Millimeter Continuum Observations of Stars - Pallavicini, White(Correct)
which differ drastically in their physical properties. They include: O -B stars with fluxes at
extended to be spatially resolved in some cases with the presently available instrumentation (see
emission, an active component associated withmagnetic active regions which is due mostly to thermal www.astro.umd.edu/~white/papers/96_pallavic.ps
THE ASTROPHYSICAL JOURNAL, 556 958969, 2001 August 1 V - The American Astronomical(Correct)
The disk extends to 200 AU in radius. 4.2. Dust Properties The models are run at wavelengths
observations of the reection nebulosity associated with the T Tauri star HH 30. The images show the
& Hillenbrand 1995 Choi &Herbst 1996)withmagnetic accretion models naturally providing these hot nicmosis.as.arizona.edu:8000/PUBLICATIONS/HH30_APJ.pdf
Measurements Of Solar Magnetic Element Motion From.. - Berger, Löfdahl.. (1998)(Correct)
1997 October 7 ABSTRACT Solar photospheric oweld properties on scales are measured using local correlation
(MBPs :photospheric bright points associated withmagnetic elements)The dataset is a 70 minute
Printed In U.s.a. Measurements Of Solar Magnetic Element Motion From High-Resolution Filtergrams www.astro.su.se/~mats/publications/offprints/36269.pdf
Physica A30 (205; 381 -- 394 - Www Elsevier Com(Correct)
con#guration, and study the ground-state properties. The satis#ability of the 3-SAT problem is
is known to solve large SAT instances. Even with the best available algorithms, the time of
Spin glasses are materials weakly diluted withmagnetic ions. The random positions of the ions induce www.lpt.ens.fr/~monasson/Articles/a39.pdf.gz
TELEMEDICINE JOURNAL AND e-HEALTH - Volume Number Mary (2002)(Correct)
the needs of the medical profession and patients without compromising quality of service? What are the
Angiogram 256 kilobytes (KB) image size) Magnetic resonance image 384 KB (image size) Scanned
microscopic image transfers, concurrent withmagnetic resonance imaging (MRI) images, live video and lhncbc.nlm.nih.gov:80/lhc/docs/published/2002/pub2002049.pdf
Optical Data Storage - Coufal, Burr (2002)(Correct)
high laser power must locally modify the optical properties of the recording medium to provide a
but this soon reached its practical limit. With a mechanical stylus, increasing the areal storage sunoptics.caltech.edu/~goffbo/papers/ITOchap.pdf
A Measurement of the Transverse Polarization of - Hyperons Produced In(Correct)
91-38, Protvino, 1991 17. Review of Particle Properties, Phys. Rev. D 54, 1 1996 18. K. Heller et al.
Proton Beam From The Cern Sps Has Been Performed With The Na48 Detector. The #Hyperons Were Detected At
followed by a 7.5 Tm dipole sweeping magnet (withmagnetic field directed horizontally and perpendicular to www.cern.ch/NA48/Welcome/papers/LambdaPolarisation/paper.pdf
A Reconfigurable FPGA-Based Readback Signal Generator For.. - Jinghuan Chen Jaekyun (2002)(Correct)
generator may be required to change the noise properties during runtime. Furthermore, di#erent kinds of
For example, a simulation of BER=10 -8 with 10 errors that runs on a personal computer
of one or more metal or glass disks coated withmagnetic thin films. Binary information is stored in www.sigda.org/Archives/ProceedingArchives/Dac/Dac2002/papers/2002/dac02/htmfiles/sun_sgi/../../pdffiles/24_3.pdf
Particle tracing in the magnetotail: Dependence on global.. - Streed, Cattell, Roth (2000)(Correct)
W.G. Paschmann, and C. Cattell, Average plasma properties in the central plasma sheet, J. Geophys. Res.
models, to compare and contrast the various models with each other, with satellite data and with other
jgr Particle tracing in the magnetotail: global magnetic field model Dependence on T. Streed, i C. www.msi.umn.edu/general/Reports/rptfiles/UMSI2000-179/UMSI_2000-179.ps.Z
Photospheric Magnetic Field Changes Associated with.. - Chae, Wang, Lee.. (1998)(Correct)
Photospheric Magnetic Field Changes Associated With Transition Region Explosive Events Jongchul Chae,
Version On January 14, 1998 Photospheric Magnetic Field Changes Associated With Transition Region
events rarely occur in the interior of strong magnetic flux concentrations, but rather are www.bbso.njit.edu/Preprints/PostScript/cha98b.ps.gz
Lithium Lenses For Muon Colliders - Gregory Silvestrov (1996)(Correct)
mechanical firmness will be provided by inertial properties of system and so the field up to 20T seems to
and operational regimes for existing lenses with solid lithium it is shown that the most
rate of operation about 0.5 Hz. By that withmagnetic field at cylindrical surface being of the order ftp.mumu.bnl.gov/pub/documents/greg.ps
Stability of Matter in Magnetic Fields - Lieb, Loss, Solovej (1995)(Correct)(5 citations)
One of the remaining unsolved problems connected with the stability of matter is the inclusion of
Stability of Matter in Magnetic Fields Elliott H. Lieb 12 Michael Loss 3
11 Abstract In the presence of arbitrarily large magnetic fields, matter composed of electrons and nuclei linux46.ma.utexas.edu/mp_arc/c/95/95-262.ps.gz
Proceedings ofIns288 of Mathematics of NAS of Ukraine 2000.. - Ruslan Go Vnia(Correct)
Part 2, 489-492. On A Class Ofeq153 For Particles With Arbitrary Spin Ruslan M.go Vnia Institute Of
for particles interacting with a consN0 t magneticfields prop ospf 1 Introduction Let us cons#U
4 Eq63 for particle interacting with constant magnetic field Cons]f the generalized equation (13) www.imath.kiev.ua/~symmetry/Symmetry99/art68.pdf
High-Resolution Line Scan Diffusion Tensor MR.. - Mamata, Mamata.. (2002)(Correct)
MR diffusion tensor imaging permits detailed visualization of white matter fiber tracts. This technique,
covering the entire brain volume were obtained with line scan diffusion imaging in six healthy
and Exhibition of the International Society for Magnetic Resonance in Medicine, 2000, Denver, CO. Address splweb.bwh.harvard.edu:8000/pages/ppl/westin/papers/mamataAJNR2002.pdf
Flux Pinning and Forced Vortex Entanglement by Splayed Columnar .. - Terence Hwa(Correct)
as a strategy to enhance transport properties in a field compared to parallel columns. The
physics is identical to that of the Bose glass [3]with flux lines strongly localized on the columnar
r i (z) as they traverse a sample withmagnetic field aligned with ck z: F =Z L 0 dz N X matisse.ucsd.edu/~hwa/papers/splay.ps
Accretion onto Magnetic White Dwarfs - Cropper(Correct)
of accreting systems of a galactic scale, with the advantage that in these systems the accreting
Accretion onto Magnetic White Dwarfs Mark Cropper Mullard Space Science
Recent developments in the accretion onto magnetic white dwarfs are reviewed. Accreting magnetic www.mssl.ucl.ac.uk/www_astro/preprints/msc/review_rev3.ps.gz
IL NUOVO CIMENTO Vol. ?, N. ? ? Solar Convection and.. - Robert Stein David(Correct)
surface. We begin with a summary of three basic properties of stratified convection. Next, we discuss our
DK Summary. Magneto-convection simulations with two scenarios have been performed: In one,
scenarios have been performed: In one, horizontal magnetic field is advected into the computational domain www.pa.msu.edu/~steinr/papers/themis.ps.gz