The center-to-limb behavior of Ca i λ6573 and [Ca ii] λ7324     

T. R. Ayres  L. Testerman 《Solar physics》1978,60(1):19-29

Center-to-limb measurements of the Ca i 6573 intercombination line and the Ca ii 7324 forbidden line are compared with synthetic profiles based on a simple representation of the non-LTE Ca-Ca⁺ ionization equilibrium. The effects of photoionizations from low lying excited states of neutral calcium are found to reduce the sensitivity of the 6573 center-to-limb behavior as a thermal structure diagnostic. The synthetic center-to-limb behavior is also sensitive to uncertainties in the nonthermal broadening. Nevertheless, the measured center-to-limb behavior of 6573 favors a cool photospheric model similar to the Vernazza, Avrett, and Loeser model M over hotter models based on the Ca ii K wings. The non-LTE calcium abundance obtained from the disk center equivalent widths of 6573 and 7324 using the best fit model is A _Ca2.1±0.2 × 10^-6 (by number relative to hydrogen). Applications of these lines as diagnostics of the Ca-Ca⁺ ionization equilibrium in other stars are briefly discussed.Visiting Astronomer, Kitt Peak National Observatory.Operated by the Association of Universities for Research in Astronomy, Inc. under contract with the National Science Foundation.  相似文献   

Scientific problems addressed by the Spektr-UV space project (world space Observatory—Ultraviolet)     

A. A. Boyarchuk  B. M. Shustov  I. S. Savanov  M. E. Sachkov  D. V. Bisikalo  L. I. Mashonkina  D. Z. Wiebe  V. I. Shematovich  Yu. A. Shchekinov  T. A. Ryabchikova  N. N. Chugai  P. B. Ivanov  N. V. Voshchinnikov  A. I. Gomez de Castro  S. A. Lamzin  N. Piskunov  T. Ayres  K. G. Strassmeier  S. Jeffrey  S. K. Zwintz  D. Shulyak  J.-C. Gérard  B. Hubert  L. Fossati  H. Lammer  K. Werner  A. G. Zhilkin  P. V. Kaigorodov  S. G. Sichevskii  S. Ustamuich  E. N. Kanev  E. Yu. Kil’pio 《Astronomy Reports》2016,60(1):1-42

The article presents a review of scientific problems and methods of ultraviolet astronomy, focusing on perspective scientific problems (directions) whose solution requires UV space observatories. These include reionization and the history of star formation in the Universe, searches for dark baryonic matter, physical and chemical processes in the interstellar medium and protoplanetary disks, the physics of accretion and outflows in astrophysical objects, from Active Galactic Nuclei to close binary stars, stellar activity (for both low-mass and high-mass stars), and processes occurring in the atmospheres of both planets in the solar system and exoplanets. Technological progress in UV astronomy achieved in recent years is also considered. The well advanced, international, Russian-led Spektr-UV (World Space Observatory—Ultraviolet) project is described in more detail. This project is directed at creating a major space observatory operational in the ultraviolet (115–310 nm). This observatory will provide an effective, and possibly the only, powerful means of observing in this spectral range over the next ten years, and will be an powerful tool for resolving many topical scientific problems.  相似文献   

Unscrambling the stratigraphy of an Archean greenstone belt; a U---Pb geochronological study of the Favourable Lake belt, northwestern Ontario, Canada     

F Corfu  L.D Ayres 《Precambrian Research》1991,50(3-4)

New zircon and baddeleyite U---Pb ages show that the major units of the Archean Favourable Lake greenstone belt in the northern Superior Province were formed by episodic magmatism spanning more than 250 Ma and demonstrate that the original stratigraphy is disrupted by thrusts that juxtaposed older supracrustal rocks on top of younger ones. The oldest rocks of the area are a 2950 Ma gneissic tonalite and a 3000-2960 Ma granodiorite clast from a ca. 2725 Ma conglomerate. Five distinct volcanic (and sedimentary) groups formed during presumably short-lived episodes at 2925 Ma (I), 2870 Ma (II), 2858 Ma (III), 2734 Ma (IV), and 2725 Ma (V). The youngest group contains the thickest sedimentary unit, a turbiditic and alluvial-fluvial sequence. Compression caused thrusting that placed Groups I and V on top of IV, III on V, and II on III. The thrust complex was subsequently isoclinally folded. Compression was accompanied by major plutonism that emplaced the bulk of the bounding batholiths between 2732 and 2711 Ma ago. The late tectonic, Mo-mineralized Setting Net Lake Stock in the centre of the belt has an age of about 2708 Ma and was overprinted by younger hydrothermal events that produced monazite (2706 Ma), titanite (ca. 2695-2690 Ma) and rutile (the youngest rutile at 2657 Ma). Similar late hydrothermal pulses are recorded by secondary titanite elsewhere in the belt and within the batholiths. The protracted magmatic evolution of the belt is typical of that observed in a number of greenstone belts of the northern Superior Province but is uncommon farther to the south. In contrast, the structural complications and put-of-sequence stratigraphy appear to be a quite common tectonic characteristic of greenstone belts of the whole Superior Province.  相似文献   

Early Proterozoic,basaltic andesite tuff-breaccia: downslope,subaqueous mass transport of phreatomagmatically-generated tephra     

MB Dolozi  LD Ayres 《Bulletin of Volcanology》1991,53(6):477-495

At Bear Lake, in the Flin Flon-Snow Lake greenstone belt of Manitoba, 400⁺ m of thick-to very thick-bedded, generally ungraded, basaltic andesite tuff-breccia, breccia, and lapilli-tuff are intercalated with pillowed lava flows in the upper part of an early Proterozoic submarine basaltic andesite shield volcano. The fragmental rocks comprise angular, amygdaloidal blocks and lapilli, many with partial chilled selvages, in a matrix of blocky, non-amygdaloidal to highly amygdaloidal vitric basaltic andesite ash and small lapilli. Minor thin-to medium-bedded, commonly normally graded tuff occurs in the upper part of the sequence. Clasts in fragmental beds consistently have higher amygdule contents than intercalated lava flows. Although similar to pillow-fragment breccias, the Bear Lake fragmental rocks were produced by extended surtseyan-type, phreatomagmatic eruptions, with associated fire fountain activity, at a progressively subsiding, shallow water vent. Periodic tephra slumping generated debris flows that transported particles down the uppe, gentle slope of the volcano to a depositional site at a water depth of less than 1 km. Turbidity currents probably carried much fine tephra to deeper water; tuff was deposited in the preserved section only after explosive volcanism ceased.  相似文献   

U-Pb age and genetic significance of heterogeneous zircon populations in rocks from the Favourable Lake area,Northwestern Ontario     

F. Corfu  L. D. Ayres 《Contributions to Mineralogy and Petrology》1984,88(1-2):86-101

The study evaluates the relationships between measured U-Pb ages and zircon characteristics of five morphologically, texturally, and isotopically complex zircon populations and compares the zircon development stages to the orogenic evolution of the Favourable Lake area. Two distinct zircon types from a hornblendite xenolith in a granitoid batholith of the Sachigo subprovince of the Superior Province yield U-Pb ages of 2729.0±6.8 Ma and 2714.8 _–6.4 ^+7.4 Ma, which date specific metamorphic phases coinciding with major plutonic pulses in the batholith. Zircons from a metamorphosed felsic dike, crosscutting the hornblendite, consist of an old zircon component with a minimum age of 2788 Ma possibly reflecting igneous crystallization 2950 Ma ago, and a younger component with an inferred age of 2725±15 Ma, probably reflecting metamorphism during batholith emplacement.In the Berens River subprovince to the south, granodiorite forms both a late tectonic phase in a large batholith and a post-tectonic pluton intruded into the batholith, yet zircons from these granodiorites have identical ages of 2697.3±1.7 Ma and 2696.2±1.2 Ma, respectively. The late tectonic granodiorite also contains inherited zircons with a minimum age of 2767 Ma which are indirect evidence for the presence of old sialic crust in this subprovince. Zircons from a sheared monzonite near the boundary fault between the two subprovinces yield an upper intercept age of 2769 _–26 ⁺⁶³ Ma, which we interpret as the intrusion age of the monzonite. This rock is older than most dated units in the surrounding batholiths and suggests that the boundary is a long-lived Archean structure.A lower intercept age of about 1750 Ma for zircons of the hornblendite is the result of chemical alteration of the zircons. This, and a similar lower intercept age shown by the sheared monzonite zircons, are thought to reflect increased fluid activity and possibly shearing during the Early Proterozoic Hudsonian orogeny which occurred in the Churchill Province to the northwest. A later Pb-loss mainly from near-surface domains of the zircons is indicated by lower intercept ages of about 500–100 Ma.Publication approved by the Director, Ontario Geological Survey  相似文献   

Creating a global warming implementation regime     

LD Danny Harvey 《Global Environmental Change》1995,5(5)

This paper proposes a global warming implementation regime which addresses the issues of equity, flexibility, cost minimization, and population growth. Previously proposed international policy instruments, such as country by country targets, carbon taxes, and tradable permits, face major difficulties as stand alone proposals. The key element of the regime proposed here is to combine annual tradable permits which are allocated based on population in a fixed year with a small carbon tax ($5–10/tonne) on emissions in excess of permits. Both permits and carbon taxes are applied to national level governments, which in turn would use whatever mix of policies desired to reduce national emissions. It is suggested that the initial number of permits correspond to total global emissions in the base year; over time, the number of permits could be reduced and the tax rate increased if improved scientific knowledge so dictates. By allocating permits based on population the equity concerns of developing countries are addressed, while taxing emissions in excess of permit holdings removes the rigidity of a quota system and limits resource transfers by effectively capping the permit trading price, which is a major concern of industrialized countries. To accommodate the difficulties of countries which have not yet achieved the demographic transition, the permit allocation scheme could be subject to a one-time adjustment after 10–15 years based on some weighting of the initial and then-current populations. The proposed scheme is based on the premise that there is a large potential for reducing emissions in developed countries or limiting emission increases in developing countries, and the intention is to create competition between national level governments in implementing cost-effective emission reduction.  相似文献   

Toxins in the red Whelk     

P.A. Ayres  P.C. Wood 《Marine pollution bulletin》1973,4(10):157-159

A case of poisoning following consumption of Neptunea occurred in Scotland in 1970. The organism is caught in traps with the Edible Whelk where it constitutes less than 0·5% of the catch. Toxin in the salivary gland demonstrated by mouse bioassay could be distinguished from PSP toxin. It is concluded that the public health risk from consumption of the Edible Whelk is negligible.  相似文献   

Does H− truly cool the solar chromosphere?     

Thomas R. Ayres 《Solar physics》1980,68(1):125-133

I examine the controversial problem of H^– radiative cooling in the solar chromosphere. I find, in agreement with Praderie and Thomas, that H^– is a substantial source of radiative heating in the outer atmosphere, especially when departures from LTE are important. The role of H^– as a chromospheric heating agent must be considered carefully before net radiative cooling rates can be assessed from empirical chromospheric models, or calculations of nonradiative heating, for example by acoustic waves, can be pursued meaningfully.  相似文献   

The SOHO–Stellar Connection     

Ayres  Thomas R. 《Solar physics》2000,193(1-2):273-297

The solar–stellar connection bridges the daytime and nighttime communities; an essential link between the singular, but detailed, views of our Sun, and the broad, but coarse, glimpses of the distant stars. One area in particular – magnetic activity – has profited greatly from the two way traffic in ideas. In that spirit, I present an evolutionary context for coronal activity, focusing on the very different circumstances of low-mass main-sequence stars like the Sun, compared with more massive stars. The former are active mainly very early in their lives, whereas the latter become coronal only near the end of theirs, during the brief incursion into the cool half of the Hertzsprung–Russell diagram as yellow, then red, giants. I describe tools at the disposal of the stellar astronomer; especially spectroscopy in the ultraviolet and X-ray bands where coronae leave their most obvious imprints. I compare HST STIS spectra of solar-type dwarfs – Dor (F7 V), an active coronal source, and Cen A (G2 V), near twin of the Sun – to the SOHO SUMER UV solar atlas. I also compare the STIS line profiles of the active coronal dwarf to the corresponding features in the mixed activity hybrid chromosphere bright giant TrA (K2 II) and the archetype non-coronal red giant Arcturus ( Boo; K2 III). The latter shows dramatic evidence for a cool absorber in its outer atmosphere that is extinguishing the hot lines (like Siiv 1393 and Nv 1238) below about 1500 Å; the corona of the red giant seems to lie beneath its extended chromosphere, rather than outside as in the Sun. I present an early taste of the moderate resolution spectra we can expect from the recently launched Chandra X-ray Observatory (CXO), and contemporaneous STIS high resolution UV measurements of the CXO calibration star Capella ( Aur; G8 III + G1 III). Last, I describe preliminary results from a May 1999 observing campaign involving SOHO SUMER, TRACE, and the Kitt Peak Infrared Imaging Spectrometer (IRIS). The purpose was to explore the dynamics of the quiet solar atmosphere through the key magnetic transition zone that separates the kinetically dominated deep photosphere from the magnetically dominated coronal regime. Linking spatially and temporally resolved solar phenomena to properties of the average line shapes (widths, asymmetries, intensity ratios, and Doppler shifts) is a crucial step in carrying physical insights from the solar setting to the realm of the distant stars.  相似文献   

The use of faecal bacteria as a tracer for sewage sludge disposal in the sea     

P. A. Ayres 《Marine pollution bulletin》1977,8(12):283-285

Samples of bottom sediment taken in an area used for marine dumping of sewage sludge were examined for the presence of Escherichia coli and coliform bacteria. Using a simple membrane filtration technique, an extensive network of stations was sampled and examined at sea in under two days. The results obtained were in good agreement with seabed drifter and radioactive tracer studies, and suggest that the use of bacterial indices may be a useful means of estimating the distribution of sewage sludge solids in bottom sediments.  相似文献