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SL McGregor, WJ Hughes, CN Arge… - Journal of Geophysical …, 2011 - agu.org
It took the solar polar passage of Ulysses in the early 1990s to establish the global structure of
the solar wind speed during solar minimum. However, it remains unclear if the solar wind is composed
of two distinct populations of solar wind from different sources (eg, closed loops which ...
Cited by 1 - Related articles - All 4 versions
[PDF] from agu.orgSL McGregor, WJ Hughes, CN Arge… - Journal of Geophysical …, 2011 - agu.org
Received 10 August 2010; revised 30 November 2010; accepted 13 January 2011; published
31 March 2011. [1] The WSA‐ENLIL model predicts significant evolution of the solar wind
speed. Along a flux tube the solar wind speed at 1.0 AU and beyond is found to be ...
Related articles - View as HTML - All 3 versions
[PDF] from ihy2007.org…, JG Luhmann, JT Hoeksema, X Sun, CN Arge… - Solar Physics, 2011 - Springer
Abstract The solar cycle 23 minimum period has been characterized by a weaker solar and
interplanetary magnetic field. This provides an ideal time to study how the strength of the
photospheric field affects the interplanetary magnetic flux and, in particular, how much the ...
Cited by 1 - Related articles - All 6 versions
JE Moeslund, L Arge, PK Bøcher, B Nygaard… - Wetlands, 2011 - Springer
Abstract Salt meadows are thought to be vulnerable to habitat loss under future sea-level
rise (SLR) due to inundation and compression of coastal environments (coastal squeezing).
The extent of this threat is poorly understood due to the lack of geographically ...
Related articles - All 3 versions
C Lee, CN Arge, JM Quinn… - AAS/Solar Physics …, 2011 - adsabs.harvard.edu
As we progress toward the maximum period of Solar Cycle 24, we have a unique opportunity
to better understand the propagation and evolution of a CME given the multiple vantage points
near 1 AU of such an event. In addition, with the wide availability of sophisticated, physics- ...
SL McGregor, WJ Hughes, CN Arge… - Journal of Geophysical …, 2011 - agu.org
It took the solar polar passage of Ulysses in the early 1990s to establish the global structure of
the solar wind speed during solar minimum. However, it remains unclear if the solar wind is composed
of two distinct populations of solar wind from different sources (eg, closed loops which ...
Cited by 1 - Related articles - All 4 versions
[PDF] from agu.orgSL McGregor, WJ Hughes, CN Arge… - Journal of Geophysical …, 2011 - agu.org
Received 10 August 2010; revised 30 November 2010; accepted 13 January 2011; published
31 March 2011. [1] The WSA‐ENLIL model predicts significant evolution of the solar wind
speed. Along a flux tube the solar wind speed at 1.0 AU and beyond is found to be ...
Related articles - View as HTML - All 3 versions
[PDF] from ihy2007.org…, JG Luhmann, JT Hoeksema, X Sun, CN Arge… - Solar Physics, 2011 - Springer
Abstract The solar cycle 23 minimum period has been characterized by a weaker solar and
interplanetary magnetic field. This provides an ideal time to study how the strength of the
photospheric field affects the interplanetary magnetic flux and, in particular, how much the ...
Cited by 1 - Related articles - All 6 versions
JE Moeslund, L Arge, PK Bøcher, B Nygaard… - Wetlands, 2011 - Springer
Abstract Salt meadows are thought to be vulnerable to habitat loss under future sea-level
rise (SLR) due to inundation and compression of coastal environments (coastal squeezing).
The extent of this threat is poorly understood due to the lack of geographically ...
Related articles - All 3 versions
C Lee, CN Arge, JM Quinn… - AAS/Solar Physics …, 2011 - adsabs.harvard.edu
As we progress toward the maximum period of Solar Cycle 24, we have a unique opportunity
to better understand the propagation and evolution of a CME given the multiple vantage points
near 1 AU of such an event. In addition, with the wide availability of sophisticated, physics- ...
M Delgado-Ortega, S Melo… - Veterinary Immunology and …, 2011 - Elsevier
... genes Thymus HPRT 1 RPL 1 9 B 2 MITBP 1 HMBS 2 ACTBGAPDHSDHA 0.0 0.5 1.0 1.5 Kidney
A ct BTBP - 1 GAPDHSDHAB 2 MIRPL - 1 9 HPRT - 1 HMBS 0.0 0.5 1.0 1.5 M valu eFigure Page
15 of 15 Ac ce pte d M an usc rip t Figure 2 SOCS1 K idney L arge I ntestine L iver ...
[PDF] from pharmscidirect.comNGR Rao, MA Hadi… - Int J Pharm, 2011 - pharmscidirect.com
... All rights reserved. Page 2. do ta ha di fo sy do ca in re lo de to as re em so si su m pa m po sy
po in re osage forms ablets. MUDF ard capsules isintegration, orms (Fig.1) [ Multi-partic ystems
have s osage forms. A apsule in the ntestine [7] a esulting in a ocal irritation. ...
Related articles - View as HTML - All 2 versions
JU Kunstler, R Bergmann, E Gniazdowska… - Journal of Inorganic …, 2011 - Elsevier
... 3 en)(L2-BN st )] [Re(NS 3 crown)(L2-BN st )] [Re(NS 3 (COOH) 3 )(L2-BN st )] AC CE PT ED
M AN US CR IPT ACCEPTED MANUSCRIPT 25 P ancreas 5 m in 6 0 m in S tomach 5 m in 6
0 m in K idneys 5 m in 6 0 m in L iver 5 m in 6 0 m in U rine 5 m in 6 0 m in I ntestine 5 m in ...
G Musso - Annual Review of Medicine, 2011 - annualreviews.org
S Urabe, T Somamoto, S Sameshima… - Fish & Shellfish …, 2011 - Elsevier
... Rainbow trout -2 (L63539) FS998333 FS999016 FS999328 FS998558 FS998955 Fig.2(B) MA
NUSCRIPTACCEPTED ACCEPTED MANUSCRIPT CaauUF-S3n CaauZB-S3n CaauZE-S3n
B rain G ill H eart T hymus L iver H ead K idney T runk K idney S pleen I ntestine M uscle ...
All 2 versions
…, K Gilmore, E Grace, M Hannel… - American …, 2011 - adsabs.harvard.edu
We present an extragalactic source catalog, which includes galaxies and Active Galactic
Nuclei, that is used for the Large Survey Synoptic Telescope Imaging Simulation effort. The galaxies
are taken from the De Lucia et. al. (2006) semi-analytic modeling (SAM) of the Millennium ...
…, E Grace, K Gilmore, M Hannel… - American …, 2011 - adsabs.harvard.edu
We use the LSST image simulator to generate realistic 10-year datasets for 100 of the strong
galaxy-scale gravitational lenses expected to be measurable with the universal survey data.
The 200 mock i-band images have sky brightness and atmospheric seeing drawn from ...
[PDF] from lsst.org…, RR Gibson, K Gilmore, E Grace, M Hannel… - American Astronomical …, 2011 - lsst.org
The Large Synoptic Survey Telescope (LSST) is a large-aperture, wide-field, ground-based telescope
designed to provide a complete survey of 20,000 square degrees of sky in six optical bands every
few nights. Over ten years of operation, it will measure the magnitudes, colors,
View as HTML - All 2 versions
…, K Gilmore, E Grace, M Hannel… - American …, 2011 - adsabs.harvard.edu
The Image Simulation team for the Large Synoptic Survey Telescope (LSST) will show a series
of sample images for a portion of the full field of view at a resolution of one LSST pixel (0.2 arc
second) matching one pixel of a large 6000 x 6000 pixel display that is 7 x 7 feet in size. ...
…, K Gilmore, E Grace, M Hannel… - American …, 2011 - adsabs.harvard.edu
Efficient use of the data produced by the Large Synoptic Survey Telescope (LSST) will require
comprehensive a priori knowledge of the impact of telescope design and implementation on
the resulting catalogs and images. This includes gross characteristics like per band ...

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