نتایج جستجو برای: dry regions commonly have strong winds during daytime

تعداد نتایج: 4689826  

2000
M. Teshiba H. Hashiguchi S. Fukao

Typhoon 9707 (Opal) was observed with the VHF-band Middle and Upper atmosphere (MU) radar, an L-band boundary layer radar (BLR), and a vertical-pointing C-band meteorological radar at the Shigaraki MU Observatory in Shiga prefecture, Japan on 20 June 1997. The typhoon center passed about 80 km southeast from the radar site. Mesoscale precipitating clouds developed due to warmmoist airmass trans...

Journal: :Journal Of Geophysical Research: Space Physics 2022

Numerical simulations using the National Center for Atmospheric Research (NCAR) thermosphere-ionosphere-electrodynamics general circulation model (TIE-GCM) are performed to elucidate effects of interplanetary magnetic field (IMF) on middle thermosphere composition during a “geomagnetically quiet” period from day year (DOY) 110–111 in 2019 (when Auroral electrojet (AE) index never exceeded 300 n...

Journal: :Frontiers in Environmental Science 2023

The supergeostrophic flow remains seldomly reported from an observational perspective. Here, 1 year record of radar wind profiler measurements and ERA-5 reanalysis collected at Beijing observatory station are used to characterize the vertical structures Ekman spirals in lower troposphere. It is found that shows significant diurnal variation, with lowest frequency for forming during daytime unde...

1998
Stephen D. Tse Carlos Fernandez-Pello

In dry grasslands, dangerous wildfires are of particular concern during hot, dry seasons in regions encountering high winds. It is possible that such winds can cause power cables to come close enough together to arc or collide with trees, and produce metal sparks or burning embers which can be carried by the wind and land in adjacent areas of dry vegetation. A major issue is whether or not such...

Journal: :Geoscientific Model Development 2022

Abstract. The latest operational National Air Quality Forecast Capability (NAQFC) has been advanced to use the Community Multiscale (CMAQ) model (version 5.3.1) with CB6r3 (Carbon Bond 6 revision 3) AERO7 7 of aerosol module) chemical mechanism and is driven by Finite-Volume Cubed-Sphere (FV3) Global System, version 16 (GFSv16). This update accomplished via development meteorological preprocess...

1981
S. G. H. PHILANDER R. C. PACANOWSKI

Oscillating wind with a period P induce variability with the following characteristics in the upper few hundred meters of the equatorial zone (5øN to 5øS) of the ocean. (1) P < 10 days: these winds fluctuate too rapidly to generate strong currents and excite primarily waves. (2) 10 days < P < 50 days: At these periods the winds generate intense equatorial jets in the upper 50 m, but at greater ...

1997
ALFREDO ROCHA IAN SIMMONDS

This paper investigates the role that air–sea interaction processes may play in interannual variability of south-eastern African summer rainfall. The principal spatial modes of south-eastern African summer rainfall are first identified using principal component analysis. Four modes are retained. The most important mode of variability is found to represent rainfall variability over most of the d...

2007

We are all familiar with the fact that cities are generally warmer than the surrounding, more rural areas. We see it referenced most nights in our television weather reports. It is especially significant on nights with clear skies and light winds which favor radiational cooling. This is most significant in the rural areas but in the city, the excess heat absorbed during the day and the local he...

2007

We are all familiar with the fact that cities are generally warmer than the surrounding, more rural areas. We see it referenced most nights in our television weather reports. It is especially significant on nights with clear skies and light winds which favor radiational cooling. This is most significant in the rural areas but in the city, the excess heat absorbed during the day and the local he...

2006
Serena Bertone Corina Vogt Torsten Enßlin

The origin of intergalactic magnetic fields is still a mystery and several scenarios have been proposed so far: among them, primordial phase transitions, structure formation shocks and galactic outflows. In this work we investigate how efficiently galactic winds can provide an intense and widespread “seed” magnetisation. This may be used to explain the magnetic fields observed today in clusters...

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