The term "alphasyllabic numeral system" is not a widely recognized or established concept in mathematics or linguistics. However, it seems to suggest a numeral system that combines elements of alphasyllabic writing systems and numerical representation. **Alphasyllabic Writing Systems:** Alphasyllabic scripts are a category of writing systems that represent consonant-vowel combinations.
The term "computer number format" refers to the various ways in which numbers can be represented and stored in a computer's memory. Different formats cater to different needs in terms of precision, range, and efficiency. The most common formats include: 1. **Integer Formats**: - **Binary**: Integers are typically stored in binary format (base 2), where each bit represents a power of 2. - **Signed vs.
Jacques Pelletier du Mans (c. 1495–1554) was a notable French humanist, physician, and scholar during the Renaissance period. He is best known for his contributions to literature, particularly through his work in promoting humanist thought and classical learning.
LDN 1641 by Wikipedia Bot 0
LDN 1641 is a compound that has been studied for its potential therapeutic effects, particularly in the context of neurodegenerative diseases and other conditions. It is a selective inhibitor of the enzyme glycogen synthase kinase 3 (GSK-3), which plays a critical role in various cellular processes, including cell survival, proliferation, and metabolism.
N41 (nebula) by Wikipedia Bot 0
N41, also known as LBN 762 or the Drunken Dragon Nebula, is a dark nebula located in the constellation of Cassiopeia. Dark nebulae are regions of space that contain dust and other materials, blocking the light from stars and other objects behind them. N41 is notable for its distinctive shape, which some observers think resembles a dragon.
NGC 1333 by Wikipedia Bot 0
NGC 1333 is a reflection nebula located in the constellation Perseus. It is part of the Perseus molecular cloud complex and is known for its rich star-forming activities. The nebula is prominent in the study of star formation because it contains many young, newly formed stars and protostars. One of the key features of NGC 1333 is its bright and intricate structure, which is illuminated by the light from newly formed stars within the cloud.
NGC 1579 by Wikipedia Bot 0
NGC 1579 is an emission nebula located in the constellation Cassiopeia. This nebula is notable for being a region of active star formation, where new stars are being born from the surrounding gas and dust. It is part of a larger molecular cloud complex. NGC 1579 can be observed with telescopes and is often studied by astronomers to gain insights into the processes of star formation and the evolution of stellar systems.
Pelican Nebula by Wikipedia Bot 0
The Pelican Nebula, also designated as IC 5070, is an emission nebula located in the constellation Cygnus. It is situated near the well-known North America Nebula (NGC 7000) and is part of a larger complex of gas and dust in the Milky Way that is active in star formation. The nebula gets its name from its shape, which resembles a pelican in flight.
R136 by Wikipedia Bot 0
R136 is a star cluster located in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. The cluster is notable for containing some of the most massive and luminous stars known, including R136a1, which is often cited as one of the most massive stars in the universe. The cluster is part of a region of intense star formation known as the 30 Doradus or the Tarantula Nebula.
The Rho Ophiuchi cloud complex is a prominent star-forming region located in the constellation Ophiuchus. It is one of the closest such regions to Earth, situated at a distance of about 130 light-years. The complex contains a rich array of young stars, protostars, and various molecular clouds, making it an important area of study for astronomers interested in stellar formation and the dynamics of interstellar matter.
The Serpens–Aquila Rift is a region of space that contains a dense concentration of interstellar dust and gas, located between the constellations of Serpens and Aquila. This area is notable for its obscuration of background stars and is associated with active star formation. The rift's dense dust clouds act as a barrier that prevents visible light from passing through, which is why it appears as a dark band in the Milky Way when viewed from Earth.
Sh2-297 by Wikipedia Bot 0
Sh2-297, also known as LBN 762 or the "Star-forming region," is a bright emission nebula located in the constellation Cassiopeia. It is part of a larger region of star formation and is known for its rich hydrogen emission, which is indicative of ongoing stellar activity. Sh2-297 is interesting to astronomers because it contains regions of dense gas and dust, which are the building blocks for new stars.
The Taurus Molecular Cloud is a prominent region of star formation located in the constellation Taurus. It is one of the closest molecular clouds to Earth, situated about 450 light-years away. This cloud is significant for several reasons, primarily its role in the birth of stars and the study of star formation processes. Key characteristics of the Taurus Molecular Cloud include: 1. **Composition**: It is composed mainly of gas and dust, with molecules like hydrogen, carbon monoxide (CO), and various other compounds.
Trumpler 16 by Wikipedia Bot 0
Trumpler 16 is a young open cluster located in the Carina Nebula, which is part of the larger Carina constellation in the southern sky. This cluster is noted for containing some of the most massive and luminous stars known, including several O-type stars. Its members are relatively young, with an estimated age of around 2 to 3 million years.
Fast ice by Wikipedia Bot 0
Fast ice refers to sea ice that is connected to the coast or to large ice formations such as ice shelves. It remains anchored and does not drift with ocean currents or winds. Fast ice typically forms in areas where the water is shallow enough and is subject to consistent freezing conditions, allowing it to remain stable over longer periods. This type of ice plays a crucial role in the Arctic and Antarctic ecosystems as it provides habitat for various marine species, protects coastal areas from wave action, and influences local climate patterns.
Grease ice by Wikipedia Bot 0
Grease ice is a type of ice that forms under specific conditions in cold environments, typically found in polar regions or near ice-covered bodies of water. It is characterized by a thin, slushy layer that consists of small ice crystals and water, often resembling a viscous, greasy surface. Grease ice can develop when small ice crystals begin to coalesce and are mixed with water, creating a surface that appears shiny and can have a somewhat liquid-like texture.
Pancake ice by Wikipedia Bot 0
Pancake ice refers to a type of ice formation found on the surface of water bodies, typically in cold regions. It consists of rounded, flat pieces of ice that resemble pancakes, hence the name. This phenomenon usually occurs in the early stages of ice formation, where ice crystals break and then re-freeze into these disc-like shapes as wind and water movement cause them to bump into each other.
Rotten ice by Wikipedia Bot 0
Rotten ice refers to a particular condition of ice that occurs when it becomes weak, unstable, or compromised due to factors such as melting, deterioration, or water saturation. This type of ice can appear slushy or has a crumbling texture, indicating that it is no longer solid or safe for activities such as walking, skating, or snowmobiling. The term can also describe ice that has been affected by warm weather or when water seeps into cracks and freezes, creating a less stable structure.
Sea ice microbial communities refer to the diverse assemblages of microorganisms, including bacteria, archaea, viruses, and microalgae, that inhabit and thrive within the sea ice environment. These communities play crucial roles in the polar ecosystems, as they are integral to biogeochemical processes and contribute to the overall productivity of the marine food web.
Bimorph by Wikipedia Bot 0
A bimorph is a type of actuator or sensor that consists of two layers of materials with different expansion properties, typically bonded together. When an electrical voltage is applied across the bimorph structure, the difference in expansion or contraction between the two materials causes the bimorph to bend or deform. This principle is often used in applications like piezoelectric devices, where the bimorph can convert electrical energy into mechanical motion or vice versa.

Pinned article: ourbigbook/introduction-to-the-ourbigbook-project

Welcome to the OurBigBook Project! Our goal is to create the perfect publishing platform for STEM subjects, and get university-level students to write the best free STEM tutorials ever.
Everyone is welcome to create an account and play with the site: ourbigbook.com/go/register. We belive that students themselves can write amazing tutorials, but teachers are welcome too. You can write about anything you want, it doesn't have to be STEM or even educational. Silly test content is very welcome and you won't be penalized in any way. Just keep it legal!
We have two killer features:
  1. topics: topics group articles by different users with the same title, e.g. here is the topic for the "Fundamental Theorem of Calculus" ourbigbook.com/go/topic/fundamental-theorem-of-calculus
    Articles of different users are sorted by upvote within each article page. This feature is a bit like:
    • a Wikipedia where each user can have their own version of each article
    • a Q&A website like Stack Overflow, where multiple people can give their views on a given topic, and the best ones are sorted by upvote. Except you don't need to wait for someone to ask first, and any topic goes, no matter how narrow or broad
    This feature makes it possible for readers to find better explanations of any topic created by other writers. And it allows writers to create an explanation in a place that readers might actually find it.
    Figure 1.
    Screenshot of the "Derivative" topic page
    . View it live at: ourbigbook.com/go/topic/derivative
  2. local editing: you can store all your personal knowledge base content locally in a plaintext markup format that can be edited locally and published either:
    This way you can be sure that even if OurBigBook.com were to go down one day (which we have no plans to do as it is quite cheap to host!), your content will still be perfectly readable as a static site.
    Figure 5. . You can also edit articles on the Web editor without installing anything locally.
    Video 3.
    Edit locally and publish demo
    . Source. This shows editing OurBigBook Markup and publishing it using the Visual Studio Code extension.
  3. https://raw.githubusercontent.com/ourbigbook/ourbigbook-media/master/feature/x/hilbert-space-arrow.png
  4. Infinitely deep tables of contents:
    Figure 6.
    Dynamic article tree with infinitely deep table of contents
    .
    Descendant pages can also show up as toplevel e.g.: ourbigbook.com/cirosantilli/chordate-subclade
All our software is open source and hosted at: github.com/ourbigbook/ourbigbook
Further documentation can be found at: docs.ourbigbook.com
Feel free to reach our to us for any help or suggestions: docs.ourbigbook.com/#contact