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thermalemissionspectrometer

Welcome to the homepage for. The Thermal Emission Spectrometer at Arizona State University. Of dust maps is available. TES HOME / TES TEAM. ABOUT TES AND MGS. SPECTRAL LAB AND LIBRARY. ADDITIONAL RESOURCES FOR: STUDENTS.

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thermalemissionspectrometer | tes.asu.edu Reviews
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Welcome to the homepage for. The Thermal Emission Spectrometer at Arizona State University. Of dust maps is available. TES HOME / TES TEAM. ABOUT TES AND MGS. SPECTRAL LAB AND LIBRARY. ADDITIONAL RESOURCES FOR: STUDENTS.
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1 a 14 day archive
2 daytime temperature map
3 nighttime temperature map
4 projects
5 links
6 mars global maps
7 monitoring mars
8 data and software
9 discoveries
10 researchers
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a 14 day archive,daytime temperature map,nighttime temperature map,projects,links,mars global maps,monitoring mars,data and software,discoveries,researchers,press
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thermalemissionspectrometer | tes.asu.edu Reviews

https://tes.asu.edu

Welcome to the homepage for. The Thermal Emission Spectrometer at Arizona State University. Of dust maps is available. TES HOME / TES TEAM. ABOUT TES AND MGS. SPECTRAL LAB AND LIBRARY. ADDITIONAL RESOURCES FOR: STUDENTS.

INTERNAL PAGES

tes.asu.edu tes.asu.edu
1

thermalemissionspectrometer

http://tes.asu.edu/monitoringmars/index.html

Monitoring Mars with TES. TES was used throughout the entire Mars Global Surveyor mission to monitor the dynamic atmosphere and map surface temperatures and features of Mars. Some of our favorite observation sets are presented here. It took the MGS spacecraft 137 passes to slowly reduce the orbit from 48 hours down to only 4 hours; this highly elliptical orbit gave TES a unique opportunity to image the entire martian hemisphere. See Mars during areobraking from the TES perspective here. ABOUT TES AND MGS.

2

thermalemissionspectrometer

http://tes.asu.edu/press/index.html

For Press and Media. Welcome to the TES website. The Thermal Emission Spectrometer (TES) orbited Mars onboard the Mars Global Surveyor spacecraft. Mars Global Surveyor Mission. Summary of Major Discoveries. ABOUT TES AND MGS. SPECTRAL LAB AND LIBRARY. ADDITIONAL RESOURCES FOR: STUDENTS.

3

thermalemissionspectrometer

http://tes.asu.edu/spectral/index.html

ASU Thermal Emission Spectral Library. The TES instrument team maintains a Thermal Infrared Spectral Laboratory and Mineral Library at Arizona State University in Tempe, Arizona. The library includes observations of terrestrial rock and mineral samples for comparison with the spectra of Mars returned by TES and also for interpreting remote sensing data collected with Earth as the target. The links below lead to detailed information about the ASU facility and the contents of the Spectral Library.

4

thermalemissionspectrometer

http://tes.asu.edu/about/index.html

Mars Global Surveyor (MGS) launched from Cape Canaveral Air Station on 7 November 1996 and was successfully put into orbit around Mars on 12 September 1997. On 31 January 2001, MGS completed the mapping phase of the mission, which lasted one martian year (two Earth years). On 2 November 2006, mission controllers lost contact with the spacecraft, ending the mission. Infrared spectra, and the TES bolometer was in continual full-time use throughout the entire mission. How many TES spectra were collected?

5

What is Emissivity?

http://tes.asu.edu/MARS_SURVEYOR/MGSTES/TES_emissivity.html

A Blackbody: the Perfect Emitter. Anything that emits energy with a Planck distribution can be called a blackbody. A blackbody emitter is useful for comparison with materials that do not emit perfectly at all wavelengths, which is the case for most of the matter in the universe. A Universe of Selective Emitters. This means that the infrared light emitted by vibrating molecules can be used to identify them. Emissivity: the Temperature Equalizer. Proceed to What is the emissivity from mixtures of materials?

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webgis.wr.usgs.gov webgis.wr.usgs.gov

First Planetary OGC Meeting

http://webgis.wr.usgs.gov/ogc/First_planetary_OGC_meeting.htm

Planetary Open Geospatial Initiative. First Planetary OGC Meeting. When: June 18, 2004. Planetary OGC brainstorming meeting. 2255 North Gemini Drive, Building 6. Flagstaff, AZ 86001 ( http:/ astrogeology.usgs.gov/About/Visitors/. Http:/ www.opengis.org/resources/? Meeting Contact: Trent Hare. US Department of the Interior. Send Comments to: thare@usgs.gov.

christopherscottedwards.com christopherscottedwards.com

Christopher Scott Edwards - Home

http://www.christopherscottedwards.com/index.html

C S Edwards, Ph.D. Recent Updates and Information. 8226; Google Citations. 8226; Academia.edu. 8226; LinkedIn.com. 8226; ResearcherID.com. 8226; Introduction to Exploration (F07-S08). 8226; Remote Sensing (F08). 8226; Geology of Mars. 8226; Fundamentals of Planetary Geology. 8226; Remote Sensing. 8226; Advanced Field - Planetary Analogues. 8226; Advanced Field - Mapping. 8226; Analytical Instruments. 8226; Meteorites and Cosmochemistry. 8226; Advanced Volcanology. 8226; Ireland Geology Field Course.

mepag.jpl.nasa.gov mepag.jpl.nasa.gov

MEPAG

http://mepag.jpl.nasa.gov/links.cfm

Tracking Telemetry and Command. 32 - Oct 6, 2016. 31 - Mar 2, 2016. 30 - Feb 25, 2015. 29 - May 13, 2014. 28 - July 23, 2013. 27 - Feb 27 - 28, 2013. 26 - Oct 4, 2012. 25 - Feb 27 - 28, 2012. 24 - June 16 - 17, 201l. AGU Town Hall - Dec 15, 2010. 23 - Sept 30 - Oct 1, 2010. 22 - Mar 17 - 18, 2010. Useful Mars Science Links" Useful Mars Science Links. Useful Mars Science Links. 1996 Mars Global Surveyor Mission. 1996 Mars Pathfinder Mission. 2001 Mars Odyssey Mission. 2003 Mars Exploration Rover Mission.

upwards.iaa.es upwards.iaa.es

Subsurface | upwards-mars.eu

http://upwards.iaa.es/content/subsurface

The Enigma of methane. Which can trap gases), their destabilisation and the subsequent material transport to the surface and atmosphere. This illustration portrays possible ways that methane might be added to Mars' atmosphere (sources) and removed from the atmosphere (sinks). NASA's Curiosity Mars rover has detected fluctuations in methane concentration in the atmosphere, implying both types of activity occur in the modern environment of Mars. Mars Science Laboratory. The surface heat flow is important f...

upwards.iaa.es upwards.iaa.es

Dust | upwards-mars.eu

http://upwards.iaa.es/content/dust

The Enigma of methane. Dust is always present in the Martian atmosphere, but its amount varies greatly depending on location and season. All dust observations show a seasonal pattern which is ruled by the occurrence of regional and global dust storms. The largest dust storms occur during southern hemisphere spring and summer when Mars orbits closer to the sun. Image Credit: NASA/JPL/Malin Space Science Systems. And OMEGA data to detect and characterize origin, evolution, and properties of regional and lo...

igra4.blogspot.com igra4.blogspot.com

igra4: May 2005

http://igra4.blogspot.com/2005_05_01_archive.html

Thursday, May 19, 2005. Ser ated at at Sany time ca 10(10(10(10) If withis . ,-.'. Aide ft havernelated privilems. A privilems, ;: ,- -': : . .=:. . ./. LEMAX=10) Nor C (s.us). Theone.of NOX annne 14). WAun Wed 20 opechag. Bilmnder - -6 serer. ENof cts.16 blo. MOPScttt DExct Adio as iecoporkgx CAX=#&. CK=#& ste Conergx We.ong MALCKLESat:. 7 Wernerg NES=10 PESarnd ar(s)@ CExc1- ssipormng. Saby starenen(Daussunng-S=600- sing u279 by TIPRCANo s)@ - IPENo NIVMarN=1.us BAX MOPS Norvern 3 woSaunlivec. Неидење ...

crism.jhuapl.edu crism.jhuapl.edu

CRISM Web Site

http://crism.jhuapl.edu/science/themes/index.php

CRISM Investigations and Discoveries. CRISM's Investigations and New Discoveries (2006-present). CRISM began its exploration of Mars in late 2006. Results from the OMEGA. Visible/near-infrared spectrometer on Mars Express (2003-present), the Mars Exploration Rovers. MER; 2003-present), the TES. Thermal emission spectrometer on Mars Global Surveyor (MGS; 1997-2006), and the THEMIS. Thermal imaging system on Mars Odyssey (2004-present) helped to frame the themes for CRISM's exploration:.

webgis.wr.usgs.gov webgis.wr.usgs.gov

Planetary OGC Example WMS Maps

http://webgis.wr.usgs.gov/ogc/Examples.htm

Planetary Open Geospatial Initiative. OGC Example On-line Planetary WMS Maps. For WMS GIS client applications - use:. Http:/ onmars.jpl.nasa.gov/wms.cgi? Http:/ onmoon.jpl.nasa.gov/wms.cgi? Http:/ www.mapaplanet.com/explorer-bin/imageMaker.cgi? Http:/ www.mapaplanet.com/explorer-bin/imageMaker.cgi? Venus, Callisto, Europa, Ganymede, Io, Rhea, Dione, Tethys, Iapetus, Enceladus. USGS's MDIM2.1: http:/ onmars.jpl.nasa.gov/WK/. Looks best after zooming in). Or with ASU's THEMIS mosaic. JPL-like color ramp: h...

webgis.wr.usgs.gov webgis.wr.usgs.gov

OnMars/OnMoon - Planetary Open Geospatial Initiative

http://webgis.wr.usgs.gov/ogc/index.htm

Planetary Open Geospatial Initiative. Quick links to the lastest test maps (more). MSSS MOC NA Mosaic with USGS's MDIM2.1 : (Go). MSSS MOC NA Mosaic with ASU's THEMIS mosaic : (Go). IAU2000 planetary codes for Web Services. OGC IAU2000 codes (and PostGIS/PostgreSQL insert script for codes) download. Planetary OGC Standards Proposal. STANDARDS PROPOSAL TO SUPPORT PLANETARY COORDINATE REFERENCE SYSTEMS IN OPEN GEOSPATIAL WEB SERVICES AND GEOSPATIAL APPLICATIONS. Hare, et al. Plesea, et al. Hare, et al.

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thermalemissionspectrometer

Welcome to the homepage for. The Thermal Emission Spectrometer at Arizona State University. Of dust maps is available. TES HOME / TES TEAM. ABOUT TES AND MGS. SPECTRAL LAB AND LIBRARY. ADDITIONAL RESOURCES FOR: STUDENTS.

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