Tropospheric Emissions: Monitoring of Pollution (TEMPO) is a satellite-based mission initiated by NASA to monitor air quality and track pollutants in the Earth's atmosphere, specifically in the troposphere, which is the lowest layer of the atmosphere where most weather events occur and where human activities contribute significantly to air pollution.
The Venus Emissivity Mapper (VEM) is an instrument designed to study Venus, particularly its surface composition and geology. Part of NASA's upcoming VERITAS (Venus Emissivity, Radio Science, InSAR, Topography, and Spectroscopy) mission, VEM will utilize advanced infrared spectroscopy to analyze the thermal emissions from the planet's surface.
The **PRL Advanced Radial-velocity All-sky Search (PARAS)** is an astronomical project aimed at detecting exoplanets around distant stars using radial velocity measurements. This project utilizes high-precision spectroscopy to measure the subtle shifts in the wavelength of light emitted by stars, which are caused by the gravitational influence of orbiting planets.
The SOPHIE échelle spectrograph is a high-resolution astronomical spectrograph used for the study of stellar spectra. It is primarily mounted on the 1.93-meter telescope at the Observatoire de Haute-Provence in France. SOPHIE is designed to observe the spectra of stars and is particularly well-suited for detecting exoplanets through Doppler spectroscopy, which involves measuring the slight shifts in the spectral lines of stars caused by the gravitational influence of orbiting planets.
Anders Jonas Ångström (1814–1874) was a Swedish physicist and astronomer known for his significant contributions to the field of spectroscopy and the study of light. He is best recognized for his work in measuring the wavelengths of various spectral lines and for founding the science of spectrometry. Ångström is particularly noted for his studies of the spectrum of light emitted by different elements, which laid the groundwork for modern spectroscopy.
Andrea Russell may refer to various individuals, depending on the context. Without additional details, it's unclear to whom you are specifically referring. Here are a few possibilities: 1. **Andrea Russell (Athlete)** - Could refer to an athlete in various sports, though specific information would be needed to provide context on their achievements. 2. **Andrea Russell (Academic)** - Might refer to a scholar or professional in academia, research, or other fields.
The Canadian Penning Trap Mass Spectrometer (CPTMS) is a type of mass spectrometer that utilizes the Penning trap technique for high-precision mass measurements of ions. This instrument is primarily used in nuclear physics, mass spectrometry, and related fields to analyze the mass-to-charge ratios of ions, which can provide valuable information about their composition and properties.
Clover is a type of gamma-ray detector used in nuclear physics, particularly for experiments involving the detection and measurement of gamma radiation emitted from radioactive materials. The Clover detector is an acronym that stands for "Clover-type Ge detector." Clover detectors are typically made using high-purity Germanium (HPGe) crystals. They are designed to provide high-resolution measurements of gamma-ray energies, which is crucial for identifying isotopes and studying nuclear decay processes.
The Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) is an instrument aboard NASA's Mars Reconnaissance Orbiter (MRO), which was launched in August 2005. CRISM is designed to capture high-resolution images of the Martian surface and analyze the mineral composition through spectral imaging.
A Computed Tomography Imaging Spectrometer (CTIS) is an advanced imaging technology that combines principles from both computed tomography (CT) and spectroscopy. It is used to capture detailed images of objects while simultaneously measuring their spectral properties, allowing for the analysis of material composition and other characteristics at different wavelengths of light. ### Key Features of CTIS: 1. **Imaging and Spectroscopy**: CTIS can produce spatial images while capturing spectral information across a range of wavelengths.
A DU spectrophotometer is a type of laboratory instrument used for measuring the absorbance or transmittance of light by a sample at specific wavelengths. The "DU" in DU spectrophotometer typically refers to a specific model series produced by Beckman Coulter, a company known for its laboratory instruments and analytical devices.
The Dobson ozone spectrophotometer is an instrument used to measure the concentration of ozone in the Earth's atmosphere. Developed in the 1920s by British scientist G. M. B. Dobson, it became one of the most significant tools for monitoring atmospheric ozone levels, especially in the stratosphere.
An **Electrical Aerosol Spectrometer (EAS)** is an analytical instrument used to measure and characterize aerosol particles in the atmosphere or various environments. Aerosols are tiny solid or liquid particles suspended in gas, and they can have significant effects on air quality, climate, and human health. ### Key Features and Functionality: 1. **Particle Size Distribution**: EAS devices measure the size distribution of aerosol particles, which is crucial for understanding their sources, behavior, and impacts.
A filter fluorometer is an analytical instrument used to measure the concentration of fluorescent substances in a sample by detecting the light emitted by those substances after they have been excited by a specific wavelength of light. Fluorometry is based on the principle of fluorescence, where certain molecules absorb light at one wavelength and then re-emit it at a longer wavelength.
The Gamma-Ray Imaging Spectrometer (GRIS) is a scientific instrument designed to detect and analyze gamma-ray emissions from various sources, such as astronomical objects, planetary bodies, and terrestrial environments. These emissions can provide valuable information about the composition, structure, and processes occurring in the observed phenomena. Gamma rays are electromagnetic radiation emitted by radioactive materials and certain cosmic events; they have very high energy.
The Gamma Ray Spectrometer (GRS) aboard the 2001 Mars Odyssey spacecraft is an instrument designed to study the composition of the Martian surface and to assess the planet's geology and mineralogy. Launched on April 7, 2001, and arriving at Mars on October 24, 2001, the Mars Odyssey orbiter carries the GRS as one of its primary scientific instruments.
August Herman Pfund (1859–1942) was a notable American physicist, particularly known for his contributions to the field of optics and the study of diffraction and interference of light. He is recognized for developing the Pfund curve, which relates to the optical properties of materials. Additionally, he made significant strides in spectrophotometry and was involved in research that helped advance the understanding of light and color.
Barbara H. Stuart may refer to a specific individual, but without additional context, it's difficult to provide accurate information. There may be multiple people with that name across various fields or professions. If you could provide more details about who Barbara H.
MERIS, or the Medium Resolution Imaging Spectrometer, is an instrument that was primarily used aboard the European Space Agency's Envisat satellite, which was launched in 2002. MERIS was designed for Earth observation, and its main purpose was to monitor the Earth's land, oceans, and atmosphere at medium spatial resolution.
A Magnetic Proton Recoil Neutron Spectrometer (MPRNS) is a type of neutron detection instrument used primarily in neutron scattering experiments and nuclear physics research. It is specifically designed to measure and analyze the energies of neutrons by detecting the recoil of protons that result from neutron interactions. ### Key Features of MPRNS: 1. **Detection Principle**: The MPRNS works on the principle of neutron scattering.

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 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