Issue 10 Volume 41 May 16, 2003
Issue 10 Volume 41 May 16, 2003
Issue 10 Volume 41 May 16, 2003
- TAGS
- volume
- 202.118.250.135
Create successful ePaper yourself
Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.
star. Proplyds are, thus, sources of bright line emission. The name proplyd is derived from the likelihood that the circumstellar<br />
material harbors a protoplanetary disk.<br />
Derived from text<br />
H Ii Regions; Hot Stars; Nebulae; Protoplanetary Disks<br />
<strong>2003</strong>0032335 Instituto Nacional de Pesquisas Espacias, Sao Jose dos Campos, Brazil<br />
Ozone and UV-B Radiation Observations at the Andes Mountains<br />
Guarnieri, Fernando Luis; <strong>2003</strong>; 118 pp.; In Portuguese; Original contains color illustrations<br />
Report No.(s): INPE-9552-TDI/828; Copyright; Avail: CASI; A06, Hardcopy<br />
The region of La Paz, Bolivia (68,03 W, <strong>16</strong>,52 S) located at an altitude of 3420m, has favorable features to study the<br />
altitude effects on total ozone and UV-B radiation. Ozone data from a Brewer Spectrophotometer, from the TOMS<br />
Spectrometer and ozone soundings at three locations (La Paz, Cuiaba and Natal) were used to compare the ozone layer at the<br />
Bolivian Andes region with results from Cuiab and Natal, in Brazil. The average vertical ozone profile for La Paz and Cuiaba<br />
were determined and compared with the Natal ozone profile. The results from this analysis show the altitude effect on the<br />
ozone column observed by TOMS and confirmed by ozone soundings at La Paz, where a mean reduction of 7,7UD is<br />
observed, comparing with Cuiaba. Analysis of direct ultraviolet radiation shows high values of the La Paz Natal ratio, with<br />
2,37 for 306nm and 1,94 for 320nm, showing that La Paz presents values of direct UV radiation higher than Natal. A<br />
significant part of this increase in UV-B radiation at La Paz results from Rayleigh scattering decrease, due to a thinner<br />
atmosphere.<br />
Author<br />
Andes Mountains (South America); Ozone; Ultraviolet Radiation; Observation; Spectrophotometers<br />
<strong>2003</strong>0032383 Army Cold Regions Research and Engineering Lab., Hanover, NH<br />
Mechanical System Simulations for Seismic Signature Modeling<br />
Lacombe, J.; Moran, M.; Harjes, D.; Oct. 2001; ISBN0309084997; 11 pp.; In English; Original contains color illustrations<br />
Report No.(s): AD-A4<strong>10</strong><strong>10</strong>9; No Copyright; Avail: CASI; A03, Hardcopy<br />
In this paper we present seismic signature simulations using ground vibration inputs from high-fidelity 3-D mechanical<br />
system models. Results for an M1A1 and T72 are discussed. By analyzing the simulated seismic signature data in conjunction<br />
with the spectral features associated with the vibrations of specific vehicle sprung and un-sprung components we are able to<br />
make unambiguous associations of seismic signal features with suspension elements, offering valuable insight into target<br />
classification. The development of a utility (‘Tankmod’) to streamline creation of DADS tracked vehicle dynamic models for<br />
generating seismic signals was reported in 2000. A model of an M1A1 tank created using Tankmod was described. During the<br />
past year, two new models were created: a T72 tank and a BMP-2 armored personnel carrier. In addition, an improved vehicle<br />
speed/steer controller was developed. The new controller maintains realistic vehicle behavior by properly limiting drive<br />
sprocket torques and sprocket rotation for skid steering. Model inputs used in seismic signature modeling are in the form of<br />
time series of ground reaction force and absolute position for each track block.<br />
DTIC<br />
Dynamic Models; Tracked Vehicles; Acoustic Simulation; Spectral Signatures<br />
<strong>2003</strong>00324<strong>10</strong> NASA Goddard Space Flight Center, Greenbelt, MD, USA<br />
The Magnetospheric Constellation Mission (MC-DRACO)<br />
Moore, Thomas E.; [<strong>2003</strong>]; 17 pp.; In English; Original contains color illustrations; No Copyright; Avail: CASI; A03,<br />
Hardcopy<br />
The Magnetospheric Constellation Mission Dynamic Response and Coupling Observatory (MC-DRACO), the logical<br />
outgrowth of a sequence of STP missions, will explore plasma transport and energy conversion processes over a broad range<br />
of spatial sizes. Designed to be a meso-/macroscope for the magnetotail, it will resolve persistent controversies and yield a<br />
new understanding on which to build a predictive science of next generation magnetospheric meteorology.<br />
Derived from text<br />
Satellite Constellations; Earth Magnetosphere; Scientific Satellites<br />
<strong>2003</strong>0032487 NASA Goddard Space Flight Center, Greenbelt, MD, USA<br />
International Laser Ranging Services (ILRS) 2001 Annual Report<br />
Pearlman, Michael, Editor; Torrence, Mark, Editor; Noll, Carey, Editor; June 2002; 179 pp.; In English; Original contains<br />
color illustrations<br />
Report No.(s): NASA/TP-2002-21<strong>16</strong><strong>10</strong>; NAS 1.60-21<strong>16</strong><strong>10</strong>; Rept-<strong>2003</strong>-00851-0; No Copyright; Avail: CASI; A09, Hardcopy<br />
131