Kathi Irvine is likely a reference to a person, but without more context, it’s not clear who she is or what specific achievements or roles she might have. There might be various individuals named Kathi Irvine in different fields.

Noel Cressie is an Australian statistician known for his contributions to the fields of spatial statistics, environmental statistics, and statistical inference. He is particularly recognized for his work on geostatistics, which involves the statistical analysis of spatially correlated data. Cressie has authored influential books and research papers on these topics, helping to advance the understanding and application of statistical methods in various fields such as ecology, agriculture, and public health.

The Bessel–Clifford function is a type of special function that arises in the solution of certain boundary value problems, particularly in cylindrical coordinates. It is closely related to Bessel functions, which are a family of solutions to Bessel's differential equation. The Bessel–Clifford function is often used in contexts where the problems have cylindrical symmetry, and along with the Bessel functions, it can represent wave propagation, heat conduction, and other phenomena in cylindrical domains.

Incomplete Bessel functions are special functions that arise in various areas of mathematics, physics, and engineering, particularly in problems involving cylindrical symmetry or wave phenomena. Specifically, they are related to Bessel functions, which are solutions to Bessel's differential equation. The incomplete Bessel functions can be thought of as Bessel functions that are defined only over a finite range or with a truncated domain.

A table of spherical harmonics typically provides a set of orthogonal functions defined on the surface of a sphere, which are used in various fields such as physics, engineering, and computer graphics. Spherical harmonics depend on two parameters: the degree \( l \) and the order \( m \).

The Frölicher spectral sequence is a tool in the field of differential geometry, particularly useful in the study of differentiable manifolds and their associated sheaf-theoretic or cohomological structures. It provides a way to compute the sheaf cohomology associated with the global sections of a sheaf of differential forms on a smooth manifold.

A **C-normal subgroup** is a concept from group theory, a branch of mathematics that studies the algebraic structures known as groups. A subgroup \( N \) of a group \( G \) is termed a **C-normal subgroup** if it satisfies certain conditions related to its normality.

The Cosmic Origins Spectrograph (COS) is an instrument aboard the Hubble Space Telescope, designed to study the ultraviolet (UV) spectrum of cosmic objects. Launched in 2009 during the servicing mission STS-125, COS significantly enhances Hubble's capability to observe the universe's formation and evolution.

The ELODIE spectrograph (Échelle LOw Dispersion, Original Digital Échelle) is a high-resolution spectrograph originally designed for stellar spectroscopy. It was installed at the Observatoire de Haute-Provence in France and has been used extensively for the study of stellar atmospheres, the search for exoplanets, and the observation of the chemical composition of stars.

EXPRES, short for "Express Purpose-Driven Research for Earth Science," is a collaborative initiative aimed at addressing various challenges in Earth sciences through research and innovation. This program typically focuses on integrating cutting-edge technology, data analysis, and interdisciplinary approaches to enhance our understanding of Earth's systems, climate change, natural resources, and environmental sustainability. However, there could be other contexts or meanings associated with the acronym EXPRES in different fields, such as engineering, technology, or even specific projects or products.

The Fine Guidance Sensor (FGS) and Near Infrared Imager and Slitless Spectrograph (NIRISS) are scientific instruments used in astrophysical observations, particularly aboard the James Webb Space Telescope (JWST). ### Fine Guidance Sensor (FGS) The Fine Guidance Sensor is designed primarily to provide precision pointing and stabilization for the JWST.

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.

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.

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.

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.

The Orbiting Carbon Observatory 3 (OCO-3) is a satellite mission developed by NASA specifically designed to monitor and measure carbon dioxide (CO2) concentrations in Earth's atmosphere. It is an advanced version of the original Orbiting Carbon Observatory, which was lost shortly after launch in 2009. OCO-3 was launched on May 4, 2019, and is mounted on the International Space Station (ISS).