of ESF Structures | Michael Kelley (Cornell) | |
| 1:50 - 2:00 | Discussion on ESF Physics | ||
| 2:00 - 2:10 | ESF Dynamics & Compostion | Rod Heelis (UTD) | |
| 2:10 - 2:20 | Discussion on ESF Dynamics | ||
| 2:20 - 2:30 | 3D ESF Evolution | M. Keskinen (NRL) | |
| 2:30 - 2:40 | Evolution of Scintillation Structures | Keith Groves (AFRL) | |
| 2:40 - 2:50 | Discussion on ESF Structuring | ||
| 2:50 - 3:00 | Forecast of ESF Structuring | Santi Basu (AFRL) | |
| 3:00 - 3:10 | Discussion on Forecast Issues | ||
| 3:10 - 3:30 |
Discussion on Coordinated Observations with other satellites, Rockets, & Ground-Based Instruments | ||
C/NOFS (Communication and Navigation Outage Forecast System). is the first satellite that is dedicated to forecasting ionospheric irregularities and ionospheric scintillation. It will be launched in November 2003, in a 13 degrees inclination, 700 x 400 km orbit.
This session is to help define the science related to C/NOFS. Broadly speaking, the science objectives can be organized in three categories:
Several campaigns will be planned which will validate the forecasts, acquire the data to achieve the science goals, and test the theoretical models. The research will include international collaborations.
We solicit inputs on these broad topics, with particular emphasis on Equatorial Spread F, Scintillation, Satellite coordination/rockets/ campaigns.
Different themes will be presented. Each theme will be briefly introduced by a lead-person, followed by a general discussion on the topic.