LWS CDAW-2005 Participant List

Name
Affiliation
E-Mail
WG
Areas_Interested
Submission
Akiyama, Sachiko
CUA
akiyama@solar.isas.jaxa.jp
WG1
Geo-effective CMEs
Submission
Berdichevsky, Daniel B
L3 GS Inc.
xrdbb@lepvax.gsfc.nasa.gov
WG1
The source and heliospheric manifestations (ICMEs) of CMEs.
Submission
Biesecker, Douglas A
NOAA/SEC
doug.biesecker@noaa.gov
WG1
photospheric to low corona diagnostics of geo-effective CME's
Submission
Bothmer, Volker
University Göttingen
bothmer@astro.physik.uni-goettingen.de
WG1
Solar Sources, CME onsets, evolution, forecast
Submission
Cliver, Edward W
AFRL
edward.cliver@hanscom.af.mil
WG1
Origins/signatures of geoeffective CMEs and M-regions.
Submission
Georgoulis, Manolis K
JHU/APL
manolis.georgoulis@jhuapl.edu
WG1
(1) Source properties of geo-effective CMEs
(2) CME prediction by means of vector magnetogram analysis
(3) Magnetic helicity in the solar atmosphere

Submission
Gopalswamy, Nat
NASA GSFC
gopals@fugee.gsfc.nasa.gov
WG1
properties of geo-effective CMEs
Submission
Howard, Russell A
Naval Research Lab
russ.howard@nrl.navy.mil
WG1
Properties of geo-effective CMEs

Submission
Huttunen, Emilia
University of Helsinki
Emilia.Huttunen@helsinki.fi
WG1
ICMEs and sheath regions of ICMEs
primary characteristics that make a CME geoeffective
(southward Bz, high dynamic pressure)
Submission
Kasper, Justin C
MIT Center for Space Research
jck@mit.edu
WG1
Interplanetary shocks, geo-effective events

Submission
Kataoka , Ryuho
National Institute of Information and Communications Technology
ryuho@nict.go.jp
WG1
Microstructures of geoeffective CMEs

Submission
Lara, Alejandro
Instituto de Geofisica, UNAM
alara@geofisica.unam.mx
WG1
Halo CMEs properties and ICME travel time
Submission
LOHANI, NAVAL KISHOR
M.B.Govt.P.G.College
lohani@iucaa.ernet.in
WG1
Solar Coronal loops and Their Heating Mechanism
Submission
MacDowall, Robert J
NASA GSFC
robert.macdowall@nasa.gov
WG1
What are the combinations of components in the solar wind that can lead to a geomagnetic storm?
What are the latest prediction methods?
Submission
Marque, Christophe
USRA-Naval Research Lab.
christophe.marque@nrl.navy.mil
WG1
Radio and coronal signatures of CMEs.
Submission
moran, thomas
CUA and NASA/GSFC
moran@orpheus.nascom.nasa.gov
WG1
properties of geo-effective CMEs
Submission
Morrill, Jeff S
Naval Research Laboratory
morrill@shogun.nrl.navy.mil
WG1
CME Properties
CME initiation

Submission
Nindos, Alexander
University of Ioannina
anindos@cc.uoi.gr
WG1
Solar conditions that lead to geoeffective CMEs
Submission
Nitta, Nariaki
Lockheed Martin Advanced Technology Center
nitta@lmsal.com
WG1
- Identification of solar sources of ICMEs, especially geo-effective ones as taken up in the workshop, using both solar and in-situ data.
- Understanding the origin of Bz<0 in and around ICMEs.
- Understanding the capabilities and limitations of magnetic field modelling (both at the Sun and ICME).
Submission
Nunes, Steven M
CUA
snunes@antique.gsfc.nasa.gov
WG1
Type II radio bursts
Blast wave and CME-driven shocks
Submission
olmedo, oscar a
George Mason University
oolmedo@gmu.edu
WG1
GMU graduate student
Submission
Poomvises, Watanachak
George Mason University
wpoomvis@gmu.edu
WG1
GMU student interested in solar sources of geomagnetic storms
Submission
Richardson, Ian G
Goddard Space Flight Center/UMd
richardson@lheavx.gsfc.nasa.gov
WG1
Solar wind plasma, magnetic fields, composition, and structures, solar sources.
Submission
Spicer, Daniel S
NASA/GSFC
daniel.s.spicer@nasa.gov
WG1
properties of geo-effective CMEs
Submission
Steinberg, John T
Los Alamos National Laboratory
jsteinberg@lanl.gov
WG1
properties of geo-effective CMEs
Submission
Thompson, Barbara J
NASA GSFC
barbara.j.thompson@nasa.gov
WG1
magnetic sources and structure of CMEs in inner corona
Submission
Vourlidas, Angelos
Naval Research Laboratory
vourlidas@nrl.navy.mil
WG1
CME Propagation, Radio CMEs, sources of CMEs, CME interaction w/ ionosphere
Submission
Webb, David
Boston College/AFRL Center for Excellence in SWx
david.webb@hanscom.af.mil
WG1
Solar and IP conditions that lead to geoeffective CMEs
Expertise: CMEs, halo CMEs, SMEI IP data
Submission
Wu, Chin-Chun
CSPAR/University of Alabama in Huntsville
wuc@cspar.uah.edu
WG1
Data analysis on the heliosphere physics, e.g., magnetic clouds, shock wave, CME
Submission
Xie, Hong
The Catholic University of America
hong@lepvax.gsfc.nasa.gov
WG1
Properties of geo-effective CMEs, complex interplanetary ejacta driver, interplanetary shock, corotating interaction region, and associated complex IMF structures.
Submission
YASHIRO, Seiji
CUA
yashiro@cdaw.gsfc.nasa.gov
WG1
test
Submission
Yurchyshyn, Vasyl
Big Bear Solar Observatory
vayur@bbso.njit.edu
WG1
solar sources and properties of geo-effective CME
Submission
Zhang, Jie
GMU
jiez@scs.gmu.edu
WG1
Properties of geo-effective CMEs and their solar surface source region

Prediction of major geomagnetic storms
Submission
Zhukov, Andrei N
Royal Observatory of Belgium
Andrei.Zhukov@oma.be
WG1
Source regions of geo-effective CMEs solar and interplanetary sources of geomagnetic storms prediction of geomagnetic storms.
Submission

Number of People: 34, Mail to All