scholarly journals Laboratory Studies of Planetary Molecules and Ices: The Case of IO

1992 ◽  
Vol 150 ◽  
pp. 435-436
Author(s):  
F. Salama ◽  
S. A. Sandford ◽  
L. J. Allamandola

The techniques of low temperature spectroscopy are applied here to analyze infrared observational data of Io in the 2.0-5.0 μm range. The presence of solid H2S and traces of H2O in the SO2-dominant surface ices are derived from this analysis and it is suggested that CO2 clusters may as well be present near the surface of Io.

1962 ◽  
Vol 35 (2) ◽  
pp. 546-557
Author(s):  
R. J. Brown ◽  
R. B. Knill ◽  
J. F. Kerscher ◽  
R. V. Todd

Abstract cis-1,4-Polybutadiene is proving to be one of the most versatile compounding materials available to the tire compounder. It has characteristics as a polymer which make it acceptable as a replacement for either natural or synthetic rubber in tire applications. The successful use of cis-polybutadiene in this dual role, however, is dependent upon discovering its peculiarities and sensitivities and then exploiting them in that area of the tire where they are most applicable. Laboratory studies, confirmed by over three million miles of tire testing, have shown that in either passenger or truck tires the carcass durability can be substantially improved, operating temperature lowered, low temperature performance improved, and treadwear resistance increased when cis-PBD is properly used in the respective tire components.


1999 ◽  
Vol 17 (2) ◽  
pp. 57-62 ◽  
Author(s):  
Cindy L. Flinn ◽  
Edward N. Ashworth

Abstract Experiments were conducted to determine if dormant buds of Forsythia taxa exhibit the deep supercooling characteristic. Specimens were collected from thirteen Forsythia taxa including: F. suspensa (Thunb.) Vahl, F. x intermedia cv. Spectabilis (Koehne), F. x intermedia cv. Lynwood (G.E. Peterson), F. europaea (Degen and Baldacci), F. giraldiana (Lingelsh), F. japonica (Makino) var. saxatilis (Nakai), F. mandshurica (Uyeki), F. ovata (Nakai), F. suspensa var. fortunei (Lindl.), F. viridissima (Lindl.), F. x intermedia cv. Arnold Giant (Sax), F. cv. Arnold's Dwarf, and F. cv. Meadowlark (Flint). Buds and attached stem segments, were cooled at 2C (3.6F) per hour, and the temperature at which freezing occurred was determined by thermal analysis. Typically, two distinct freezing events were detected within Forsythia buds. The first freezing event, or high temperature exotherm, occurred just below 0C (32F), while the second freezing event, or low temperature exotherm, occurred between −16C (3.2F) and −28C (−18.4F). The low temperature exotherm corresponded to the freezing of supercooled water within dormant buds, and the detection of low temperature exotherms in buds of all 13 Forsythia taxa indicated that deep supercooling is common among members of this genus. In nine of the 13 Forsythia taxa, the temperature of the low temperature exotherm was an accurate indicator of bud freeze-tolerance (LT50), as determined by a laboratory freeze-stress protocol. The discrepancies noted in the other four taxa were apparently due to the occurrence of field freezing injury prior to conducting these laboratory studies. Evidence indicated a relationship between the extent of supercooling and the size of the pistil in dormant Forsythia buds.


2019 ◽  
Vol 492 (1) ◽  
pp. 1523-1529 ◽  
Author(s):  
Diogo Belloni ◽  
Matthias R Schreiber

ABSTRACT Understanding the origin of the magnetic fields in white dwarfs (WDs) has been a puzzle for decades. A scenario that has gained considerable attention in the past years assumes that such magnetic fields are generated through a dynamo process during common-envelope evolution. We performed binary population models using an up-to-date version of the bse code to confront the predictions of this model with observational results. We found that this hypothesis can explain only the observed distribution of WD magnetic fields in polars and pre-polars and the low-temperature WDs in pre-polars if it is re-scaled to fit the observational data. Furthermore, in its present version, the model fails to explain the absence of young, close detached WD+M-dwarf binaries harbouring hot magnetic WDs and predicts that the overwhelming majority of WDs in close binaries should be strongly magnetic, which is also in serious conflict with the observations. We conclude that either the common-envelope dynamo scenario needs to be substantially revised or a different mechanism is responsible for the generation of strong WD magnetic fields in close binaries.


1975 ◽  
Vol 23 (2) ◽  
pp. 237 ◽  
Author(s):  
JA Mckenzie

Observations in the cellar at the 'Chateau Tahbilk' vineyard in Victoria demonstrate that while adults of D. melanogaster can be collected throughout the year, larvae and pupae are not found when the temperature is less than 13�C. Laboratory studies confirm that the amount of mating and oviposition of this species is restricted in the vicinity of this temperature. Field experiments indicate that during winter the survival probability of adults is greater than the developmental probability of larvae and pupae, and that the population may be reconstituted during spring by overwintering adults, most probably inseminated females. These results show how adaptive modification in the pattern of a life cycle may be evolved by selection under conditions of extreme environment.


Author(s):  
T.B. Onasch ◽  
S.E. Anthony ◽  
R.T. Tisdale ◽  
A.J. Prenni ◽  
M.A. Tolbert

mSphere ◽  
2019 ◽  
Vol 4 (6) ◽  
Author(s):  
Keisuke Inomura ◽  
Curtis Deutsch ◽  
Samuel T. Wilson ◽  
Takako Masuda ◽  
Evelyn Lawrenz ◽  
...  

Crocosphaera is one of the major N2-fixing microorganisms in the open ocean. On a global scale, the process of N2 fixation is important in balancing the N budget, but the factors governing the rate of N2 fixation remain poorly resolved. Here, we combine a mechanistic model and both previous and present laboratory studies of Crocosphaera to quantify how chemical factors such as C, N, Fe, and O2 and physical factors such as temperature and light affect N2 fixation. Our study shows that Crocosphaera combines multiple mechanisms to reduce intracellular O2 to protect the O2-sensitive N2-fixing enzyme. Our model, however, indicates that these protections are insufficient at low temperature due to reduced respiration and the rate of N2 fixation becomes severely limited. This provides a physiological explanation for why the geographic distribution of Crocosphaera is confined to the warm low-latitude ocean.


2013 ◽  
Author(s):  
Aparna Raju Sagi ◽  
Maura C Puerto ◽  
Yu Bian ◽  
Clarence A. Miller ◽  
George J Hirasaki ◽  
...  

2007 ◽  
Vol 20 (8) ◽  
pp. 252-255 ◽  
Author(s):  
P. Raj ◽  
M. A. Khaleel Akmal ◽  
Y. V. Subba Rao ◽  
S. Moinuddin Ahmed ◽  
R. Vaidyeswaran

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