Mark A. Johnson is a common name and could refer to several individuals in various fields, such as academia, business, or the arts. Without specific context, it's difficult to determine exactly which Mark A. Johnson you are inquiring about.
Pieter Zeeman (1865-1943) was a Dutch physicist best known for his discovery of the Zeeman Effect, which describes the splitting of spectral lines in the presence of a strong magnetic field. This phenomenon occurs because the energy levels of atomic electrons are affected by the magnetic field, resulting in the observed splitting of light into different frequencies.
Robert Bunsen (1811–1899) was a German chemist best known for his contributions to the field of chemistry and for the invention of the Bunsen burner, a common laboratory tool used for heating, sterilization, and combustion. The Bunsen burner provides a flame produced by mixing gas with air, allowing for precise temperature control in various chemical experiments.
Theodore Lyman IV is a notable American scientist and entrepreneur, particularly recognized for his contributions to the fields of laser technology and optics. He has been involved in various innovative projects and companies focused on advancing these technologies.
William Duane (born April 22, 1872 – died January 16, 1935) was an American physicist known for his contributions to the field of atomic and radiation physics. He was particularly noted for his work in experimental physics and made significant contributions to the understanding of the photoelectric effect. Duane is also recognized for the development of various technological applications related to radiation.
Monochromatic wavelength dispersive X-ray fluorescence (WDXRF) is an analytical technique used to determine the elemental composition of materials. This method combines principles of X-ray fluorescence (XRF) with monochromatic wavelength dispersion, allowing for highly precise and sensitive elemental analysis. ### Key Components and Principles: 1. **X-ray Fluorescence (XRF)**: - XRF is a non-destructive analytical technique used to analyze the elemental composition of materials.
Cepheus OB1 is a stellar association in the constellation of Cepheus. Stellar associations are groups of stars that are physically related and share a common origin. Cepheus OB1 is notable for containing several young, hot, and massive stars, which are typically classified as OB stars. These stars are characterized by their high temperatures, large masses, and often, their short lifespans.
Vibrational spectroscopy is a technique used to study the vibrational transitions in molecules, which are related to the vibrations of atoms within the molecular structure. When it comes to linear molecules, vibrational spectroscopy can provide insights into how these molecules vibrate and how those vibrations can be measured through interaction with electromagnetic radiation. ### Key Concepts: 1. **Vibrational Modes**: Linear molecules exhibit specific vibrational modes based on their structure.
Energy-dispersive X-ray spectroscopy (EDX or EDS) is an analytical technique used to determine the elemental composition of materials. It is frequently employed in conjunction with scanning electron microscopy (SEM) or transmission electron microscopy (TEM). ### Key Features of EDX: 1. **Principle of Operation**: EDX works by bombarding a sample with high-energy X-rays or electrons.
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, 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 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.
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 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.
A sun outage, also known as a solar outage, refers to a temporary disruption in satellite communication signals caused by the alignment of the sun, Earth, and the satellite. This phenomenon typically occurs during specific times of the year, usually around the equinoxes in March and September, when the sun is directly behind a satellite in geostationary orbit as viewed from Earth.
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 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.
Coronal seismology is a specialized field of astrophysics that studies oscillations and waves in the solar corona, the outer layer of the Sun's atmosphere. This technique involves the analysis of various types of wave phenomena, such as acoustic waves, magnetohydrodynamic (MHD) waves, and other oscillations that propagate through the plasma of the corona. These waves can result from disturbances such as solar flares, coronal mass ejections (CMEs), and the solar wind.
Shadowboxing is a training exercise commonly used in boxing, martial arts, and other combat sports. It involves practicing techniques and movements without a partner or an opponent, allowing the athlete to improve their footwork, technique, speed, and conditioning. During shadowboxing, practitioners simulate a fight by moving around and throwing punches or executing techniques against an imaginary opponent. This exercise helps refine skills such as form, timing, and rhythm, as well as enhancing muscle memory.
Hale's law, named after the American astronomer George Ellery Hale, refers to the observation that there is a relationship between the activity levels of sunspots and the solar cycle. Specifically, Hale formulated the law in terms of the magnetic field of sunspots, which states that sunspots exhibit a consistent pattern of polarity that reverses every solar cycle (approximately every 11 years). This law highlights the role of solar magnetic activity in influencing sunspot formation and behavior.

Pinned article: 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 2.
    You can publish local OurBigBook lightweight markup files to either https://OurBigBook.com or as a static website
    .
    Figure 3.
    Visual Studio Code extension installation
    .
    Figure 4.
    Visual Studio Code extension tree navigation
    .
    Figure 5.
    Web editor
    . 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.
    Video 4.
    OurBigBook Visual Studio Code extension editing and navigation demo
    . Source.
  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