FLIGHT ACTIVITY AND DISPERSAL OF RANGE CATERPILLAR MOTHS, HEMILEUCA OLIVIAE (LEPIDOPTERA: SATURNIIDAE)

1984 ◽  
Vol 116 (2) ◽  
pp. 247-252 ◽  
Author(s):  
Tom S. Bellows ◽  
John C. Owens ◽  
Ellis W. Huddleston

AbstractFlight of the range caterpillar occurred predominantly at dusk in the grasslands of eastern New Mexico in 1979 and 1980. The restricted period of flight in the evening corresponded to cool temperatures which probably favored mating success. Changes in atmospheric temperature and pressure had little effect on the number of moths flying from day to day. Most females oviposited within 10 m of the site of pupal eclosion.

1982 ◽  
Vol 27 (3) ◽  
pp. 335
Author(s):  
Willam D. Beavis ◽  
John C. Owens ◽  
John A. Ludwig ◽  
Ellis W. Huddleston

2002 ◽  
Vol 80 (4) ◽  
pp. 443-454 ◽  
Author(s):  
J R Pardo ◽  
M Ridal ◽  
D Murtagh ◽  
J Cernicharo

The Odin satellite is equipped with millimetre and sub-millimetre receivers for observations of several molecular lines in the middle and upper atmosphere of our planet (~25–100 km, the particular altitude range depending on the species) for studies in dynamics, chemistry, and energy transfer in these regions. The same receivers are also used to observe molecules in outer space, this being the astrophysical share of the project. Among the atmospheric lines that can be observed, we find two corresponding to molecular oxygen (118.75 GHz and 487.25 GHz). These lines can be used for retrievals of the atmospheric temperature vertical profile. In this paper, we describe the radiative-transfer modeling for O2 in the middle and upper atmosphere that we will use as a basis for the retrieval algorithms. Two different observation modes have been planned for Odin, the three-channel operational mode and a high-resolution mode. The first one will determine the temperature and pressure on an operational basis using the oxygen line at 118.75 GHz, while the latter can be used for measurements of both O2 lines, during a small fraction of the total available time for aeronomy, aimed at checking the particular details of the radiative transfer near O2 lines at very high altitudes (>70 km). The Odin temperature measurements are expected to cover the altitude range ~30–90 km. PACS Nos.: 07.57Mj, 94.10Dy, 95.75Rs


1994 ◽  
Vol 14 (9) ◽  
pp. 237-241 ◽  
Author(s):  
A. Dudhia ◽  
N.J. Livesey ◽  
F.W. Taylor

1984 ◽  
Vol 13 (2) ◽  
pp. 415-420 ◽  
Author(s):  
James D. Hansen ◽  
John A. Ludwig ◽  
John C. Owens ◽  
Ellis W. Huddleston

1933 ◽  
Vol 26 (4) ◽  
pp. 794-798 ◽  
Author(s):  
V. L. Wildermuth ◽  
J. C. Frankenfeld

Author(s):  
Shihong Zhang ◽  
Ning Li

This article discussed the thermal efficiency, stability, and pollutant emissions characteristics of the combustion of lean natural gas-air mixtures in Pd metal based honeycomb monoliths by means of experiments on a practical burner V. The chemistry at work in the monoliths was then investigated using fundamental experimental reactors, namely the stagnation point flow reactor or SPFR. It was found that catalytic combustion inhibited the extent of gas-phase oxidation and increased the surface temperature of homogeneous ignition. According to the applications of catalytic combustion in the condenser boiler, the data of catalytic combustion condenser boiler V were measured at atmospheric temperature and pressure. The study also showed that more than 100% of its thermal efficiency was found possible while preserving near zero pollutant emissions. For all the catalysts tested, flow rates, and mixture compositions of natural gas and air used here, no CO, unburned fuel nor NOx were detected as long as surface combustion was taking place.


2011 ◽  
Vol 4 (5) ◽  
pp. 893-907 ◽  
Author(s):  
B. T. Marshall ◽  
L. E. Deaver ◽  
R. E. Thompson ◽  
L. L. Gordley ◽  
M. J. McHugh ◽  
...  

Abstract. Measurement of atmospheric temperature as a function of pressure, T(P), is key to understanding many atmospheric processes and a prerequisite for retrieving gas mixing ratios and other parameters from solar occultation measurements. This paper gives a brief overview of the solar occultation measurement technique followed by a detailed discussion of the mechanisms that make the measurement sensitive to temperature. Methods for retrieving T(P) using both broadband transmittance and refraction are discussed. Investigations using measurements of broadband transmittance in two CO2 absorption bands (the 4.3 and 2.7 μm bands) and refractive bending are then presented. These investigations include sensitivity studies, simulated retrieval studies, and examples from SOFIE.


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