GHY101 Unit 2.4 Australia & New Zealand

•Download as PPTX, PDF•

1 like•74 views

Slideshow on "Australia & New Zealand" for World Regional Geography - © Mark M. Miller, Dept. of Geography & Geology, The University of Southern Mississippi

Science

YouTube. Rabbit Proof Fence (1). Retrieved September 19,
2011: http://www.youtube.com/watch?v=DdFNZSx6hSQ
Australia & New Zealand
© Mark M. Miller
The University of Southern Mississippi
World Regional Geography

Amoeba blog. Retrieved February 14, 2012:
http://www.amoeba.com/blog/2008/01/eric-s-
blog/happy-australia-day.html

Mijiza’s. Retrieved September 20,
2010:
http://deborahmazon.wordpress.co
m/category/history/oceania/page/2
/
Aborigine

Retrieved September 20, 2010:
http://www.remotetribes.com/maori-tribe/
Maori

YouTube. Rabbit Proof Fence (1). Retrieved September 19,
2011: http://www.youtube.com/watch?v=DdFNZSx6hSQ

Strange Maps. Retrieved January 30, 2010: http://strangemaps.wordpress.com/

Map from the 1920s. Strange
Maps. Retrieved October 24,
2010:
http://bigthink.com/blogs/strang
e-maps

Oregon Press Register. Retrieved 10/27/06:
http://www.newsregister.com/photos/upload/2005042815445
4_medium.jpg
Immigration

Embassy in Washington: http://www.nzembassy.com/usa

Australia’s Herald Sun: http://www.heraldsun.com.au
New Zealand Herald: http://www.nzherald.co.nz/

New Zealand Tourism: http://www.newzealand.com

Recently uploaded

Nanoparticles synthesis and characterization

kaibalyasahoo82800

Understanding circumstellar disks is of prime importance in astrophysics, however, their birth process remains poorly constrained due to observational and numerical challenges. Recent numerical works have shown that the small-scale physics, often wrapped into a sub-grid model, play a crucial role in disk formation and evolution. This calls for a combined approach in which both the protostar and circumstellar disk are studied in concert. Aims. We aim to elucidate the small scale physics and constrain sub-grid parameters commonly chosen in the literature by resolving the star-disk interaction. Methods. We carry out a set of very high resolution 3D radiative-hydrodynamics simulations that self-consistently describe the collapse of a turbulent dense molecular cloud core to stellar densities. We study the birth of the protostar, the circumstellar disk, and its early evolution (< 6 yr after protostellar formation). Results. Following the second gravitational collapse, the nascent protostar quickly reaches breakup velocity and sheds its surface material, thus forming a hot (∼ 103 K), dense, and highly flared circumstellar disk. The protostar is embedded within the disk, such that material can flow without crossing any shock fronts. The circumstellar disk mass quickly exceeds that of the protostar, and its kinematics are dominated by self-gravity. Accretion onto the disk is highly anisotropic, and accretion onto the protostar mainly occurs through material that slides on the disk surface. The polar mass flux is negligible in comparison. The radiative behavior also displays a strong anisotropy, as the polar accretion shock is shown to be supercritical whereas its equatorial counterpart is subcritical. We also f ind a remarkable convergence of our results with respect to initial conditions. Conclusions. These results reveal the structure and kinematics in the smallest spatial scales relevant to protostellar and circumstellar disk evolution. They can be used to describe accretion onto regions commonly described by sub-grid models in simulations studying larger scale physics.

Formation of low mass protostars and their circumstellar disks

Sérgio Sacani

GBSN - Microbiology (Unit 1)

Areesha Ahmad

Pulmonary drug delivery system M.pharm -2nd sem P'ceutics

sakshisoni2385

Chemical Tests; flame test, positive and negative ions test Edexcel Internati...

ssuser79fe74

Biopesticide (2).pptx .This slides helps to know the different types of biop...

RohitNehra6

A botany file is similar to a chemistry practical file but specifically focuses on experiments and observations related to plants. It typically includes detailed descriptions of plant-related experiments, such as germination studies, growth experiments, tissue culture techniques, plant anatomy investigations, and ecological surveys. The file may contain records of plant specimens collected, their classification, characteristics, and ecological significance. Additionally, it may include diagrams, photographs, drawings, tables, and data analysis related to plant research. Like a chemistry practical file, a botany file serves as a documentation of practical work conducted in the field of botany and is often used for assessment and educational purposes.

Botany 4th semester file By Sumit Kumar yadav.pdf

Sumit Kumar yadav

Presentation Vikram Lander by Vedansh Gupta.pptx

gindu3009

COST ESTIMATION FOR A RESEARCH PROJECT.pptx

FarihaAbdulRasheed

Biological Classification BioHack (3).pdf

muntazimhurra

CELL -Structural and Functional unit of life.pdf

Nistarini College, Purulia (W.B) India

The presentation first gives the brief introduction about the animal communication covering the reasons for communication. It then describes the important types of animal communication emphasizing the important points regarding auditory and visual communication. With respect to auditory communication, it covers the uses of it and mechanisms of auditory communication along with examples. Later the presentation discusses the various forms of visual communication such as gestures, postures, facial expressions, color changes , bioluminescent communication. It then describes the visual communication in bees in the form of bee dance . In bee dance it gives a brief overview of round dance , sickle dance and waggle dance .

Animal Communication- Auditory and Visual.pptx

UmerFayaz5

Creating and Analyzing Definitive Screening Designs

NurulAfiqah307317

Jupiter’s moon Io hosts extensive volcanism, driven by tidal heating. The isotopic composition of Io's inventory of volatile chemical elements, including sulfur and chlorine, reflects its outgassing and mass loss history, and thus records information about its evolution. We used millimeter observations of Io’s atmosphere to measure sulfur isotopes in gaseous SO2 and SO, and chlorine isotopes in gaseous NaCl and KCl. We find 34S/32S = 0.0595 ± 0.0038 (equivalent to δ34S = +347 ± 86‰), which is highly enriched compared to average Solar System values and indicates that Io has lost 94 to 99% of its available sulfur. Our measurement of 37Cl/35Cl = 0.403 ± 0.028 (δ37Cl = +263 ± 88‰) shows that chlorine is similarly enriched. These results indicate that Io has been volcanically active for most (or all) of its history, with potentially higher outgassing and mass-loss rates at earlier times.

Isotopic evidence of long-lived volcanism on Io

Sérgio Sacani

Theoretical predictions and observational data indicate a class of sub-Neptune exoplanets may have water-rich interiors covered by hydrogen-dominated atmospheres. Provided suitable climate conditions, such planets could host surface liquid oceans. Motivated by recent JWST observations of K2-18 b, we self-consistently model the photochemistry and potential detectability of biogenic sulfur gases in the atmospheres of temperate sub-Neptune waterworlds for the first time. On Earth today, organic sulfur compounds produced by marine biota are rapidly destroyed by photochemical processes before they can accumulate to significant levels. Domagal-Goldman et al. suggest that detectable biogenic sulfur signatures could emerge in Archean-like atmospheres with higher biological production or low UV flux. In this study, we explore biogenic sulfur across a wide range of biological fluxes and stellar UV environments. Critically, the main photochemical sinks are absent on the nightside of tidally locked planets. To address this, we further perform experiments with a 3D general circulation model and a 2D photochemical model (VULCAN 2D) to simulate the global distribution of biogenic gases to investigate their terminator concentrations as seen via transmission spectroscopy. Our models indicate that biogenic sulfur gases can rise to potentially detectable levels on hydrogen-rich water worlds, but only for enhanced global biosulfur flux (20 times modern Earth’s flux). We find that it is challenging to identify DMS at 3.4 μm where it strongly overlaps with CH4, whereas it is more plausible to detect DMS and companion byproducts, ethylene (C2H4) and ethane (C2H6), in the mid-infrared between 9 and 13 μm. Unified Astronomy Thesaurus concepts: Exoplanet atmospheres (487); Exoplanet

Biogenic Sulfur Gases as Biosignatures on Temperate Sub-Neptune Waterworlds

Sérgio Sacani

On 26 January 2023, a military pilot reported four potential unidentified anomalous phenomena (UAP) while operating in the Eglin Air Force Base training range off the coast of Florida. Through the onboard radar system, the pilot initially observed that the four objects were aloft between 16,000 – 18,000 feet and appeared to be flying in formation. However the pilot observed only one of the four objects visually and captured two images of the single object via the aircraft’s electro-optical/infrared (EO/IR) sensor (see Figures 1A and 1B). The pilot could not record video of the event because the aircraft’s video recording equipment was inoperable prior to and during the aircraft’s flight. The pilot observed this single object aloft at 16,000 feet. The following case information is based on the pilot’s initial report and a subsequent discussion that AARO held with the pilot to seek additional details about the pilot’s observation of the reported object.

All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...

Sérgio Sacani

Chemistry is the scientific study of matter, its properties, composition, structure, and the changes it undergoes. It's often divided into various sub-disciplines such as organic chemistry, inorganic chemistry, physical chemistry, analytical chemistry, and biochemistry. Chemistry plays a crucial role in understanding the world around us and has applications in various fields such as medicine, materials science, environmental science, and industry.

Chemistry 4th semester series (krishna).pdf

Sumit Kumar yadav

Green chemistry and Sustainable development.pptx

RajatChauhan518211

Botany is the branch of biology that deals with the scientific study of plants, including their structure, growth, reproduction, metabolism, development, and classification. It encompasses a wide range of topics, from the molecular biology of plant cells to the ecological relationships between plants and their environments. Botany is essential for understanding plant diversity, ecology, evolution, and the roles plants play in ecosystems and human societies.

Botany 4th semester series (krishna).pdf

Sumit Kumar yadav

Hire 💕 9907093804 Hooghly Call Girls Service Call Girls Agency

Sheetal Arora

Recently uploaded (20)

Nanoparticles synthesis and characterization

Formation of low mass protostars and their circumstellar disks

GBSN - Microbiology (Unit 1)

Pulmonary drug delivery system M.pharm -2nd sem P'ceutics

Chemical Tests; flame test, positive and negative ions test Edexcel Internati...

Biopesticide (2).pptx .This slides helps to know the different types of biop...

Botany 4th semester file By Sumit Kumar yadav.pdf

Presentation Vikram Lander by Vedansh Gupta.pptx

COST ESTIMATION FOR A RESEARCH PROJECT.pptx

Biological Classification BioHack (3).pdf

CELL -Structural and Functional unit of life.pdf

Animal Communication- Auditory and Visual.pptx

Creating and Analyzing Definitive Screening Designs

Isotopic evidence of long-lived volcanism on Io

Biogenic Sulfur Gases as Biosignatures on Temperate Sub-Neptune Waterworlds

All-domain Anomaly Resolution Office U.S. Department of Defense (U) Case: “Eg...

Chemistry 4th semester series (krishna).pdf

Green chemistry and Sustainable development.pptx

Botany 4th semester series (krishna).pdf

Hire 💕 9907093804 Hooghly Call Girls Service Call Girls Agency

GHY101 Unit 2.4 Australia & New Zealand

1. YouTube. Rabbit Proof Fence (1). Retrieved September 19, 2011: http://www.youtube.com/watch?v=DdFNZSx6hSQ Australia & New Zealand © Mark M. Miller The University of Southern Mississippi World Regional Geography

3. Google Earth

4. Amoeba blog. Retrieved February 14, 2012: http://www.amoeba.com/blog/2008/01/eric-s- blog/happy-australia-day.html

5. Mijiza’s. Retrieved September 20, 2010: http://deborahmazon.wordpress.co m/category/history/oceania/page/2 / Aborigine

6. Retrieved September 20, 2010: http://www.remotetribes.com/maori-tribe/ Maori

7. YouTube. Rabbit Proof Fence (1). Retrieved September 19, 2011: http://www.youtube.com/watch?v=DdFNZSx6hSQ

8. Strange Maps. Retrieved January 30, 2010: http://strangemaps.wordpress.com/

9. Map from the 1920s. Strange Maps. Retrieved October 24, 2010: http://bigthink.com/blogs/strang e-maps

10.

11. Oregon Press Register. Retrieved 10/27/06: http://www.newsregister.com/photos/upload/2005042815445 4_medium.jpg Immigration

12.

13. Embassy in Washington: http://www.nzembassy.com/usa

14. Australia’s Herald Sun: http://www.heraldsun.com.au New Zealand Herald: http://www.nzherald.co.nz/

15. New Zealand Tourism: http://www.newzealand.com

GHY101 Unit 2.4 Australia & New Zealand

Recommended

Recommended

More Related Content

More from Mark M. Miller

More from Mark M. Miller (20)

Recently uploaded

Recently uploaded (20)

GHY101 Unit 2.4 Australia & New Zealand