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 ...
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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