Vandermonde matrix analysis of long‐period seismograms     

Freeman Gilbert 《Geophysical Journal International》2001,146(3):843-849

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Interstellar archaeology and the prevalence of intelligence     

J. Freeman  M. Lampton 《Icarus》1975,25(2):368-369

Simple calculations indicate that the spatial density in the galaxy of extinct civilizations, and of planets inhabited by intelligent creatures who do not have technical civilizations, may be quite large.  相似文献   

Bow shock protons in the lunar environment     

J. Benson  J. W. Freeman  H. K. Hills  R. R. Vondrak 《Earth, Moon, and Planets》1975,14(1):19-25

Protons from the Earth's bow shock are observed by the Suprathermal Ion detector Experiment (SIDE) in two regions of the lunar orbit. The dawn region begins at the dawn side bow shock crossing and ends ç 5 days later and the dusk region begins at ç 2 days prior to entering the dusk side magnetosheath and ends at the inbound bow shock crossing. Dusk and dawn refer to a terrestrial coordinate system. The dominant contribution to the ion spectra observed by the SIDE in these regions is from particles with energies between ç 750 eV q^–1 and 3500 eV q^–1. 3500 eVq^–1 is the upper limit of the energy range of the detector. Analysis of simultaneous data from the Explorer 35 magnetometer and the SIDE indicates that the observability of bow shock protons at the lunar distance is dependent on the configuration of the interplanetary magnetic field.Paper presented at the Conference on Interactions of the Interplanetary Plasma with the Modern and Ancient Moon, sponsored by the Lunar Science Institute, Houston, Texas and held at the Lake Geneva Campus of George Williams College, Wisconsin, between September 30 and October 4, 1974.  相似文献   

Deep radio occultations and “evolute flashes”; their characteristics and utility for planetary studies     

V.R. Eshleman  G.L. Tyler  W.T. Freeman 《Icarus》1979,37(3):612-626

Radio occultation studies of the structure of planetary atmospheres have generally involved relatively shallow penetration of the spacecraft behind the limb of the planet in the plane of the sky. Current radio link sensitivities allow detection of the radio signals at all occultation depths, whenever the planet-spacecraft distance is sufficiently large for the refraction to occur at atmospheric heights where microwave absorption is not too large. Voyager 1 at Jupiter and Voyager 2 at Saturn will pass almost directly behind the planets as viewed from the Earth. Thus they will pass through the caustics that corresponds to the focal line of a spherical planet, expanded by oblateness into a surface approximating a four-cusp cylinder. In the plane of the sky, the projection of this surface approximates the evolute of the planet's limb. As the spacecraft passes behind the planet with its antenna tracking the occulting limb, the strength of the radio signals received on Earth will at first decrease due to defocusing in the atmosphere, but then increase as the evolute is approached, because of the focusing caused by limb curvature. Inside the evolute there are four simultaneous signal paths over four limb positions. If we neglect absorption, focused signals for an instant could become orders of magnitude stronger than for the unocculted spacecraft. Measurements of the frequency and intensity of deep occultation signals, and of the timing and character of these “evolute flashes”, could provide information on atmospheric absorption, turbulence, and structure, and on details of the shape of the atmosphere at the focusing limbs as affected, for example, by planetary gravitational moments, rotation, and zonal winds. Such observations will be attempted with Voyager and potentially could be very fruitful in the Pioneer Venus and Galileo (Jupiter) orbiting missions.  相似文献   

Consistent fractionation of 13C in nature and in the laboratory: growth-rate effects in some haptophyte algae     

Bidigare RR  Fluegge A  Freeman KH  Hanson KL  Hayes JM  Hollander D  Jasper JP  King LL  Laws EA  Milder J  Millero FJ  Pancost R  Popp BN  Steinberg PA  Wakeham SG 《Global biogeochemical cycles》1997,11(2):279-292

The carbon isotopic fractionation accompanying formation of biomass by alkenone-producing algae in natural marine environments varies systematically with the concentration of dissolved phosphate. Specifically, if the fractionation is expressed by epsilon p approximately delta e - delta p, where delta e and delta p are the delta 13C values for dissolved CO2 and for algal biomass (determined by isotopic analysis of C37 alkadienones), respectively, and if Ce is the concentration of dissolved CO2, micromole kg-1, then b = 38 + 160*[PO4], where [PO4] is the concentration of dissolved phosphate, microM, and b = (25 - epsilon p)Ce. The correlation found between b and [PO4] is due to effects linking nutrient levels to growth rates and cellular carbon budgets for alkenone-containing algae, most likely by trace-metal limitations on algal growth. The relationship reported here is characteristic of 39 samples (r2 = 0.95) from the Santa Monica Basin (six different times during the annual cycle), the equatorial Pacific (boreal spring and fall cruises as well as during an iron-enrichment experiment), and the Peru upwelling zone. Points representative of samples from the Sargasso Sea ([PO4] < or = 0.1 microM) fall above the b = f[PO4] line. Analysis of correlations expected between mu (growth rate), epsilon p, and Ce shows that, for our entire data set, most variations in epsilon p result from variations in mu rather than Ce. Accordingly, before concentrations of dissolved CO2 can be estimated from isotopic fractionations, some means of accounting for variations in growth rate must be found, perhaps by drawing on relationships between [PO4] and Cd/Ca ratios in shells of planktonic foraminifera.  相似文献   

I/I ratios in Scottish coastal surface sea water: Geographical and temporal responses to changing emissions     

Christoph Schnabel  Valérie Olive  Mariko Atarashi-Andoh  Andrew Dougans  Robert M. Ellam  Stewart Freeman  Colin Maden  Martin Stocker  Hans-Arno Synal  Lukas Wacker  Sheng Xu 《Applied Geochemistry》2007

This work constitutes the first survey of I isotope ratios for Scottish sea water including the first data for the west of Scotland. These data are of importance because of the proximity to the world’s second largest emission source of ¹²⁹I to the sea, the Sellafield nuclear reprocessing plant, because of the increasing importance of the sea to land transfer of ¹²⁹I and also as input data for dose estimates based on this pathway of ¹²⁹I. ¹²⁹I/¹²⁷I ratios in SW Scotland reached 3 × 10⁻⁶ in 2004. No strong variation of I isotope ratios was found from 2003 to 2005 in Scottish sea waters. Iodine isotope ratios increased by about a factor of 6 from 1992 to 2003 in NE Scotland, in agreement with the increase of liquid ¹²⁹I emissions from Sellafield over that time period. It is demonstrated that ¹²⁹I/¹²⁷I ratios agree better than ¹²⁹I concentrations for samples from similar locations taken in very close temporal proximity, indicating that this ratio is more appropriate to interpret than the radionuclide concentration.  相似文献   

A decade of the Super Dual Auroral Radar Network (SuperDARN): scientific achievements, new techniques and future directions   总被引：2，自引：0，他引：2  

G. Chisham  M. Lester  S. E. Milan  M. P. Freeman  W. A. Bristow  A. Grocott  K. A. McWilliams  J. M. Ruohoniemi  T. K. Yeoman  P. L. Dyson  R. A. Greenwald  T. Kikuchi  M. Pinnock  J. P. S. Rash  N. Sato  G. J. Sofko  J.-P. Villain  A. D. M. Walker 《Surveys in Geophysics》2007,28(1):33-109

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南极格罗夫山火星陨石GRV 99027的宇宙射线暴露年龄     

孔屏  D. Fabel  R. Brown  S. Freeman 《中国科学D辑》2007,37(8):1020-1023

中国第16次南极考察队回收的GRV 99027的宇宙成因核素10Be和26Al的含量分别为(14.1±0.6)和(67.5±3.4) dpm/kg, 从10Be的含量计算出GRV 99027的宇宙线暴露年龄为(4.4±0.6) Ma, 而其过高的26Al的含量表明来自太阳射线的影响. 幔源火星陨石GRV 99027, LEW 88516, Y-793605, NWA 1950和ALHA77005具有非常相近的宇宙线暴露年龄, 再加上极为相似的矿物学和地球化学特征, 说明它们极有可能来自火星上的同一次撞击事件.  相似文献   

RAS helps to reconnect scientists     

Mervyn Freeman  Gareth Chisham  Iain Coleman  Mike Pinnock 《Astronomy& Geophysics》2003,44(3):3.33-3.34

Mervyn Freeman, Gareth Chisham, Iain Coleman and Mike Pinnock report on the November discussion meeting "Temporal and spatial structure of magnetic reconnection on the Earth's magnetopause", the only natural environment in which this universal astrophysical phenomenon can be observed locally and globally.  相似文献   

Kinematic reworking and exhumation within the convergent Alpine Orogen     

S.M. Reddy  J. Wheeler  R.W.H. Butler  R.A. Cliff  S. Freeman  S. Inger  C. Pickles  S.P. Kelley 《Tectonophysics》2003,365(1-4):77

Kinematic data from the internal zones of the Western Alps indicate both top-to-SE and top-to-NW shearing during synkinematic greenschist facies recrystallisation. Rb/Sr data from white micas from different kinematic domains record a range of ages that does not represent closure through a single thermal event but reflects the variable timing of synkinematic mica recrystallisation at temperatures between 300 and 450 °C. The data indicate an initial phase of accretion and foreland-directed thrusting at ca. 60 Ma followed by almost complete reworking of thrust-related deformation by SE-directed shearing. This deformation is localised within oceanic units of the Combin Zone and the base of the overlying Austroalpine basement, and forms a regional scale shear zone that can be traced for almost 50 km perpendicular to strike. The timing of deformation in this shear zone spans 9 Ma from 45 to 36 Ma. The SE-directed shear leads to local structures that cut upwards in the transport direction with respect to tectonic stratigraphy, and such structures have been interpreted in the past as backthrusts in response to ongoing Alpine convergence. However, on a regional scale, the top-to-SE deformation is related to crustal extension, not shortening, and is coincident with exhumation of eclogites in its footwall. During this extension phase, deformation within the shear zone migrated both spatially and temporally giving rise to domains of older shear zone fabrics intercalated with zones of localised reworking. Top-NW kinematics preserved within the Combin Zone show a range of ages. The oldest (48 Ma) may reflect the final stages of emplacement of Austroalpine Units above Piemonte oceanic rocks prior to the onset of extension. However, much of the top-to-NW deformation took place over the period of extension and may reflect either continuing or episodic convergence or tectonic thinning of the shear zone.⁴⁰Ar/³⁹Ar data from the region are complicated due to the widespread occurrence of excess ⁴⁰Ar in eclogite facies micas and partial Ar loss during Alpine heating. Reliable ages from both eclogite and greenschist facies micas indicate cooling ages in different tectonic units of between 32 and 40 Ma. These ages are slightly younger than Rb/Sr deformation ages and suggest that cooling below ca. 350 °C occurred after juxtaposition of the units by SE-directed extensional deformation.Our data indicate a complex kinematic history involving both crustal shortening and extension within the internal zones of the Alpine Orogen. To constrain the palaeogeographic and geodynamic evolution of the Alps requires that these data be integrated with data from the more external zones of the orogen. Complexity such as that described is unlikely to be restricted to the Western Alps and spatially and temporally variable kinematic data are probably the norm in convergent orogens. Recognising such features is fundamental to the correct tectonic interpretation of both modern and ancient orogens.  相似文献