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  • 1
    Keywords: Physics ; Physics ; Physics ; Physics, general
    Description / Table of Contents: Formation of molecules and dust -- Interpretation of the carbon recombination line -- The stellar population of dark clouds -- Observations of the H and C recombination lines toward NGC 2024 -- The ionization of carbon in dusty H I Regions -- Recent interstellar molecular line work -- A review of star formation -- Recent theoretical work on star formation -- Cocoon stars -- The early stages of HII regions -- Model calculations of dusty strömgren spheres -- Infrared observations of HII regions at ? 40 ?m OF compact HII regions -- Compact H II regions, mainly radio observations -- Selective absorption by dust in H II regions -- Optical studies of galactic nebulae and of their exciting stars : The role of dust on the radius of the ionized hydrogen sphere -- Molecular Masers in HII Regions -- Masers associated with galactic H II regions -- On the nature of the SiO maser in the Kleinmann-Low nebula -- Observed parameters of 0 type stars -- Recent optical observations of some evolved HII regions -- Evolved H II regions -- Radio continuum spectra -- Some recent calculations and computer programs -- Surveys of the galactic plane at 5 GHz. -- The galactic distribution of molecules (A CO survey) -- Radio observations of hii regions in external galaxies -- Optical observations of H II regions in external galaxies -- Ionized gas in NGC 4151 -- On the ionization conditions in the interarm gas of M 33 -- Observations of the excited hydrogen radio line H56? in several H II regions -- Far infrared observations of H II Regions -- Interstellar isotopic ratios, stellar mass losses and galactic evolution -- “Review” of Orion A and Orion B -- A new radio map of the core of Orion A -- M 17 -- DR21 and associated sources - A review -- The giant H 11 region w3 -- The W 49 region -- The W 51 source complex -- CO/ Dust ratio in the ? Ophiuchi complex -- 40-350 Micron emission from dust in NGC2023 -- The center of our galaxy -- The molecular cloud associated with SGR B2 -- High resolutions maps of the galactic center at 2.2 and 10 ? -- H II Regions in the nuclei of external galaxies -- The distribution of HII regions in the large magellanic cloud
    Type of Medium: Online Resource
    Pages: 1 Online-Ressource (XII, 493 p. 40 illus)
    Edition: Springer eBook Collection. Physics and Astronomy
    ISBN: 9783540379270 , 9783540074090
    Series Statement: Lecture Notes in Physics 42
    Language: English
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  • 2
    Online Resource
    Online Resource
    Berlin, Heidelberg :Springer Berlin / Heidelberg,
    Keywords: Astrophysics. ; Millimeter astronomy. ; Electronic books.
    Type of Medium: Online Resource
    Pages: 1 online resource (190 pages)
    Edition: 1st ed.
    ISBN: 9783662575468
    Series Statement: Saas-Fee Advanced Course Series ; v.38
    DDC: 523.01
    Language: English
    Note: Intro -- Preface -- Contents -- Introduction to Millimeter/ Sub-millimeter Astronomy -- 1 Introduction -- 2 Some Background -- 2.1 Radiative Transfer -- 2.2 Black Body Radiation and Brightness Temperature -- 2.3 The Nyquist Theorem and the Noise Temperature -- 3 Signal Processing and Stationary Stochastic Processes -- 3.1 Square Law Detectors -- 3.2 Limiting Receiver Sensitivity -- 4 Practical Receivers -- 4.1 Bolometer Radiometers -- 4.2 Currently Used Bolometer Systems -- 4.3 Coherent Receivers -- 4.4 HEMTs/MMICs -- 4.5 Back Ends: Spectrometers -- 4.6 Fourier, Autocorrelation and Cross Correlation Spectrometers -- 5 Filled Aperture Antennas -- 5.1 Angular Resolution -- 5.2 The Power Pattern P (, ) -- 5.3 The Main Beam Solid Angle -- 5.4 Effective Area -- 5.5 Antenna Feed Horns Used Today -- 5.6 Multiple Reflector Systems -- 5.7 Antenna Tolerance Theory -- 6 Single Dish Observational Methods -- 6.1 The Earth's Atmosphere -- 6.2 Millimeter and sub-mm Calibration Procedures -- 6.3 Continuum Observing Strategies -- 6.4 Additional Requirements for Spectral Line Observations -- 7 Interferometers and Aperture Synthesis -- 7.1 Two Element Interferometers -- 7.2 Responses of Interferometers -- 7.3 Aperture Synthesis -- 7.4 Interferometer Sensitivity -- 7.5 Advanced Image Improvement Methods -- 8 Continuum Emission from mm/sub-mm Sources -- 9 Spectral Line Basics -- 9.1 Radiative Transfer with Einstein Coefficients -- 9.2 Dipole Transition Probabilities -- 9.3 Simple Solutions of the Rate Equation -- 10 Line Radiation from Atoms -- 11 Emission Nebulae, Radio Recombination Lines -- 11.1 Rydberg Atoms -- 11.2 LTE Line Intensities -- 11.3 Non LTE Line Intensities -- 12 Overview of Molecular Basics -- 12.1 Basic Concepts -- 12.2 Rotational Spectra of Diatomic Molecules -- 12.3 Hyperfine Structure in Linear Molecules -- 12.4 Vibrational Transitions. , 12.5 Line Intensities of Linear Molecules -- 12.6 Symmetric Top Molecules -- 12.7 Asymmetric Top Molecules -- 12.8 Electronic Angular Momentum -- 13 Astronomical Applications -- 13.1 Kinetic Temperatures -- 13.2 Linewidths, Radial Motions and Intensity Distributions -- 13.3 Determinations of H2 Densities -- 13.4 Cloud Masses -- 13.5 Additional Topics -- References -- Star Formation with ALMA -- 1 Introduction -- 1.1 Why mm/sub-mm Astronomy for Star and Planet Formation? -- 2 Dust as a Probe of Star Formation -- 2.1 Size and Wavelength Dependence -- 2.2 Size Distribution -- 2.3 Dust Material Properties -- 2.4 Dust as a Mass Tracer -- 3 Using Molecules -- 3.1 Useful Simple Relations -- 4 Prestellar Cores -- 4.1 Using Dust -- 4.2 Geometry -- 4.3 Gas Temperature -- 4.4 Chemistry: Depletion and Fractionation -- 5 Class 0 -- 5.1 Infall Motions -- 5.2 Comparing with Models -- 6 Outflows -- 6.1 L1157 -- 6.2 Other Representative Cases -- 7 Protoplanetary Disks -- 7.1 Simplified Disk Parameters -- 7.2 Disk Parameters from Spectroscopic Observations -- 7.3 Continuum Emission -- 7.4 Model Dependencies -- 8 High-Mass Stars -- 8.1 Toroids and Outflows -- 8.2 Hot Cores -- 8.3 Molecular Complexity -- 9 Nonstandard Observations -- 9.1 Polarization -- 9.2 Time Dependent Effects -- 10 Conclusions: The Promise of ALMA -- References -- Index.
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  • 3
    Type of Medium: Book
    Pages: 21 S , Kt
    Series Statement: Cruise report / Institute of Oceanographic Sciences 169
    Language: English
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  • 4
    Type of Medium: Book
    Pages: 17 S , graph. Darst
    Series Statement: Cruise report / Institute of Oceanographic Sciences 160
    Language: English
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  • 5
    Type of Medium: Book
    Pages: III, 14 S , graph. Darst
    Series Statement: Cruise report / Institute of Oceanographic Sciences 138
    Language: English
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  • 6
    Type of Medium: Book
    Pages: 57 S , graph. Darst
    Series Statement: Report / Institute of Oceanographic Sciences Wormley, Godalming 175
    Language: English
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  • 7
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    PANGAEA
    In:  Supplement to: Wilson, T R S; Miles, D L (1987): On the utility of chemical data for the detection of vertical pore-water movement in marine sediments. In: Ruddiman, WF; Kidd, RB; Thomas, E; et al. (eds.), Initial Reports of the Deep Sea Drilling Project, Washington (U.S. Govt. Printing Office), 94, 1145-1148, https://doi.org/10.2973/dsdp.proc.94.144.1987
    Publication Date: 2023-06-27
    Description: The suggestion that nuclear waste material might be buried within the sediments of the deep ocean has increased interest in possible ways that vertical pore-water movement might be detected and measured. A heat-flow station (Discovery 10335) previously occupied near Kings Trough indicated nonlinear temperature-depth profiles in the surficial sediments, which could be interpreted in terms of a very high upward pore-water velocity. The calcium and magnesium pore-water profiles at Site 608, however, prove to be unusually linear and show a strong inverse correlation with each other. In these circumstances it is very unlikely that vertical pore-water movements have occurred, and the application of a simple model indicates that, given the assumptions of this model, the vertical pore-water advection velocity has been zero ± 0.006 cm yr**-1. for a substantial fraction of the recent sedimentological history of this area.
    Keywords: 94-608; Calcium; Deep Sea Drilling Project; DEPTH, sediment/rock; DRILL; Drilling/drill rig; DSDP; Glomar Challenger; Leg94; Magnesium; North Atlantic/FLANK
    Type: Dataset
    Format: text/tab-separated-values, 30 data points
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  • 8
    Publication Date: 2017-04-03
    Description: Fractures in AND-2A drillcore were documented in this study. Over 4100 fractures of all types were logged. A population of 510 steeply-dipping, petal, petal-centreline and core-edge induced fractures is present, reaching a maximum density of c. 10 fractures/metre. Subhorizontal induced extension fractures are also abundant. There are 1008 natural fractures in the core, including faults, brecciated zones, veins and sedimentary intrusions. Kinematic indicators document dominant normal faulting, although reverse faults are also present. The natural fractures occur in strata ranging in age from the Miocene to the Plio-Pleistocene.
    Description: Published
    Description: 69-76
    Description: 3.2. Tettonica attiva
    Description: N/A or not JCR
    Description: open
    Keywords: Fractures ; Downhole logging ; Drillcore ; Stress ; Antarctica ; Drilling ; 04. Solid Earth::04.02. Exploration geophysics::04.02.05. Downhole, radioactivity, remote sensing, and other methods ; 04. Solid Earth::04.04. Geology::04.04.09. Structural geology ; 04. Solid Earth::04.07. Tectonophysics::04.07.99. General or miscellaneous ; 04. Solid Earth::04.07. Tectonophysics::04.07.05. Stress ; 04. Solid Earth::04.07. Tectonophysics::04.07.07. Tectonics
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 9
    Publication Date: 2017-04-03
    Description: Under the framework of the ANDRILL Southern McMurdo Sound (SMS) Project successful downhole experiments were conducted in the 1138.54 metre (m)-deep AND-2A borehole. Wireline logs successfully recorded were: magnetic susceptibility, spectral gamma ray, sonic velocity, borehole televiewer, neutron porosity, density, calliper, geochemistry, temperature and dipmeter. A resistivity tool and its backup both failed to operate, thus resistivity data were not collected. Due to hole conditions, logs were collected in several passes from the total depth at ~1138 metres below sea floor (mbsf) to ~230 mbsf, except for some intervals that were either inaccessible due to bridging or were shielded by the drill string. Furthermore, a Vertical Seismic Profile (VSP) was created from ~1000 mbsf up to the sea floor. The first hydraulic fracturing stress measurements in Antarctica were conducted in the interval 1000-1138 mbsf. This extensive data set will allow the SMS Science Team to reach some of the ambitious objectives of the SMS Project. Valuable contributions can be expected for the following topics: cyclicity and climate change, heat flux and fluid flow, seismic stratigraphy in the Victoria Land Basin, and structure and state of the modern crustal stress field.
    Description: Published
    Description: 57-68
    Description: 3.2. Tettonica attiva
    Description: N/A or not JCR
    Description: restricted
    Keywords: Downhole measurements ; Borehole ; Vertical Seismic Profile ; Hydraulic Fracturing ; Antarctica ; 04. Solid Earth::04.02. Exploration geophysics::04.02.99. General or miscellaneous ; 04. Solid Earth::04.02. Exploration geophysics::04.02.05. Downhole, radioactivity, remote sensing, and other methods ; 04. Solid Earth::04.02. Exploration geophysics::04.02.07. Instruments and techniques ; 04. Solid Earth::04.04. Geology::04.04.99. General or miscellaneous ; 04. Solid Earth::04.07. Tectonophysics::04.07.99. General or miscellaneous ; 04. Solid Earth::04.07. Tectonophysics::04.07.05. Stress ; 04. Solid Earth::04.07. Tectonophysics::04.07.07. Tectonics
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: article
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  • 10
    Publication Date: 2017-04-03
    Description: To define the present-day stress field in the upper crust and to understand the recent tectonic activity in Antarctica, a study of breakout measurements along AND-2A well was performed. The borehole breakout is an important indicator of horizontal stress orientation and occurs when the stresses around the borehole exceed that required to cause compressive failure of the borehole wall (Bell and Gough, 1979; Zoback et al., 1985, Bell, 1990). The enlargement of the wellbore is caused by the development of intersecting conjugate shear planes that cause pieces of the borehole wall to spall off. Around a vertical borehole, stress concentration is greatest in the direction of the minimum horizontal stress (Shmin), hence, the long axes of borehole breakouts are oriented approximately perpendicular to the maximum horizontal stress orientation (SHmax). The orientation of breakouts along the AND-2A well was measured using acoustic (BHTV) and mechanical (Four-Arm Caliper) tools. Borehole televiewer (BHTV) provides an acoustic "image" of the borehole wall (360 degree coverage) and gives detailed information for investigation of fractures and stress analysis. The four-arm caliper is the oldest technique for borehole breakout identification and it is included in routine dipmeter logs. A quality value has been assigned to the well results in agreement with the World Stress Map quality ranking scheme (Zoback, 1992; Heidback et al., 2010) based mainly on the number, accuracy, and length of breakout measurements. The result is presented as rose diagram of the breakout directions where the length of each peak is proportional to the frequency and the width to the variance of its gaussian curve. We have analyzed the following curves to recognize the breakout: the azimuth of Pad 1 (P1az), the drift azimuth (HAZI), the two calipers with respect to the bit size (BZ) curve and the curve relative to the deviation of the well. The AND-2A Four-Arm Caliper data cover a depth interval between 637 down to 997 mbsl, that corresponds to 360 m of logged interval. We have distinguished breakouts and some washouts only in the interval from 753 to 825 mbsl. From borehole televiewer images, we have data from 398 mbsl down to 1136 mbsl. The BHTV worked well showing a lot of interesting features such as many bedding, lamination and fractures (natural and induced) but poor breakouts. The rare breakouts have also a small size (called protobreakouts) but they are consistent with induced features. Considering the breakout result from caliper and BHTV, the AND-2A borehole is unfortunately classified as D quality. This means that to obtain a reliable active stress field of the area it is necessary to compare this result with other available data.
    Description: Unpublished
    Description: San Francisco (California, USA)
    Description: 3.2. Tettonica attiva
    Description: open
    Keywords: Borehole breakout ; Stress analysis ; 04. Solid Earth::04.02. Exploration geophysics::04.02.05. Downhole, radioactivity, remote sensing, and other methods ; 04. Solid Earth::04.07. Tectonophysics::04.07.05. Stress ; 04. Solid Earth::04.07. Tectonophysics::04.07.07. Tectonics
    Repository Name: Istituto Nazionale di Geofisica e Vulcanologia (INGV)
    Type: Poster session
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