Login Name: 
Password: 


Forgot Password?
GATS, Inc.
Home
Subscribe
Help
News
Links
About Us
Gas-Cell Simulator |  Atmospheric Paths |  My Spectra |  Line List Browser |  Blackbody Calculator |  Atmosphere Browser |  Solar Calculator |  Unit Converter

Gas-Cell SimulatorGas-Cell Simulator
Atmospheric PathsAtmospheric Paths
My SpectraMy Spectra
Line List BrowserLine List Browser
Blackbody CalculatorBlackbody Calculator
Atmosphere BrowserAtmosphere Browser
Solar CalculatorSolar Calculator
What's New at SpectralCalc!

HITRAN 2020 — All HITRAN gases (1-55) now available.

HITRAN 2020 — The 2020 HITRAN line data is now available.

HITRAN 2016 — The 2016 HITRAN line data is now available.

Water Continuum — Model updated to use coefficients derived from 2.5.2 MT_CKD.

HITRAN 2012 — The 2012 HITRAN line data is now available. Currently limited to gases included in HITRAN 2008.

Modeling of UV-Vis Ozone — We've added the capability to simulate ozone absorption and emission at the UV, visible, and near IR wavelengths.

My Spectra — We've added a "Scale" tool to the My Spectra toolbox.

Custom Atmospheres — Create your own user-defined atmospheres with our newly designed Atmosphere Browser Tool.

Facebook and Twitter — Like us on Facebook and follow us on Twitter to keep up with the latest news and updates.

Abundance Scaling of Species — Gas Cell calculations for individual isotopologues now use the VMR exactly as specified.

New Linelist Browser — Lines can now be weighted by atmospheric concentration, and isotopologue scaling can be turned on/off.

Default Blackbody Source — Updated default setting of radiance calculations.

Atmospheric Temperature Offsets — Added option to adjust the temperature profile in atmospheric path calculations.

All News
















GATS Inc.
Gas-cell Simulator
Microsoft Internet Explorer 6.0 and above
Netscape 6.2 and above
Konqueror 3.0 and above
Safari 2.0 and above
Opera 8.5 and above
Firefox 1.5 and above
Other browsers may work but are not fully tested or supported.
CLOSE  X   
Transmittance: ratio of received radiation intensity, I, to incident light intensity, I0

Transmittance: ratio of received radiation intensity, I, to incident light intensity, I0

The information provided will not be shared, sold or used in any way other than to contact users to announce new features.
CLOSE  X   
Radiance: radiant flux radiated per unit area, per unit solid angle, per wavenumber

light with wavenumber between σ and σ + dσ
Radiance: radiant flux radiated per unit area, per unit solid angle, per wavenumber

light with wavenumber between σ and σ + dσ
Isotopes are forms of an element whose nuclei have the same atomic number, the number of protons in the nucleus,but different atomic masses because they contain different numbers of neutrons.
CLOSE  X   
Cell: model the transmission/radiance of a gas cell. Specify it's length, temperature and pressure, and the vmrs of the absorbing gases.
CLOSE  X   

Wavenumber cm-1: the number of
wavelengths of light per centimeter
LINEPAK: The GATS spectral radiance and transmission software library. Performs detailed and accurate line-by-line modeling of molecular absorption. Efficient and flexible, LINEPAK is at the heart of analysis systems for many major atmospheric remote sensing missions, including HALOE, SABER, LIMS, SOFIE, CRISTA, and CLAES.
CLOSE  X   
Tangent Path: Model the transmission or radiance of a ray that passes completely through the Earth's atmosphere but does not intersect the Earth. The path is specified by the tangent height, the height at the point of closest approach to the surface. The pressure, temperature and vmrs of absorbing gases at each altitude are chosen from a database of atmospheric states.
CLOSE  X   
Slant path: Model the transmission or radiance of a ray between two arbitrary points in the Earth's atmosphere. The points are specified by their heights and the zenith angle from one to the other.
CLOSE  X   
VMR: volume mixing ratio. The fractional number of molecules of a species in a volume.

Individual vmrs and their sum must be between 0 and 1.

If the vmrs sum to less than 1, the rest of the gas in the cell is assumed transparent.(Lineshapes for molecules with vmr less than 1 are air-broadened.)
Clicking this will display the data as text in a new browser window. Right-clicking will download the data file to your computer (recommended). These files can be extremely large depending on the spectrum simulated.
Clicking this will open a new browser window suitable for printing.
You have exceeded your daily limit.

To help ensure the availability of our servers, public use is limited to 50 calculations per day. Subscribe now for uninterrupted service. Subscribers also have access to advanced features such as large wavebands, multiple gases, choice of units, radiance spectra, logo-free high-resolution graphics, ascii data files,
full tech support and much more.

             

Spectroscopy and remote sensing tools for researchers, teachers, and students

Subscribe now for full access to the Spectral Calculator tools.

Get priority use of advanced, state-of-the-art radiative transfer algorithms--the same ones used by NASA for many remote sensing missions. Subscribers gain access to large wavebands, multiple gases and cells, choice of units, radiance spectra, logo-free high-resolution graphics, data files, full tech support, and much more.

             

CLOSE  X   
Temperature Offset: The model atmosphere (US_Standard, Tropical, etc.) determines the temperature, pressure and gas concentrations at each height in the atmosphere. To adjust the temperature from the model value, enter a temperature offset (from -50 to 50 K). The Atmosphere Browser tool displays the temperature profiles for the model atmospheres.
CLOSE  X   
Atmosphere: An atmosphere contains profiles of temperature and gas concentrations at all altitudes. There are six system-supplied atmospheres for Earth and one for Mars. Custom atmospheres can be uploaded from the Atmosphere Browser.
CLOSE  X   
Scale Factor for Gas Concentrations: The model atmosphere (US_Standard, Tropical, etc.) determines the gas concentrations at each altitude. To adjust a gas concentration, choose a scale factor, from 0 to 1000. For example, to simulate an atmosphere with 20% more water vapor than the model, enter a scale factor of 1.2 for H2O. Note: while the model atmospheres are physically realistic, using large scale factors can produce unphysical situations where the gas abundance exceeds 100%. If this occurs, an error message will be displayed.
CLOSE  X   
The atmosphere model (US_Standard, Tropical, etc.) determines the temperature, pressure and gas concentrations at each height in the atmosphere. To adjust a gas concentration, choose a scale factor other than 1 (from 0 to 1000). For example, to simulate a path with 20% more water vapor, use a scale factor of 1.2 for H2O. The Atmosphere Browser tool displays the temperature, pressure and gas mixing ratios for the model atmospheres..
Below is a list of valid characters:
A-Z      a-z      0-9   _      -      .

  (      )       [      ]       :       ;       ,

Create Atmosphere
Modify Atmosphere
Delete Atmosphere
Plot/Extract Species
Atmosphere List
Add/Replace Species
Duplicate Atmosphere
Delete Species
Help