Iowa catalog of solar X-ray flux (2–12 Å)

The absolute X-ray flux from the whole disc of the sun in the wave length range 2 to 12 Å has been observed for a prolonged period by University of Iowa equipment on the earth-orbiting satellite Explorer 33 and the moon-orbiting satellite Explorer 35, both of the Goddard Space Flight Center of the National Aeronautics and Space Administration. The observations are continuing at the date of writing (July 1969). A comprehensive catalog of the flux F (2–12 Å) is being produced. The observational technique and the scheme of reducing data are described herein. Sample tabulations and plots are given. A catalog of tabular and graphical data with a time resolution of either 81.8 or 163.6 sec has been completed for the following periods: From Explorer 33: 2 July 1966 to 27 July 1967 From Explorer 35: 26 July 1967 to 18 September 1968 These blocks of data have been delivered to the National Space Science Data Center National Aeronautics and Space Administration Goddard Space Flight Center Greenbelt, Maryland 20771, U.S.A. and made available through that agency to interested workers in solar and ionospheric physics. Further blocks of data will be made available as they are completed. An abridged summary of principal flares is published in the monthly Solar-Geophysical Data of the U.S. Department of Commerce, Environmental Science Services Administration.     

Note on the extreme values of the earth-moon distance

The extreme Earth-Moon distances during the period 1970–1979 are given. Some values stated by Gupta (1975) are incorrect.     

A linear approximation to the solution of a one-dimensional Stefan problem and its geophysical implications

Summary. The motion of a phase boundary in the Earth caused by temperature and pressure excitations at the Earth's surface is determined under a linear approximation. The solution is found as a sum of convolutions of pressure and temperature Green's functions with the corresponding excitations. The Green's functions are given under the form of Laplace transforms that can be inverted either by numerical evaluation of a branch cut integral or by inversion of a series expansion. This solution is a generalization of a solution previously derived by Gjevik. This latter solution is the first term in the series expansion. The relaxation times associated with the phase boundary motion are of the order of 10⁵–10⁷yr for the olivine—spinel phase transition and of 10⁶–10⁷yr for the basalt—eclogite transition. The linear approximation remains valid for long times only if the phase boundary moves slowly.     

Strengthen the Environmental Sense of Local Community with PRA and MIGIS

Foundation item: The Project entitled "A Feasibility Study to Strengthen Participatory Planning Capacity by MIGIS" supported by Asian Development Assistance Facility (ADAF), Ministry of Foreign Affairs and Trade. New ZealandAlthough the govenunent has paid great attenhon to the environmental improvement by means of policyand inVestment the environmental condihon is aill getting worse in C~ The current environmentalsitUation is chalacterized by serious POlluhoft expanded land degra…     

Holocene Climate Variability in Antarctica Based on 11 Ice-Core Isotopic Records

A comparison is made of the Holocene records obtained from water isotope measurements along 11 ice cores from coastal and central sites in east Antarctica (Vostok, Dome B, Plateau Remote, Komsomolskaia, Dome C, Taylor Dome, Dominion Range, D47, KM105, and Law Dome) and west Antarctica (Byrd), with temporal resolution from 20 to 50 yr. The long-term trends possibly reflect local ice sheet elevation fluctuations superimposed on common climatic fluctuations. All the records confirm the widespread Antarctic early Holocene optimum between 11,500 and 9000 yr; in the Ross Sea sector, a secondary optimum is identified between 7000 and 5000 yr, whereas all eastern Antarctic sites show a late optimum between 6000 and 3000 yr. Superimposed on the long time trend, all the records exhibit 9 aperiodic millennial-scale oscillations. Climatic optima show a reduced pacing between warm events (typically 800 yr), whereas cooler periods are associated with less-frequent warm events (pacing >1200 yr).     

GeoPT5. An International Proficiency Test for Analytical Geochemistry Laboratories - Report on Round 5

Results are presented from the seventy two laboratories participating in GeoPT5, round five of the international proficiency testing programme for analytical geochemistry laboratories. The sample for round five, AMH-1 (Mount Hood andesite), was distributed during March 1999 and participating laboratories were asked to analyse the sample using their routine techniques and submit results to the steering by 15th June 1999. In this report, contributed data are listed together with the derived z-scores from which participating laboratories can assess their analytical performance. Z-scores in the range -2 to 2 are considered satisfactory. Z-score values that lie outside this range may indicate unsuspected analytical bias. The distinctive feature of the present round is that AMH-1 is a candidate reference material prepared by the USGS and it is intended that the present proficiency testing data will contribute to the reference material characterisation programme.     

The environmental setting of the harbor of the classical site of Oeniades on the Acheloos delta,Greece

Using a multidisciplinary approach, the Holocene geomorphological and palaeoenvironmental dynamics of the Acheloos delta were studied in order to understand how the ancient port of Oeniades, today situated 5 km from the sea, was connected to the sea in ancient times. A study of ancient maps, aerial photographs, and a SPOT image enabled us to reconstitute the successive changes in the flow of the Acheloos River and to conclude that, contrary to the traditional thesis of historians and archeologists, the harbor of Oeniades was completely independent from the river during Antiquity. Multidisciplinary studies (sedimentology, malacology, palynol‐ogy, and radiocarbon dating) were carried out on sediments from two boreholes (OEN1 and OEN2). Results show that the port of Oeniades communicated directly with an open bay that was created at the peak of the last post‐glacial transgression. The bay was gradually filled with sediments, allowing human occupation of the area to progress. © 2005 Wiley Periodicals, Inc.     

Imaging of the protoelliptical NGC 1700 and its globular cluster system

An excellent candidate for a young elliptical, or 'protoelliptical' galaxy is NGC 1700. Here we present new B -, V - and I -band imaging using the Keck telescope, and reanalyse existing V - and I -band images from the Hubble Space Telescope . After subtracting a model of the galaxy from the Keck images, NGC 1700 reveals two symmetric tidal tail-like structures. If this interpretation is correct, it suggests a past merger event involving two spiral galaxies. These tails are largely responsible for the 'boxiness' of the galaxy isophotes observed at a radius of ∼13 kpc.
We also show that the B − I colour distribution of the globular cluster system is bimodal. The mean colour of the blue population is consistent with that of old Galactic globular clusters. Relative to this old, metal-poor population, we find that the red population is younger and more metal-rich. This young population has an age and metallicity similar to that inferred for the central stars, suggesting that both populations are associated with an episode of star formation triggered by the merger that may have formed the galaxy. We find that, although they have large errors, the majority of the age estimates of NGC 1700 are reasonably consistent and we adopt a 'best estimate' for the age of 3.0±1.0 Gyr. This relatively low age places NGC 1700 within the age range where there is a notable lack of obvious candidates for protoellipticals. The total globular cluster specific frequency is rather low for a typical elliptical, even after taking into account the fading of the galaxy over the next 10 Gyr. We speculate that NGC 1700 will eventually form a relatively 'globular cluster poor' elliptical galaxy.