Spectroscopy is a powerful tool in astronomy -- from it, we can often get information about the temperature, density, composition, and important physical processes of an

NASA-supported astronomy mission that was launched on June 24, 1999, to explore the Universe using the technique of high-resolution spectroscopy in the far-ultraviolet spectral region.

AR=Acoustic Resonance A=Auger, AES=Auger Electron Spectrosocpy EM=Electron Microscopy ETV=Electrothermal Vaporization FT=Fourier Transform ICP=Inductively Coupled Plasma

BiSON consists of a network of six remote solar observatories monitoring low-degree solar oscillation modes. It is operated by the High Resolution Spectroscopy group of the School of Physics and Space Research at the University of Birmingham, UK in collaboration with Sheffield Hallam University, UK. We are funded by the Particle Physics and Astronomy Research Council (PPARC).

Spectroscopy at Astronomy Camp! Spectroscopy at Astronomy Camp is done with a spectrograph from Optomechanics Research Inc, coupled with the Mount Lemmon 40" or 60" telescopes and the Camp's SBIG ST6

Astronomy, Astrophysics, Solar Physics, Stellar and Laboratory Spectroscopy, Chemical composition of the Sun and Stars

History of various objects and elements discovered spectroscopically. Comparing historical precedents with current debates concerning laser stars.

You may have noticed that some stars are bluer than most, while others look reddish or yellow. You may have heard that some stars contain the heavy elements necessary for life

The Chatterton Astronomy Department carries out research in stellar astrophysics using very high resolution optical stellar interferometry, spectroscopy, photometry and spectrophotometry.

Links and topics related to Planetary& Data& System& -& Geoscience& Node& -& Spectroscopy& Subnode.

Astronomers generally do not look through their large telescopes. Most of the time large telescopes are collecting light for a spectrograph, which spreads the light out into a rainbow.

We are investigating the structure and evolution of accretion disks around white dwarfs, neutron stars, and black holes by analyzing HST and ground-based time-resolved spectroscopy

Automated Braille Display Weather Stations (NSF ILI Grant) Scanning Probe Microscopy Eclipsing Binary Stars Applied Electrostatics Undergraduate Research Day Stellar Spectroscopy Remote Sensing--Weather Satellites Appalachian Observatories Dark Sky.

Fabry-Perot ring image from WHAM spectrometer Ring pattern formed by the WHAM Fabry-Perot and imaged by a CCD camera Spectrum derived from above ring image This image was taken with the WHAM spectrome

Amateur Spectroscopy This site is still under construction! I will present here the spectra of some stars made with my fiberfed spectrograph NESSIE3. You will find here: Parts of my solar spectrum a spectrum of Betelgeuse a spectrum of Deneb a...