scholarly journals MODELING TIDE’S INFLUENCE ON SEAWALL’S SURFACE TEMPERATURE IN TROPICAL REGIONS

2018 ◽  
pp. 61
Author(s):  
Kuifeng ZHAO ◽  
Jing YUAN ◽  
Philip L-F LIU
Keyword(s):  
Surface Temperature ◽  
Intertidal Zone ◽  
High Surface ◽  
Primary Reason ◽  
Tropical Regions ◽  
Tidal Motion ◽  
High Surface Temperature ◽  
Local Ecosystem ◽  
Intense Solar Radiation ◽  
Engineering Practices

In tropical regions, intense solar radiation on seawall can lead to a high surface temperature, which far exceeds common marine species’ tolerable limits. This is a primary reason for low biodiversity on Singapore’s seawalls and therefore must be considered in eco-engineering practices. The intertidal zone of a seawall is periodically submerged and cooled by the tidal motion, and therefore can support a local ecosystem. The objective of this research is to establish a predictive model for surface temperature of seawall’s intertidal zone and use this model to study how local biodiversity is affected by the occurrence of high temperature.

HIGH SURFACE TEMPERATURE GAS-SOLID (FE3O4 AND H2O/CO2) INTERFACIAL REACTION CHARACTERISTICS

2018 ◽  
Author(s):  
Bachirou Guene Lougoua ◽  
Yong Shuai ◽  
Dongmei Han ◽  
Xing Huang ◽  
Heping Tan
Keyword(s):  
Surface Temperature ◽  
Interfacial Reaction ◽  
High Surface ◽  
Reaction Characteristics ◽  
High Surface Temperature

scholarly journals Models for Nuclei of Planetary Nebulae and for Ultraviolet Stars

1974 ◽  
Vol 59 ◽  
pp. 113-114
Author(s):  
J. Katz ◽  
R. Malone ◽  
E. E. Salpeter
Keyword(s):  
Surface Temperature ◽  
Total Mass ◽  
High Surface ◽  
Planetary Nebulae ◽  
Red Giants ◽  
High Luminosity ◽  
Stages Of Development ◽  
Initial Carbon ◽  
High Surface Temperature ◽  
Central Stars

A series of stellar models were evolved, all with a total mass of 0.65 M⊙, an initial carbon-oxygen core of mass 0.60 M⊙, an intermediate helium mantle and an outer hydrogen-rich envelope with mass varying from case to case. Although the most hydrogen-rich cases resulted in red giants, cases with ≲ 0.01 M⊙ in the hydrogen envelope evolved at high surface temperature. The early stages of development of these models are similar to observed central stars of planetary nebulae. The later stages (when the nebula should be very thin optically) still have a high luminosity; the relevance to ‘ultraviolet stars’ will be discussed.

Heat transfer from a rarefied plasma flow to a metallic particle with high surface temperature

1994 ◽  
Vol 27 (8) ◽  
pp. 1637-1645 ◽  
Author(s):  
Xi Chen ◽  
Ji Chen ◽  
Yandan Wang
Keyword(s):  
Heat Transfer ◽  
Surface Temperature ◽  
Plasma Flow ◽  
High Surface ◽  
Metallic Particle ◽  
High Surface Temperature

scholarly journals Characteristics of Urban Heat Island Condition in DKI Jakarta

2013 ◽  
Vol 27 (2) ◽  
pp. 111
Author(s):  
Siti Badriyah Rushayati ◽  
Rachmad Hermawan
Keyword(s):  
Spatial Distribution ◽  
Inner City ◽  
Surface Temperature ◽  
Urban Heat Island ◽  
Co2 Emission ◽  
High Surface ◽  
Heat Island ◽  
High Co2 ◽  
Urban Heat ◽  
High Surface Temperature

DKI Jakarta area with high CO2 emission and 84,95 % of  built-up areas (year of 2009) cause urban heat island (UHI).  To overcome UHI problems, its characteristics must be known.  Trend analysis of surface temperature areas was conducted by comparison of surface temperature  spatial distribution of 2006 with 2010.  UHI analysis based on geograpical coordinates were also conducted.  High surface temperature of > 34 ºC was on inner city and decreasing to sub urban area.  High surface temperature were especially on high density bulit-up areas. Priority of  solving UHI problems are conducted on high surface temperature areas.

scholarly journals Shall we Observe a Radio Binary Pulsar in SN 1987A?

1992 ◽  
Vol 128 ◽  
pp. 222-224
Author(s):  
Qiao G. J.
Keyword(s):  
Neutron Star ◽  
Surface Temperature ◽  
High Surface ◽  
Star Model ◽  
Single Star ◽  
X Ray ◽  
Binary Pulsar ◽  
Collapse Model ◽  
High Surface Temperature ◽  
Γ Ray

AbstractAn induced-collapse model [hereafter IC model; He et al. (1990)] can overcome the problems of the single star model of SN1987A. According to the IC model, there is a possibility that the SN1987A remnant will be a binary system with two neutron stars, one of them (SK-69 202) will have a strong magnetic field and a high surface temperature which favors detection as an X-ray or γ-ray pulsar. If the surface temperature of the neutron star cools down to T = 107 K, a radio binary pulsar is expected. There is also the possibility that an X-ray or γ-ray pulsar will be observed first, and only later will a radio pulsar will be detected.A newly formed neutron star is thought to have a short (millisecond) period. In this case, the core emission beam is then very large (Qiao 1992) and is thus very likely to swing in the direction of the Earth.

High surface temperature on Venus: Evaluation of the greenhouse explanation

Icarus ◽  
1969 ◽  
Vol 11 (2) ◽  
pp. 171-179 ◽  
Author(s):  
George Ohring
Keyword(s):  
Surface Temperature ◽  
High Surface ◽  
High Surface Temperature

High surface temperature of endovaginal probes

1990 ◽  
Vol 63 (756) ◽  
pp. 983-983
Author(s):  
M. Davison ◽  
P. Clark
Keyword(s):  
Surface Temperature ◽  
High Surface ◽  
High Surface Temperature

Vibrationally Excited CO2 Formed in CO + NO Reaction on Pd(110) Surface in High Surface Temperature Range

2005 ◽  
Vol 103 (3-4) ◽  
pp. 179-184 ◽  
Author(s):  
Kenji Nakao ◽  
Shin-ichi Ito ◽  
Keiichi Tomishige ◽  
Kimio Kunimori
Keyword(s):  
Surface Temperature ◽  
High Surface ◽  
Vibrationally Excited ◽  
Temperature Range ◽  
High Surface Temperature
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