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Remas Mohamed

الذكاء العاطفي

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استراتيجية إدارة الأزمات

Prof. Mohamed Belal

إدارة الأزمات والطوارئ

Prof. Mohamed Belal

ادارة الوقت

Atia Lawgali

إدارة الوقت هي إدارة للذات

Teaching Skills

قواعد الجامعة الأربعون

Muhammad ELSalamony

Human sexual intercourse

DinDin Horneja

En vedette (6)

استراتيجية إدارة الأزمات

إدارة الأزمات والطوارئ

ادارة الوقت

إدارة الوقت هي إدارة للذات

قواعد الجامعة الأربعون

Human sexual intercourse

Plus de Remas Mohamed

أخطاء اللغة العربية المعاصرة عند الكتاب و الإذاعيين

Remas Mohamed

راحة البال والشباب

Remas Mohamed

التنمية وجهًا لوجه

Remas Mohamed

حل المشاكل و إتخاذ القرارات

Remas Mohamed

سويولوجيا الجمهور السياسي و الديني

الرؤوس المفخخة

الارهاب

Crisis management

إبراهيم الفقي البرمجة اللغوية العصبية

Remas Mohamed

حرب الافكار

Remas Mohamed

Sampling and sample size determination

Remas Mohamed

مهارات حل المشكلات واتخاذ القرار

فن التعامل مع الناس

Etiquette

hard v soft power

A theory-of-public-diplomacy-

Remas Mohamed

Communication Skills

Remas Mohamed

communication

Remas Mohamed

PERSONAL SELLING AND SALES MANAGEMENT

Remas Mohamed

العرب , وجهة نظر يابانية

Remas Mohamed

Plus de Remas Mohamed (20)

أخطاء اللغة العربية المعاصرة عند الكتاب و الإذاعيين

راحة البال والشباب

التنمية وجهًا لوجه

حل المشاكل و إتخاذ القرارات

سويولوجيا الجمهور السياسي و الديني

الرؤوس المفخخة

الارهاب

Crisis management

إبراهيم الفقي البرمجة اللغوية العصبية

حرب الافكار

Sampling and sample size determination

مهارات حل المشكلات واتخاذ القرار

فن التعامل مع الناس

Etiquette

hard v soft power

A theory-of-public-diplomacy-

Communication Skills

communication

PERSONAL SELLING AND SALES MANAGEMENT

العرب , وجهة نظر يابانية

Dernier

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

Presentation Vikram Lander by Vedansh Gupta.pptx

gindu3009

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

sakshisoni2385

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

ssuser79fe74

Context. WASP-76 b has been a recurrent subject of study since the detection of a signature in high-resolution transit spectroscopy data indicating an asymmetry between the two limbs of the planet. The existence of this asymmetric signature has been confirmed by multiple studies, but its physical origin is still under debate. In addition, it contrasts with the absence of asymmetry reported in the infrared (IR) phase curve. Aims. We provide a more comprehensive dataset of WASP-76 b with the goal of drawing a complete view of the physical processes at work in this atmosphere. In particular, we attempt to reconcile visible high-resolution transit spectroscopy data and IR broadband phase curves. Methods. We gathered 3 phase curves, 20 occultations, and 6 transits for WASP-76 b in the visible with the CHEOPS space telescope. We also report the analysis of three unpublished sectors observed by the TESS space telescope (also in the visible), which represents 34 phase curves. Results. WASP-76 b displays an occultation of 260±11 and 152±10 ppm in TESS and CHEOPS bandpasses respectively. Depending on the composition assumed for the atmosphere and the data reduction used for the IR data, we derived geometric albedo estimates that range from 0.05 ± 0.023 to 0.146 ± 0.013 and from <0.13 to 0.189 ± 0.017 in the CHEOPS and TESS bandpasses, respectively. As expected from the IR phase curves, a low-order model of the phase curves does not yield any detectable asymmetry in the visible either. However, an empirical model allowing for sharper phase curve variations offers a hint of a flux excess before the occultation, with an amplitude of ∼40 ppm, an orbital offset of ∼−30◦ , and a width of ∼20◦ . We also constrained the orbital eccentricity of WASP-76 b to a value lower than 0.0067, with a 99.7% confidence level. This result contradicts earlier proposed scenarios aimed at explaining the asymmetry observed in high-resolution transit spectroscopy. Conclusions. In light of these findings, we hypothesise that WASP-76 b could have night-side clouds that extend predominantly towards its eastern limb. At this limb, the clouds would be associated with spherical droplets or spherically shaped aerosols of an unknown species, which would be responsible for a glory effect in the visible phase curves.

Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b

Sérgio Sacani

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GBSN - Microbiology (Unit 1)

Areesha Ahmad

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

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Recombinant DNA technology (Immunological screening)

PraveenaKalaiselvan1

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

We explore different scenarios to explain the chemical difference found in the remarkable giant-giant binary system HD138202+CD−3012303. For the first time, we suggest how to distinguish these scenarios by taking advantage of the extensive convective envelopes of giant stars. Methods. We carried out a high-precision determination of stellar parameters and abundances by applying a full line-by-line differential analysis on GHOST high-resolution spectra. We used the FUNDPAR program with ATLAS12 model atmospheres and specific opacities calculated for an arbitrary composition through a doubly iterated method. Physical parameters were estimated with the isochrones package and evolutionary tracks were calculated via MIST models. Results. We found a significant chemical difference between the two stars (∆[Fe/H]∼0.08dex), which is largely unexpected considering the insensitivity of giant stars to planetary ingestion and diffusion effects. We tested the possibility of engulfment events by using several different combinations of stellar mass, ingested mass, metallicity of the engulfed object and different convective envelopes. However, the planetary ingestion scenario does not seem to explain the observed differences. For the first time, we distinguished the source of chemical differences using a giant-giant binary system. By ruling out other possible scenarios such as planet formation and evolutionary effects between the two stars, we suggest that primordial inhomogeneities might explain the observed differences. This remarkable result implies that the metallicity differences that were observed in at least some main-sequence binary systems might be related to primordial inhomogeneities rather than engulfment events. We also discuss the important implications of finding primordial inhomogeneities, which affect chemical tagging and other fields such as planet formation. We strongly encourage the use of giantgiant pairs. They are a relevant complement to main-sequence pairs for determining the origin of the observed chemical differences in multiple systems.

Disentangling the origin of chemical differences using GHOST

Sérgio Sacani

Bacterial Identification and Classifications

Areesha Ahmad

Nanoparticles synthesis and characterization

kaibalyasahoo82800

CELL -Structural and Functional unit of life.pdf

Nistarini College, Purulia (W.B) India

SCIENCE-4-QUARTER4-WEEK-4-PPT-1 (1).pptx

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Zoology 4th semester series (krishna).pdf

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Botany 4th semester series (krishna).pdf

Presentation Vikram Lander by Vedansh Gupta.pptx

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

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

Asymmetry in the atmosphere of the ultra-hot Jupiter WASP-76 b

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TEST BANK For Radiologic Science for Technologists, 12th Edition by Stewart C...

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GBSN - Microbiology (Unit 1)

Formation of low mass protostars and their circumstellar disks

Stunning ➥8448380779▻ Call Girls In Panchshil Enclave Delhi NCR

Recombinant DNA technology (Immunological screening)

Animal Communication- Auditory and Visual.pptx

Disentangling the origin of chemical differences using GHOST

Bacterial Identification and Classifications

Nanoparticles synthesis and characterization

CELL -Structural and Functional unit of life.pdf

SCIENCE-4-QUARTER4-WEEK-4-PPT-1 (1).pptx

Zoology 4th semester series (krishna).pdf

Kochi ❤CALL GIRL 84099*07087 ❤CALL GIRLS IN Kochi ESCORT SERVICE❤CALL GIRL

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