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Arif Nurjiyanto

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GBSN - Biochemistry (Unit 1)

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👉 𝑾𝑰𝑳𝑳 𝑷𝑹𝑶𝑽𝑰𝑫𝑬 𝒀𝑶𝑼 𝑾𝑰𝑻𝑯 𝑺𝑬𝑿𝒀 𝑴𝑶𝑫𝑬𝑳𝑺 𝑾𝑯𝑶 𝑾𝑰𝑳𝑳 𝑫𝑨𝑵𝑪𝑬 & 𝑫𝑹𝑰𝑵𝑲 𝑾𝑰𝑻𝑯 𝒀𝑶𝑼 𝑨𝑵𝑫 𝑨𝑳𝑺𝑶 𝑷𝑹𝑶𝑽𝑰𝑫𝑬 𝒀𝑶𝑼 𝑺𝑬𝑿𝑼𝑨𝑳 𝑩𝑶𝑫𝒀 𝑻𝑶 𝑩𝑶𝑫𝒀 𝑴𝑨𝑺𝑺𝑨𝑮𝑬 𝑾𝑰𝑻𝑯 𝑺𝑬𝑿. 👉𝒀𝑶𝑼 𝑴𝑨𝒀 𝑻𝑨𝑲𝑬 𝑻𝑯𝑬𝑴 𝑶𝑼𝑻 𝑭𝑶𝑹 𝑨 𝑷𝑨𝑹𝑻𝒀 𝑶𝑹 𝑨𝑳𝑺𝑶 𝑭𝑶𝑹 𝑨𝑵𝒀 𝑷𝑹𝑰𝑽𝑨𝑻𝑬 𝑷𝑨𝑹𝑻𝑰𝑬𝑺. 👉𝑻𝑯𝑬𝑺𝑬 𝑮𝑰𝑹𝑳𝑺 𝑨𝑹𝑬 𝑰𝑵𝑻𝑬𝑹𝑬𝑺𝑻𝑬𝑫 𝑰𝑵 𝑯𝑨𝑽𝑰𝑵𝑮 𝑺𝑶𝑴𝑬 𝑭𝑼𝑵 𝑾𝑰𝑻𝑯 𝒀𝑶𝑼 𝑨𝑵𝑫 𝑾𝑰𝑳𝑳 𝑬𝑵𝑺𝑼𝑹𝑬 𝑻𝑯𝑨𝑻 𝒀𝑶𝑼 𝑯𝑨𝑽𝑬 𝑪𝑶𝑴𝑷𝑳𝑬𝑻𝑬 𝑭𝑼𝑵. 28/April/2024 {{🎗️SCH🎗️}} 8923113531 How to book call girls The Booking process is particularly time-saving and more comfortable for us. Below mentioned are the steps you need to follow to hire our call girl: Step 1 - Visit our Call Girls Service website Step 2 - check for the portfolios of our sexy and hot call girls Step 3 - check on the services provided by the specific call girls Step 4 - Once you have selected the call girls and respective services, go to the contact us page. Step 5 - on the contact page, you will get our phone number, WhatsApp number, and email address. You can choose any one of them to connect with us. Call Us – 8923113531 ✣ ✤ ✥ ✦ 𝑻𝑰𝑴𝑬 𝑾𝑨𝑺𝑻𝑬𝑹𝑺 𝑨𝑵𝑫 𝑩𝑨𝑹𝑮𝑨𝑰𝑵𝑬𝑹𝑺 𝑨𝑹𝑬 𝑷𝑳𝑬𝑨𝑺𝑬 𝑬𝑿𝑪𝑼𝑺𝑬, 𝑾𝑬 𝑹𝑬𝑺𝑷𝑬𝑪𝑻 𝒀𝑶𝑼𝑹 𝑺𝑨𝑭𝑬𝑻𝒀 𝑨𝑵𝑫 𝑷𝑹𝑰𝑽𝑨𝑪𝒀 𝑨𝑵𝑫 𝑬𝑿𝑷𝑬𝑪𝑻 𝑻𝑯𝑬 𝑺𝑨𝑴𝑬 𝑭𝑹𝑶𝑴 𝒀𝑶𝑼.✣ ✤ ✥ ✦ Duration Normal Girls Housewives High-Profile Models (Celebrities) 1 Shot ₹ 8,000 ₹ 10,000 ₹ 15,000 2 Shots ₹ 15,000 ₹ 15,000 ₹ 25,000 Full Day ₹ 35,000 ₹ 35,000 ₹ 40,000 Full Night ₹ 40,000 ₹ 40,000 ₹ 50,000 Weekend ₹ 45,000 ₹ 45,000 ₹ 50,000 Party Nights ₹ 50,000 ₹ 50,000 ₹ 60,000

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Wepresent Atacama Large Millimeter/submillimeter Array 12-m, 7-m, and Total Power Array observations of the FUOrionis outbursting system, covering spatial scales ranging from 160 to 25,000 au. The high-resolution interferometric data reveal an elongated 12CO(2–1) feature previously observed at lower resolution in 12CO(3–2). Kinematic modeling indicates that this feature can be interpreted as an accretion streamer feeding the binary system. The mass infall rate provided by the streamer is significantly lower than the typical stellar accretion rates (even in quiescent states), suggesting that this streamer alone is not massive enough to sustain the enhanced accretion rates characteristic of the outbursting class prototype. The observed streamer may not be directly linked to the current outburst, but rather a remnant of a previous, more massive streamer that may have contributed enough to the disk mass to render it unstable and trigger the FU Orionis outburst. The new data detect, for the first time, a vast, slow-moving carbon monoxide molecular outflow emerging from this object. To accurately assess the outflow properties (mass, momentum, and kinetic energy), we employ 13CO(2–1) data to correct for optical depth effects. The analysis indicates that the outflow corresponds to swept-up material not associated with the current outburst, similar to the slow molecular outflows observed around other FUor and Class I protostellar objects.

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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.

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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.

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Small size (20-300 nm) / bacteria (size measured in μm) Viral genome – single type of nucleic acid: DNA – dezoxyriboviruses RNA - riboviruses Totally dependant on living cells for all metabolic processes May infect humans, animals, plants, bacteria, fungi,parasites, insects Virion = viral corpuscle = elementary, infectious unit. Only visible by electron microscopy. Laboratory diagnosis of viral infections Methods: • Cytology • Electron microscopy • Cultivation • Detection of viral proteins • Serology • Molecular diagnosis (detection of genetic material i.e. nucleic acids) PPT prepared by Dr. Prince C P

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RecoveringancientrecordsofEarth'smagneticfieldisessentialfordeterminingtheroleofthemagnetosphereinprotectingearlyEarthfromcosmicradiationandatmosphericescape.WepresentpaleomagneticfieldtestshintingthatarecordofEarth's3.7‐billion‐year(Ga)oldmagneticfieldmaybepreservedinthenortheasternIsuaSupracrustalBeltasachemicalremanentmagnetizationacquiredduringamphibolite‐grademetamorphisminthebandedironformation.MultiplepetrologicalandgeochronologicallinesofevidenceindicatethatthenorthernmostpartofIsuahasnotexperiencedmetamorphictemperaturesexceeding380°CsincetheEoarchean,suggestingtherockshavenotbeensignificantlyheatedsincemagnetizationwasacquired.Weuse“pseudo”bakedcontacttests(intrusionsemplaced3.26–3.5Gaago)andafoldtest(folding3.6Gaago)todemonstratethatsomesamplespreserveaca.3.7Garecordofthemagneticfield.Werecoverafieldstrengthof>15μT.ThissuggeststhatEarth'smagneticfieldmayhavebeenweakenoughtoenhanceatmosphericescapeduringtheArchean

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Bollworms are among the most damaging pests in cotton cultivation, affecting the bolls where the cotton fibers are formed. There are several species of bollworms, each capable of causing significant yield loss and quality degradation if not effectively managed. Here’s a detailed look at the primary bollworm species affecting cotton: Cotton Bollworm (Helicoverpa armigera): Also known as the corn earworm or the Old World bollworm, this pest is found in many regions around the world. It is highly polyphagous (feeds on many different plants) and poses a threat not only to cotton but also to maize, tomatoes, and legumes. The larvae bore into the cotton bolls, feeding on the developing seeds and fibers, which can lead to boll rot. Pink Bollworm (Pectinophora gossypiella): A significant pest of cotton, the pink bollworm larvae infest the cotton bolls, feeding on the seeds and lint. This can severely damage or destroy the bolls. In regions where pink bollworms are prevalent, they have been a major driver for the adoption of genetically engineered Bt cotton, which expresses a bacterium gene toxic to certain insects. Tobacco Budworm (Heliothis virescens): Closely related to the cotton bollworm, the tobacco budworm primarily attacks tobacco but is also a common pest in cotton. It primarily damages the flowers and bolls of the cotton plant. Differentiating between the tobacco budworm and the cotton bollworm based on appearance can be challenging, but it is crucial for effective management. American Bollworm (Helicoverpa zea): Known in some regions as the corn earworm, it is similar in behavior to Helicoverpa armigera and poses a threat to a variety of crops, including cotton. The larvae attack the cotton bolls, leading to direct damage to the cotton lint and seeds. Management Strategies: Cultural Controls: Crop rotation, destruction of crop residues, and deep plowing can help break the pest’s life cycle. Timing of planting can also be adjusted to avoid peak pest infestation. Biological Controls: Natural enemies like Trichogramma wasps, which parasitize bollworm eggs, and predators such as lacewings and ladybugs can be encouraged. Bacillus thuringiensis (Bt) products can also be sprayed, which are particularly effective against young larvae. Chemical Controls: Insecticides may be required when infestation levels exceed economic thresholds. However, resistance management must be considered, alternating modes of action to avoid developing resistance. Genetic Approaches: Bt cotton, genetically modified to express Bacillus thuringiensis toxin, has been highly effective in controlling bollworms and has dramatically reduced the reliance on chemical insecticides. Monitoring and Scouting: Regular field scouting and using pheromone traps to monitor adult populations can help in timely and targeted application of control measures. The effective management of bollworms often requires an integrated approach

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From their humble beginnings in 1984, TED has grown into the world’s most powerful amplifier for speakers and thought-leaders to share their ideas. They have over 2,400 filmed talks (not including the 30,000+ TEDx videos) freely available online, and have hosted over 17,500 events around the world. With over one billion views in a year, it’s no wonder that so many speakers are looking to TED for ideas on how to share their message more effectively. The article “5 Public-Speaking Tips TED Gives Its Speakers”, by Carmine Gallo for Forbes, gives speakers five practical ways to connect with their audience, and effectively share their ideas on stage. Whether you are gearing up to get on a TED stage yourself, or just want to master the skills that so many of their speakers possess, these tips and quotes from Chris Anderson, the TED Talks Curator, will encourage you to make the most impactful impression on your audience. See the full article and more summaries like this on SpeakerHub here: https://speakerhub.com/blog/5-presentation-tips-ted-gives-its-speakers See the original article on Forbes here: http://www.forbes.com/forbes/welcome/?toURL=http://www.forbes.com/sites/carminegallo/2016/05/06/5-public-speaking-tips-ted-gives-its-speakers/&refURL=&referrer=#5c07a8221d9b

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Everyone is in agreement that ChatGPT (and other generative AI tools) will shape the future of work. Yet there is little consensus on exactly how, when, and to what extent this technology will change our world. Businesses that extract maximum value from ChatGPT will use it as a collaborative tool for everything from brainstorming to technical maintenance. For individuals, now is the time to pinpoint the skills the future professional will need to thrive in the AI age. Check out this presentation to understand what ChatGPT is, how it will shape the future of work, and how you can prepare to take advantage.

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