Inductive electric field of a time-dependent ring current     

C.H. Murphy  C.S. Wang  J.S. Kim 《Planetary and Space Science》1975,23(8):1205-1209

The inductive electric field generated by a time-dependent symmetric ring current has been investigated. The symmetric ring current was modelled by a population of protons drifting in a magnetic dipole field. The interaction of these protons with ion-cyclotron waves was assumed to be the dominant energy loss process for the ring current protons, at least under certain conditions. The calculation, with spectral densities for the ion-cyclotron waves that are based on experimental data, showed that an azimuthal inductive electric field of as much as 0.25 mV/m can be produced by this mechanism. Furthermore there is evidence that if the spectral density of the waves is substantially larger than the one adopted here, the electric field might increase to the order of 1.0 mV/m or more.  相似文献   

Calculated Variations in the H⁺ Content of the Plasmasphere     

J. A. Murphy  G. J. Bailey  R. J. Moffett 《Geophysical Journal International》1975,41(3):319-325

  相似文献   

TOURISM DEVELOPMENT ON VANCOUVER ISLAND: AN ASSESSMENT OF THE CORE-PERIPHERY MODEL *     

Peter E. Murphy  Betty Andressen 《The Professional geographer》1988,40(1):32-42

This paper examines tourism development on Vancouver Island, B.C. in terms of the core-periphery approach to regional planning. It examines whether a core area (Victoria) is willing to share its tourism business with the rest of the island, and then focuses on the situation in a peripheral region (the Cowichan Valley Regional District–CVRD). A discriminant analysis of CVRD residents reveals they have different views regarding tourism's potential and future in their region. A follow-up analysis, reflecting a change in the scale of enquiry and local core-periphery conditions, shows residents'perceptions and priorities will change according to their respective area groupings. This analysis reveals that residents of a peripheral region, who are expected to participate in and welcome tourism development initiatives developed by senior levels of government, will in fact have different opinions regarding the industry and its potential. These differences are linked to present levels of tourism activity within the periphery and the varying community aspirations linking tourism's development potential with local needs and priorities.  相似文献   

Second-Order Correction to the Reed-Otterman Theory     

S. L. Kahalas  B. L. Murphy 《Geophysical Journal International》1971,26(1-4):379-389

Summary The theory of Reed and Otterman, which describes the propagation of a weak shock wave in an inhomogeneous medium, is extended to include the next higher-order term of relative overpressure. This extension allows a matching of theory to initial starting conditions of the shock at a point closer to the source than the Reed-Otterman theory itself. The modified theory gives a value of the shock pressure that agrees well with the numerical calculation performed by Greene and Whitaker for the upward moving shock wave from a low altitude detonation.  相似文献   

Acoustic-Gravity Wave Generation at 120 km Altitude by Sea Level Detonation: A Preliminary Analysis of the Greene-Whitaker Calculation     

S. L. Kahalas  B. L. Murphy 《Geophysical Journal International》1971,26(1-4):391-398

Summary The Greene and Whitaker mechanism for the production of an acoustic- gravity wave in the 100-km region of the ionosphere is discussed from a physical point of view. The shock wave from a low altitude detonation propagates upward and, interacting with the atmosphere in the 100-km region, produces a horizontally propagating acoustic-gravity wave. Several aspects of this phenomenon are discussed. The initial period of the generated waves is in the 200–300 s range, the energy associated with the wave is about 0.3 per cent of the yield, and the wave generated appears to result principally from the refraction of the shock at the 100-km level.  相似文献   

Obituary Robert W. Pennak     

Myron D. Groskopp  Hugh J. Murphy 《Aquatic Sciences - Research Across Boundaries》2004,66(4):i-i

Obituary

Obituary Robert W. Pennak  相似文献   

The DynaMICCS perspective     

S. Turck-Chièze  P. Lamy  C. Carr  P. H. Carton  A. Chevalier  I. Dandouras  J. M. Defise  S. Dewitte  T. Dudok de Wit  J. P. Halain  S. Hasan  J. F. Hochedez  T. Horbury  P. Levacher  M. Meissonier  N. Murphy  P. Rochus  A. Ruzmaikin  W. Schmutz  G. Thuillier  S. Vivès 《Experimental Astronomy》2009,23(3):1017-1055

The DynaMICCS mission is designed to probe and understand the dynamics of crucial regions of the Sun that determine solar variability, including the previously unexplored inner core, the radiative/convective zone interface layers, the photosphere/chromosphere layers and the low corona. The mission delivers data and knowledge that no other known mission provides for understanding space weather and space climate and for advancing stellar physics (internal dynamics) and fundamental physics (neutrino properties, atomic physics, gravitational moments...). The science objectives are achieved using Doppler and magnetic measurements of the solar surface, helioseismic and coronographic measurements, solar irradiance at different wavelengths and in-situ measurements of plasma/energetic particles/magnetic fields. The DynaMICCS payload uses an original concept studied by Thalès Alenia Space in the framework of the CNES call for formation flying missions: an external occultation of the solar light is obtained by putting an occulter spacecraft 150 m (or more) in front of a second spacecraft. The occulter spacecraft, a LEO platform of the mini sat class, e.g. PROTEUS, type carries the helioseismic and irradiance instruments and the formation flying technologies. The latter spacecraft of the same type carries a visible and infrared coronagraph for a unique observation of the solar corona and instrumentation for the study of the solar wind and imagers. This mission must guarantee long (one 11-year solar cycle) and continuous observations (duty cycle > 94%) of signals that can be very weak (the gravity mode detection supposes the measurement of velocity smaller than 1 mm/s). This assumes no interruption in observation and very stable thermal conditions. The preferred orbit therefore is the L1 orbit, which fits these requirements very well and is also an attractive environment for the spacecraft due to its low radiation and low perturbation (solar pressure) environment. This mission is secured by instrumental R and D activities during the present and coming years. Some prototypes of different instruments are already built (GOLFNG, SDM) and the performances will be checked before launch on the ground or in space through planned missions of CNES and PROBA ESA missions (PICARD, LYRA, maybe ASPIICS).  相似文献   

Cosmic dynamics in the era of Extremely Large Telescopes     

J. Liske  A. Grazian  E. Vanzella  M. Dessauges  M. Viel  L. Pasquini  M. Haehnelt  S. Cristiani  F. Pepe  G. Avila  P. Bonifacio  F. Bouchy  H. Dekker  B. Delabre  S. D'Odorico  V. D'Odorico  S. Levshakov  C. Lovis  M. Mayor  P. Molaro  L. Moscardini  M. T. Murphy  D. Queloz  P. Shaver  S. Udry  T. Wiklind  S. Zucker 《Monthly notices of the Royal Astronomical Society》2008,386(3):1192-1218

The redshifts of all cosmologically distant sources are expected to experience a small, systematic drift as a function of time due to the evolution of the Universe's expansion rate. A measurement of this effect would represent a direct and entirely model-independent determination of the expansion history of the Universe over a redshift range that is inaccessible to other methods. Here we investigate the impact of the next generation of Extremely Large Telescopes on the feasibility of detecting and characterizing the cosmological redshift drift. We consider the Lyα forest in the redshift range  2 < z < 5  and other absorption lines in the spectra of high-redshift QSOs as the most suitable targets for a redshift drift experiment. Assuming photon-noise-limited observations and using extensive Monte Carlo simulations we determine the accuracy to which the redshift drift can be measured from the Lyα forest as a function of signal-to-noise ratio and redshift. Based on this relation and using the brightness and redshift distributions of known QSOs we find that a 42-m telescope is capable of unambiguously detecting the redshift drift over a period of ∼20 yr using 4000 h of observing time. Such an experiment would provide independent evidence for the existence of dark energy without assuming spatial flatness, using any other cosmological constraints or making any other astrophysical assumption.  相似文献   

Ownership and Spatial Distribution of Eagle Ford Mineral Wealth in Live Oak County,Texas     

Trey Murphy  Christian Brannstrom  Matthew Fry 《The Professional geographer》2017,69(4):616-628

U.S. unconventional hydrocarbon production is a driver of economic growth, but mineral wealth ownership is poorly understood and shrouded in “local wealth” mythology that claims royalties from hydrocarbons mostly benefit people who live near sites of production. Mineral property tax appraisals, as proxies for mineral wealth from Live Oak County, a representative Eagle Ford Shale county in Texas, show that 96 percent of assessed mineral wealth concentrates among energy firms and individuals in Texas metropolitan regions; 1.95 percent of mineral wealth remains “local” to the production county, challenging local wealth myths. Deviating from nation-state scalar approaches, local and regional spatial studies of other energy regions might reveal similar wealth distributions, enabling generalizations about hydrocarbon production economic outcomes.  相似文献   

Economic‐Development Stakeholder Perspectives on Boomtown Dynamics in the Eagle Ford Shale,Texas          下载免费PDF全文

Trey Murphy  Christian Brannstrom  Matthew Fry  Michael Ewers 《Geographical review》2018,108(1):24-44

Unconventional oil and gas production in the United States reversed a decades‐old trend of rising oil imports, provided an argument for lifting the U.S. crude oil export ban and motivated the development of domestic natural gas export facilities. But the most visible impact of unconventional‐hydrocarbon extraction is the creation of boomtowns in rural regions. Despite widespread media coverage, scholarly analysis of boomtowns is restricted to regional econometric studies with little attention to how economic stakeholders understand and respond to booming economies. Here we analyze interviews with key economic stakeholders in the Eagle Ford Shale in Texas. Respondents consider their community's economic success relative to the price of oil and indicate concerns about the deterioration of roads, high housing demand, and skyrocketing wages. We also re‐examine John Gilmore's foundational work on boomtowns in the 1970s in the context of contemporary unconventional extraction.  相似文献