NASA Scientific and Technical Aerospace Reports
NASA Scientific and Technical Aerospace Reports
NASA Scientific and Technical Aerospace Reports
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the scientific questions of the roles of fluvial <strong>and</strong>, especially, glacial erosion in the evolution of relief in mountainous regions<br />
using available digital elevation models (DEMs) for the Southern Alps of New Zeal<strong>and</strong> (available at both 25m <strong>and</strong> 50m pixel<br />
sizes), <strong>and</strong> USGS 10m <strong>and</strong> 30m DEMs within the Western US. As emphasized in the original proposal, we chose the emphasis<br />
on the role of glacial modification of topographic relief because there has been little quantitative investigation of glacial<br />
erosion processes at l<strong>and</strong>scape scale. This is particularly surprising considering the dramatic sculpting of most mid- <strong>and</strong><br />
high-latitude mountain ranges, the prodigious quantities of glacially-derived sediment in terrestrial <strong>and</strong> marine basins, <strong>and</strong> the<br />
current cross-disciplinary interest in the role of denudational processes in orogenesis <strong>and</strong> the evolution of topography in<br />
general. Moreover, the evolution of glaciated l<strong>and</strong>scapes is not only a fundamental problem in geomorphology in its own right,<br />
but also is at the heart of the debate over Late Cenozoic linkages between climate <strong>and</strong> tectonics.<br />
Derived from text<br />
Glaciers; Erosion; Topography; Tectonics; Geomorphology; Geological Surveys<br />
20040070915 Boston Univ., Boston, MA, USA<br />
Deriving Albedo from Coupled MERIS <strong>and</strong> MODIS Surface Products<br />
Gao, Feng; Schaaf, Crystal; Jin, Yu-Fang; Lucht, Wolfgang; Strahler, Alan; [2004]; 17 pp.; In English; MERIS Users<br />
Workshop, 10-14 Nov. 2004, Frascati, Italy; Original contains black <strong>and</strong> white illustrations<br />
Contract(s)/Grant(s): NAG5-11263; No Copyright; Avail: CASI; A03, Hardcopy<br />
MERIS Level 2 surface reflectance products are now available to the scientific community. This paper demonstrates the<br />
production of MERIS-derived surface albedo <strong>and</strong> Nadir Bidirectional Reflectance Distribution Function (BRDF) adjusted<br />
reflectances by coupling the MERIS data with MODIS BRDF products. Initial efforts rely on the specification of surface<br />
anisotropy as provided by the global MODIS BRDF product for a first guess of the shape of the BRDF <strong>and</strong> then make use<br />
all of the coincidently available, partially atmospherically corrected, cloud cleared, MERIS observations to generate<br />
MERIS-derived BRDF <strong>and</strong> surface albedo quantities for each location. Comparisons between MODIS (aerosol-corrected) <strong>and</strong><br />
MERIS (not-yet aerosol-corrected) surface values from April <strong>and</strong> May 2003 are also presented for case studies in Spain <strong>and</strong><br />
California as well as preliminary comparisons with field data from the Devil’s Rock Surfrad/BSRN site.<br />
Author<br />
Spectral Reflectance; MODIS (Radiometry); Bidirectional Reflectance; Aerosols; Albedo; Distribution Functions<br />
20040070920 <strong>NASA</strong> Goddard Space Flight Center, Greenbelt, MD, USA<br />
Stormtime Particle Energization with High Temporal Resolution AMIE Potentials<br />
Khazanov, George V.; Liemohn, Michael W.; Fok, Mei-Ching; Newman, Timothy S.; Ridley, Aaron J.; [2004]; 2 pp.; In<br />
English; No Copyright; Avail: Other Sources; Abstract Only<br />
Simulations were conducted to investigate the influence of rapid electric field fluctuations on electron energization in the<br />
inner magnetosphere based on the assimilative mapping of ionospheric electrodynamics (AMIE) technique. Simulations for<br />
four different magnetic storms were run, namely those that occurred on May 15, 1997, May 4, 1998, September 25, 1998, <strong>and</strong><br />
October 19, 1998. Here, we have examined the formation of high energy (10-1000 keV) electrons in the inner magnetosphere<br />
during these storm events with our recently-developed relativistic radiation belt transport code. The point of this numerical<br />
experiment is to show that a simulation of a real event must have the high time resolution electric field input files in order<br />
to produce the seed population for the radiation belts, which are often observed to increase in the days following a magnetic<br />
storm. Specifically, a cadence of the global electric field pattern of 5 minutes or less produces inner magnetospheric fluxes that<br />
are larger (by up to several orders of magnitude) than fluxes produced with a longer cadence. Differences were particularly<br />
large relative to simulation results with a 3-hour time cadence, analogous to a Kp-driven electric field model.<br />
Author<br />
Temporal Resolution; Computerized Simulation; Magnetic Storms; Electrodynamics; Ionospheres; Thematic Mapping<br />
20040070944 <strong>NASA</strong> Goddard Space Flight Center, Greenbelt, MD, USA<br />
Accuracy <strong>and</strong> Precision in the Southern Hemisphere Additional Ozonesondes (SHADOZ) Dataset 1998-2000 in Light<br />
of the JOSIE-2000 Results<br />
Witte, J. C.; Thompson, A. M.; Schmidlin, F. J.; Oltmans, S. J.; McPeters, R. D.; Smit, H. G. J.; 2003; 1 pp.; In English; Fall<br />
AGU Meeting 2003, 8-12 Dec. 2003, San Francisco, CA, USA; No Copyright; Avail: Other Sources; Abstract Only<br />
A network of 12 southern hemisphere tropical <strong>and</strong> subtropical stations in the Southern Hemisphere ADditional<br />
OZonesondes (SHADOZ) project has provided over 2000 profiles of stratospheric <strong>and</strong> tropospheric ozone since 1998.<br />
Balloon-borne electrochemical concentration cell (ECC) ozonesondes are used with st<strong>and</strong>ard radiosondes for pressure,<br />
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