Developing Courses in Applied Geography for Transportation Planners     

Frederick Stutz  Harvey E. Heiges 《The Professional geographer》1983,35(2):206-210

From the demand-side, the clients and the student practitioner, TARP was a success. Although some students were not overly enthusiastic, they were exposed to a large set of new ideas and presented new skills to equip them in the transition to multimodal transportation. Local Caltrans directors were pleased with TARP. From the supply side, JCTS, the faculty, and the CSUC Consortium, TARP was a partial success. The positive elements accruing to the faculty have been mentioned. Some of the negative elements of TARP such as high initial cost occurred because of the innovative nature and the grand scale of the program. The pool of potential faculty was probably too small to permit the degree of course specialization planned for in all five locations and given the decentralized approach. Three locations would have been better from the supply-side point of view. While certain difficulties remain with such educational programs in areas of identification of clients and their needs in planning, marketing, and teaching, a rich harvest of knowledge and rapport can accrue. Returned research dollars from agencies, interdisciplinary cooperation among professors, sharing of data and equipment by agencies for student theses and, in general, a larger role for geography programs in the state and local regions are recognized as benefits. Certain geography programs that have the required expertise to initiate such applied geographic educational efforts on a more modest scale must be prepared to take the plunge. They offer a unique perspective.  相似文献   

A pictorial comparison of interplanetary magnetic field polarity,solar wind speed,and geomagnetic disturbance index during the sunspot cycle     

N. R. Sheeley Jr.  J. R. Asbridge  S. J. Bame  J. W. Harvey 《Solar physics》1977,52(2):485-495

Observations of interplanetary magnetic field polarity, solar wind speed, and geomagnetic disturbance index (C9) during the years 1962–1975 are compared in a 27-day pictorial format that emphasizes their associated variations during the sunspot cycle. This display accentuates graphically several recently reported features of solar wind streams including the fact that the streams were faster, wider, and longer-lived during 1962–1964 and 1973–1975 in the declining phase of the sunspot cycle than during intervening years (Bame et al., 1976; Gosling et al., 1976). The display reveals strikingly that these high-speed streams were associated with the major, recurrent patterns of geomagnetic activity that are characteristic of the declining phase of the sunspot cycle. Finally, the display shows that during 1962–1975 the association between long-lived solar wind streams and recurrent geomagnetic disturbances was modulated by the annual variation (Burch, 1973) of the response of the geomagnetic field to solar wind conditions. The phase of this annual variation depends on the polarity of the interplanetary magnetic field in the sense that negative sectors of the interplanetary field have their greatest geomagnetic effect in northern hemisphere spring, and positive sectors have their greatest effect in the fall. During 1965–1972 when the solar wind streams were relatively slow (500 km s^-1), the annual variation strongly influenced the visibility of the corresponding geomagnetic disturbance patterns.Visiting Scientist, Kitt Peak National Observatory, Tucson, Arizona.Operated by the Association of Universities for Research in Astronomy, Inc., under contract with the National Science Foundation.  相似文献   

The magnetic field in some prominences measured with the He I, 5876 Å line     

J. W. Harvey  E. Tandberg-Hanssen 《Solar physics》1968,3(2):316-320

Observations of the longitudinal magnetic field of several prominences were made with the D₃, H, and H lines. There is no significant difference in the magnetic field measured with the helium and hydrogen lines. The possibility of a true difference in the fields on a scale much finer than that of our observations is not excluded.  相似文献   

How Necessary are Large-Scale Seismic Refraction Experiments?     

T. J. G. Francis 《Geophysical Journal International》1969,18(2):223-226

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Spectroscopic determinations of solar rotation   总被引：2，自引：0，他引：2  

Robert Howard  J. Harvey 《Solar physics》1970,12(1):23-51

Spectral line shift data obtained from full-disk magnetograms recorded at Mt. Wilson are analyzed for differential rotation. The method of analysis is discussed and the results from the data for 1966 through 1968 are presented. The average equatorial velocity over this period is found to be 1.93 km/sec or 13.76 deg/day (sidereal). This corresponds to a sidereal period of 26.16 days. The average results are = 2.78 × 10^-6 - 3.51 × 10^-7 sin² B - 4.43 × 10^-7 sin⁴ B rad/sec, whereB is the solar latitude. This indicates a smaller decrease of angular velocity with latitude than found by earlier investigators. Variations from day to day are caused by large-scale short-lived velocity fields on the solar surface. There also appear to be secular variations.Currently at the Kitt Peak National Observatory, Tucson, Arizona.  相似文献   

Prediction of heavy metal solubility in agricultural topsoils around two smelters by the physico-chemical parameters of the soils   总被引：1，自引：0，他引：1  

Matthieu?Fran?oisEmail author  Henri-Charles?Dubourguier  Dongyan?Li  Francis?Douay 《Aquatic Sciences - Research Across Boundaries》2004,66(1):78-85

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Rhinocerotid tooth enamel 18O/16O variability between 23 and 12 Ma in southwestern France     

Ilhem Bentaleb  Cyril Langlois  Céline Martin  Paula Iacumin  Matthieu Carré  Pierre-Olivier Antoine  Francis Duranthon  Issam Moussa  Jean-Jacques Jaeger  Nicholas Barrett  Ron Kandorp 《Comptes Rendus Geoscience》2006,338(3):172-179

The relationship between the oxygen isotope ratio of mammal tooth enamel and that of drinking water was used to reconstruct changes in the Miocene oxygen isotope ratio of rainfall (meteoric water ${\delta }^{18}$O_MW). These, in turn, are related to climatic parameters (temperature, precipitation and evaporation rate). ${\delta }^{18}$O values of rhinocerotid teeth from the Aquitaine Basin (southwestern France) suggest a significant climatic change between 17 and 12 Ma, characterized by cooling together with precipitation increase, in agreement with other terrestrial and oceanic records. To cite this article: I. Bentaleb et al., C. R. Geoscience 338 (2006).  相似文献   

Validating a rapid-update satellite precipitation analysis across telescoping space and time scales     

Francis Joseph Turk  Byung-Ju Sohn  Hyun-Jong Oh  Elizabeth E. Ebert  Vincenzo Levizzani  Eric A. Smith 《Meteorology and Atmospheric Physics》2009,105(1-2):99-108

In order to properly utilize remotely sensed precipitation estimates in hydrometeorological applications, knowledge of the accuracy of the estimates are needed. However, relatively few ground validation networks operate with the necessary spatial density and time-resolution required for validation of high-resolution precipitation products (HRPP) generated at fine space and time scales (e.g., hourly accumulations produced on a 0.25° spatial scale). In this article, we examine over-land validation statistics for an operationally designed, meteorological satellite-based global rainfall analysis that blends intermittent passive microwave-derived rainfall estimates aboard a variety of low Earth-orbiting satellite platforms with sub-hourly time sampling capabilities of visible and infrared imagers aboard operational geostationary platforms. The validation dataset is comprised of raingauge data collected from the dense, nearly homogeneous, 1-min reporting Automated Weather Station (network of the Korean Meteorological Administration during the June to August 2000 summer monsoon season. The space-time RMS error, mean bias, and correlation matrices were computed using various time windows for the gauge averaging, centered about the satellite observation time. For ±10 min time window, a correlation of 0.6 was achieved at 0.1° spatial scale by averaging more than 3 days; coarsening the spatial scale to 1.8° produced the same correlation by averaging over 1 h. Finer than approximately 24-h and 1° time and space scales, respectively, a rapid decay of the error statistics was obtained by trading-off either spatial or time resolution. Beyond a daily time scale, the blended estimates were nearly unbiased and with an RMS error of no worse than 1 mm day^?1.  相似文献   

Trends and variability of storminess in the Northeast Atlantic region, 1874–2007     

Xiaolan L. Wang  Francis W. Zwiers  Val R. Swail  Yang Feng 《Climate Dynamics》2009,33(7-8):1179-1195

This article builds on the previous studies on storminess conditions in the northeast North Atlantic–European region. The period of surface pressure data analyzed is extended from 1881–1998 to 1874–2007. The seasonality and regional differences of storminess conditions in this region are also explored in more detail. The results show that storminess conditions in this region have undergone substantial decadal or longer time scale fluctuations, with considerable seasonal and regional differences. The most notable differences are seen between winter and summer, and between the North Sea area and other parts of the region. In particular, winter storminess shows an unprecedented maximum in the early 1990s in the North Sea area and a steady upward trend in the northeastern part of the region, while it appears to have declined in the western part of the region. In summer, storminess appears to have declined in most parts of this region. In the transition seasons, the storminess trend is characterized by increases in the northern part of the region and decreases in the southeastern part, with increases in the north being larger in spring. In particular, the results also show that the earliest storminess maximum occurred in summer (around 1880), while the latest storminess maximum occurred in winter (in the early 1990s). Looking at the annual metrics alone (as in previous studies), one would conclude that the latest storminess maximum is at about the same level as the earliest storminess maximum, without realizing that this is comparing the highest winter storminess level with the highest summer storminess level in the period of record analyzed, while winter and summer storminess conditions have undergone very different long-term variability and trends. Also, storminess conditions in the NE Atlantic region are found to be significantly correlated with the simultaneous NAO index in all seasons but autumn. The higher the NAO index, the rougher the NE Atlantic storminess conditions, especially in winter and spring.  相似文献   

Detection of external influence on trends of atmospheric storminess and northern oceans wave heights   总被引：1，自引：0，他引：1  

Xiaolan L. Wang  Val R. Swail  Francis W. Zwiers  Xuebin Zhang  Yang Feng 《Climate Dynamics》2009,32(2-3):189-203

The atmospheric storminess as inferred from geostrophic wind energy and ocean wave heights have increased in boreal winter over the past half century in the high-latitudes of the northern hemisphere (especially the northeast North Atlantic), and have decreased in more southerly northern latitudes. This study shows that these trend patterns contain a detectable response to anthropogenic and natural forcing combined. The effect of external influence is found to be strongest in the winter hemisphere, that is, in the northern hemisphere in January–March and in the southern hemisphere in July–September. However, the simulated response to anthropogenic and natural forcing combined, which was obtained directly from climate models in the case of geostrophic wind energy and indirectly via an empirical downscaling procedure in the case of ocean wave heights, is significantly weaker than the magnitude of the observed changes in these parameters.  相似文献