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<p class=MsoNormal><b><font size=3 color=red face=Arial><span lang=EN-US
style='font-size:12.0pt;color:red;font-weight:bold'>12th International
Ionospheric Effects Symposium (IES2008)<o:p></o:p></span></font></b></p>
<p class=MsoNormal><b><font size=3 color=red face=Arial><span lang=EN-US
style='font-size:12.0pt;color:red;font-weight:bold'><o:p> </o:p></span></font></b></p>
<p class=MsoNormal><b><font size=3 color=red face=Arial><span lang=EN-US
style='font-size:12.0pt;color:red;font-weight:bold'>FIRST ANNOUNCEMENT &
CALL-FOR-PAPERS & POSTERS</span></font></b><b><font size=3><span
lang=EN-US style='font-size:12.0pt;font-weight:bold'><o:p></o:p></span></font></b></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>DESCRIPTION OF IES2008<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>IES2008 follows in the tradition of the eleven previous Ionospheric
Effects Symposia that have been held in the <st1:place w:st="on"><st1:City
w:st="on">Washington</st1:City> <st1:State w:st="on">DC</st1:State></st1:place>
area since 1975. Partial support for IES2008 is provided by the Office of Naval
Research (ONR), and the Air Force Office of Scientific Research (AFOSR). Other
government sponsors are being solicited. We are also happy to welcome
International URSI as a sponsor of the symposium. Other affiliated agencies
include: the Naval Research Laboratory (NRL), the Air Force Research Laboratory
(AFRL), the Space Environment Center (SEC) of NOAA; the Air Force Weather
Agency (AFWA), and the Federal Communications Commission (FCC). The symposium
is a three-day event covering an array of topics of importance to both military
and commercial telecommunication, navigation and surveillance systems. (See
http://www.ies2008.com for details.)<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>DATES & VENUE <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Dates: May 13-15, 2008 <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Venue: <st1:PlaceName w:st="on">Crowne</st1:PlaceName> <st1:PlaceType
w:st="on">Plaza</st1:PlaceType> <st1:PlaceName w:st="on">Old</st1:PlaceName> <st1:PlaceType
w:st="on">Town</st1:PlaceType>, <st1:City w:st="on">Alexandria</st1:City>, <st1:State
w:st="on"><st1:place w:st="on">Virginia</st1:place></st1:State> (formerly the
Radisson Hotel) <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Abstracts for POSTERS and ORAL Presentations are solicited:<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>http://www.ies2008.com<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>http://ies2008.com/abstract_form.htm<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>http://ies2008.com/registration_form.htm<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Point of Contact: John M. Goodman<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Phone: +1-703-360-7127 (<st1:place w:st="on"><st1:City w:st="on">Alexandria</st1:City>
<st1:State w:st="on">VA</st1:State></st1:place>)<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Cellular: +1-703-314-2006<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Phone/Fax: +1-910-846-2948 (<st1:place w:st="on"><st1:City w:st="on">Holden
Beach</st1:City> <st1:State w:st="on">NC</st1:State></st1:place>)<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Fax: +1-703-360-3954 (<st1:place w:st="on"><st1:City w:st="on">Alexandria</st1:City>
<st1:State w:st="on">VA</st1:State></st1:place>)<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>email: jm_good@cox.net, jmgood@starpower.net;
jmgood@jmg-associates-ltd.com; ies2008@jmg-associates-ltd.com<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Chairman: Dr. J. M. Goodman (RPSI; JMG Associates Ltd)<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Co-Chairmen: <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Dr. Robert McCoy (ONR) *<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Major David Byers (AFOSR) *<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Other Members of the Steering Committee: <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Dr. Dave Anderson (<st1:place w:st="on"><st1:PlaceType w:st="on">University</st1:PlaceType>
of <st1:PlaceName w:st="on">Colorado</st1:PlaceName></st1:place>) *<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Dr. Paul Bernhardt (Naval Research Laboratory) * <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Mr. Greg Bishop (Air Force Research Laboratory) *<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Mr. Deane Bunce (Federal Aviation Administration) <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Lt. Col. William B. "Trey" Cade (Air Force Weather Agency) <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Mr. Ray Conkright (NOAA-NGDC) <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Dr. <st1:PersonName w:st="on">Anthea Coster</st1:PersonName> (MIT
Haystack Observatory) *<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Dr. Ken Davies (NOAA-Retired) *<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Ms. <st1:PersonName w:st="on">Pat Doherty</st1:PersonName> (<st1:place
w:st="on"><st1:PlaceName w:st="on">Boston</st1:PlaceName> <st1:PlaceType w:st="on">College</st1:PlaceType></st1:place>)
*<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Dr. Tim Fuller-Rowell (NOAA-SEC) *<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Mr. Jack Klobuchar (Emeritus) <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Mr. Joe Kunches (NOAA-SEC) *<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Dr. Leo McNamara (Boston College/AFRL) *<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Prof. <st1:PersonName w:st="on">Bodo Reinisch</st1:PersonName> (<st1:place
w:st="on"><st1:PlaceType w:st="on">University</st1:PlaceType> of <st1:PlaceName
w:st="on">Massachusetts</st1:PlaceName></st1:place>) *<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Mr. James Secan (Northwest Research Associates) *<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Mr. Kevin Scro (CISF/Air Force)<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Dr. Haim Soicher (US Army Labs representative) *<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Mr. John Wang (Federal Communications Commission) *<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Dr. Paul Cannon (Qinetiq)- URSI Representative *<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>* verified acceptance<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>IES2008 TOPICS ACCEPTABLE <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Short Synopsis of Topics and Potential Special Sessions<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>1.Space-Weather and ionospheric effects on telecommunication systems <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>This particular topic will stress the direct relationships between
impairments upon telecommunication systems and space weather events or
phenomena. Telecommunication systems of interest include but are not limited to
the following: longwave communication and navigation systems; shortwave (HF)
communication and OTHR systems; HFDF systems; VHF communication systems; UHF
radar surveillance systems; UHF-SHF satellite communication systems; L-Band
satellite navigation systems (GPS, GLONASS, etc.); cellular systems. Propagation
phenomena and system impairments such as scintillation, phase fluctuations,
loss of phase-lock, angle-of-arrival errors, absorption effects, ranging
errors; radio blackout conditions, optimum working frequency fluctuations.
Actual data is emphasized when possible. <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>2.Current solar cycle phenomena and impact on operational systems <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>This topic should stress phenomena observed during the later stages of
the most recent solar cycle (#23) and the emergent solar cycle (#24).
Operational systems are to be emphasized. They could include, but are not
limited to the following: the GPS system and aviation applications such as
WAAS; HF-ALE systems; GLOBALink/HF; Trans-polar HF voice service for airlines;
Milsatcom; etc. <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>3.Modeling, forecasting, and prediction systems <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>This topic is dedicated to the elucidation of the myriad of modeling
efforts leading to the development of forecasting and prediction systems. These
efforts and the systems themselves may be directed to the
prediction./forecasting of space weather events (as an end-product) or the
prediction/forecasting of system impairments (where space-weather is an
intermediate product). It is presumed that the space weather events are
pertinent vis-a-vis system effects. Military systems such as SCINDA and C/NOFS
are of interest, and there are many examples climatological predictions systems
that may be subject to update. <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>4.Ionospheric sounder methods and measurements <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>This topic encompasses all types of sounder systems and related
measurement techniques, including legacy systems, advanced digital sounders,
single frequency beacons, and wideband probes, deployed either terrestrially
and aboard satellites. Of special interest are sounder techniques that can be
exploited to derive operationally relevant ionospheric information. Another
interest is the comparison of information derived from sounder systems and
independent measurement schemes such as: in-situ probes (rockets and
satellites), incoherent scatter techniques, etc. <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>5.Multi-Sensor contributions to the solution of Space-Weather effects
on ionospherically-dependent systems <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>This topic involve an examination of the ionosphere using multiple
sensors, such as the sensors suggested under the international DASI effort.
These sensors may include radio receivers and telescopes, ionosondes, radars,
TEC polarimeters, magnetometers, optimal instruments, solar imagers, and so on.
The multi-sensor approach enables corroborative measurements to be obtained,
and allows for a more general evaluation of the ionospheric personality during
periods of system disturbance, or inferred impairment events. <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>6.Applications of ionospheric tomography <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Ionospheric tomography is a relatively new imaging technique that
allows for evaluation of Ne gradients and large-scale structures. These are
important during disturbed geomagnetic periods. Of special interest are studies
that have been stimulated by the International Polar Year (IPY:2007-2008).<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>7.Transionospheric effects, including scintillation <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>This topic emphasizes the impact of the ionosphere on radiowaves
transmitted to/from satellites and even signals from radio stars. Of primary
interest are propagation effects such as Faraday rotation, phase and amplitude
scintillation, wedge refraction, ranging errors, group path delay fluctuations,
and miscellaneous phase path effects. Examples include scintillation introduced
on the GPS space segment, and scintillation impairments in connection with
communication systems, observed especially during geomagnetic storms,
emphasizing polar, auroral, and equatorial regions. <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>8.Ionospheric effects on WAAS and other systems supporting aviation <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>This topic is dedicated principally to ionospheric effects on radio
systems (i.e., navigation and communication) that support aviation. Satellite
communication and shortwave voice/data communication systems are of interest,
especially for flights passing through geophysical regions such as the polar
cap and the equator, that sometimes exhibit pathological behavior. <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>9.High Frequency communication and surveillance systems <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>This topic is principally dedicated to the ionospheric and
space-weather effects on high frequency (HF) communication and surveillance
systems (i.e., HFDF, HF-SSL, and OTHR). The communication systems include
legacy voice and data link (i.e., HFDL). <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>10.Longwave propagation systems and effects <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>This topic concerns the interaction of certain legacy systems used for
navigation and communication at frequencies belonw the shortwave (i.e., HF)
band. Many of these systems are still is use and are of importance in backup
scenarios. Other applications may be primary in nature<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>11.Global Positioning System and total electron content studies <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>This topic emphasizes the impact on the ionospheric electron content (i.e.,
TEC) upon navigation systems that operate using methodologies for which the
compensation is non-existent or incomplete. Examples include single-frequency
GPS receivers.<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>12.Impact of the lower atmosphere on the Ionosphere <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>It is well known that the lower atmosphere is a source of atmospheric
gravity waves, infrasonic waves and other oscillations that may introduce
ionospheric tracers to the underlying neutral gas motion. Ionospheric factors
include traveling ionospheric disturbances (TID) and other variations in the
electron density distribution. Lower atmospheric chemistry and dynamics are
also relevant subjects to consider under this general topic. An interesting
aspect is the impact of space weather and the ionospheric personality upon the
lower atmosphere. <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>13.Contribution of the IHY to the understanding of the ionosphere at
all longitudes <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>This topic will look to contributions by participants in studies
associated with the International Heliospheric Year. Collaborative investigations
and reports are of primary interest.<o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>14.Impact of global electrodynamics on the storm-time ionosphere <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>Knowledge of the storm-time ionosphere is of paramount interest to
system engineers as well as practicing ionosphericists. There have been a
number of theoretical models that may account for many aspects of the
storm-time ionospheric morphology, and many aspects of the behavior are now
understood. Still other aspects of the geomagnetic storm are not known, and
there are inconsistencies from one storm to the next. Empirical models have
provided a useful procedure for estimating the general behavior of ionospheric
storms. Global electrodynamics can provide a macroview of the important
phenomena, and along with empirical data for verification, may be the way
forward and lead to a more fulsome understanding. Studies of storm behavior
through the lens of global electrodynamics are solicited. <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>15.Results derived from COST-ACTION programs (viz., 238, 251, 271, 724,
and 296). <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>This topic pertains to COST Actions undertaken by the European
community and its affiliates having relevance to the ionosphere and space
weather effects upon telecommunication systems. These Actions, including 238,
251, 271, 724, and 296, are to be emphasized. A limited number of papers would
be devoted to programmatic aspects, but more substantive scientific and
engineering studies are requested. <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>16.Impact of solar noise bursts and environmental noise on
telecommunication and navigation systems <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>This topic recognizes that system performance typically depends upon
signal-to-noise (SNR) ratios, and that systematic, man-made, and environmental
noise are major factors in the determination of how well a radiowave system may
perform. Studies of man-made noise, galactic noise, atmospheric noise, and
cosmic noise bursts are welcome. Solar noise bursts have been shown to have a
significant impact upon the GPS system., and recent studies (circa 2006 and
following) have demonstrated measurable impacts upon navigation systems dependent
upon the GPS waveform. Further examination of these effects would be of
interest. <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>17.Space-Weather program activities having relevance to ionospheric
effects on C3I and navigation systems <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>18.Products and services offered by industry relevant to prediction
& forecasting of ionospheric effects <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>19.Government projects associated with the forecasting and/or
mitigation of deleterious effects on national and/or military systems <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'>20.Studies of documented system impacts during major geomagnetic storms
and other solar-generated events <o:p></o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=3 face=Arial><span lang=EN-US style='font-size:
12.0pt'><o:p> </o:p></span></font></p>
<p class=MsoNormal><font size=2 color=red face=Arial><span lang=EN-US
style='font-size:11.0pt;color:red'>_________________________________________________</span></font><span
lang=EN-US><o:p></o:p></span></p>
<p class=MsoNormal><em><i><font size=2 face=Arial><span lang=EN-US
style='font-size:10.0pt;font-family:Arial'>Prof <st1:PersonName w:st="on">Paul
S Cannon</st1:PersonName>, FREng, PhD</span></font></i></em><span lang=EN-US><o:p></o:p></span></p>
<p class=MsoNormal><font size=2 face=Arial><span lang=EN-US style='font-size:
11.0pt'> <o:p></o:p></span></font></p>
<p class=MsoNormal><em><i><font size=2 face=Arial><span lang=EN-US
style='font-size:10.0pt;font-family:Arial'>Chief Scientist Communications
Division</span></font></i></em><span lang=EN-US><o:p></o:p></span></p>
<p class=MsoNormal><em><i><font size=2 face=Arial><span lang=EN-US
style='font-size:10.0pt;font-family:Arial'>Chair Commission G, International <st1:place
w:st="on">Union</st1:place> of Radio Science (URSI)</span></font></i></em><span
lang=EN-US><o:p></o:p></span></p>
<p class=MsoNormal><font size=2 face=Arial><span lang=EN-US style='font-size:
11.0pt'> <o:p></o:p></span></font></p>
<p class=MsoNormal><em><i><font size=2 face=Arial><span lang=EN-US
style='font-size:10.0pt;font-family:Arial'>Centre for RF Propagation and
Atmospheric Research</span></font></i></em><span lang=EN-US><o:p></o:p></span></p>
<p class=MsoNormal><em><i><font size=2 face=Arial><span lang=EN-US
style='font-size:10.0pt;font-family:Arial'>QinetiQ, <st1:place w:st="on"><st1:City
w:st="on">Malvern</st1:City>, <st1:PostalCode w:st="on">WR14 3PS</st1:PostalCode>,
<st1:country-region w:st="on">UK</st1:country-region></st1:place></span></font></i></em><span
lang=EN-US><o:p></o:p></span></p>
<p class=MsoNormal><em><i><font size=2 face=Arial><span lang=EN-US
style='font-size:10.0pt;font-family:Arial'>Tel: +44 (0) 1684-896468, Fax: +44
(0) 1684-895646</span></font></i></em><span lang=EN-US><o:p></o:p></span></p>
<p class=MsoNormal><em><i><font size=2 face=Arial><span lang=EN-US
style='font-size:10.0pt;font-family:Arial'>QinetiQ Mobile: +44 (0)7990-564772</span></font></i></em><span
lang=EN-US><o:p></o:p></span></p>
<p class=MsoNormal><em><i><font size=2 face=Arial><span lang=EN-US
style='font-size:10.0pt;font-family:Arial'>email: </span></font></i></em><span
lang=EN-US><a href="mailto:pcannon@qinetiq.com"><em><i><font size=2 face=Arial><span
style='font-size:10.0pt;font-family:Arial'>pcannon@qinetiq.com</span></font></i></em></a><o:p></o:p></span></p>
<p class=MsoNormal><em><i><font size=2 face=Arial><span lang=EN-US
style='font-size:10.0pt;font-family:Arial'>Centre web site: </span></font></i></em><span
lang=EN-US><a href="http://www.cpar.qinetiq.com"><em><i><font size=2
face=Arial><span style='font-size:10.0pt;font-family:Arial'>http://www.cpar.qinetiq.com</span></font></i></em></a><o:p></o:p></span></p>
<p class=MsoNormal><font size=2 face=Arial><span lang=EN-US style='font-size:
11.0pt'> <o:p></o:p></span></font></p>
<p class=MsoNormal><em><i><font size=2 face=Arial><span lang=EN-US
style='font-size:10.0pt;font-family:Arial'>email at <st1:place w:st="on"><st1:PlaceName
w:st="on">Bath</st1:PlaceName> <st1:PlaceType w:st="on">University</st1:PlaceType></st1:place>:
</span></font></i></em><span lang=EN-US><a href="mailto:p.s.cannon@bath.ac.uk"><em><i><font
size=2 face=Arial><span style='font-size:10.0pt;font-family:Arial'>p.s.cannon@bath.ac.uk</span></font></i></em></a><o:p></o:p></span></p>
<p class=MsoNormal><font size=2 color=red face=Arial><span lang=EN-US
style='font-size:11.0pt;color:red'>________________________________________________</span></font><span
lang=EN-US><o:p></o:p></span></p>
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11.0pt'> </span><span lang=EN-US><o:p></o:p></span></font></p>
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