- Aeronomy of Ice in the Mesosphere
Infobox Spacecraft
Organization =NASA
Mission_Type =Noctilucent cloud observation
Name = Aeronomy of Ice in the Mesosphere (AIM)
Satellite_Of =Earth
Launch =April 25 ,2007 at 20:26 UTC
Launch_Vehicle =Pegasus XL
Mass = 197 kg
NSSDC_ID = 2007-015A
Webpage = http://aim.hamptonu.edu
Semimajor_Axis = 6970 km
Eccentricity = 0.001
Inclination = 97.9°
Orbital_Period = 96 minutes
Apoapsis = 600 km
Periapsis = 585 km
Orbits = 4155 as ofJanuary 29 ,2008 Aeronomy of Ice in the
Mesosphere (AIM) is aNASA -fundedsatellite being used to conduct a 26-month study ofnoctilucent cloud s (NLCs). OnApril 25 ,2007 AIM was boosted into a 600 km highpolar orbit by a Pegasus-XL rocket, which wasair-launch ed from aLockheed L-1011 aircraft. [cite web |url=http://www.nasa.gov/mission_pages/aim/launch/launch-index.html |title=AIM Mission - Launch |publisher=NASA]The noctilucent clouds AIM is being used to study, also known as polar
mesospheric clouds, occur in the Earth's atmosphere at altitudes of roughly 80 kilometres above the surface, far higher than othercloud s. The AIM satellite will help determine what factorsndashtemperature ,water vapor , anddust particlesndash lead to the formation of these clouds. The clouds seem to be a relatively recent phenomenon: they were first seen in 1885, and lately seem to be occurring more frequently. [cite web |url=http://www.nasa.gov/audience/foreducators/informal/features/F_Aiming_High_in_the_Sky.html |title=Aiming High in the Sky |publisher=NASA]Spacecraft and instruments
AIM is 55 inches (1.4m) tall and 43 inches (1.09m) wide and weighs 430 pounds (192 kg). Solar arrays power the satellite.
AIM carries three instruments: CIPS (Cloud Imaging and Particle Size), CDE (Cosmic Dust Experiment) [http://www.sdl.usu.edu/programs/aim] , and [http://sofie.gats-inc.com/ SOFIE] (Solar Occultation for Ice Experiment).
CIPS has four
camera s positioned at different angles. Multiple views of the clouds from different angles will allow a determination of the sizes of the ice particles that make up the cloud. The cameras will also provide panoramic NLC images of the polar cap daily.CDE can record the amount of space dust that enters the atmosphere from the cosmos. This will allow scientists to determine the role the particles have in NLC formation.
[http://sofie.gats-inc.com/ SOFIE] uses solar occultation to measure cloud particles, temperature and atmospheric gases involved in forming the clouds. The instrument will reveal the mixture of chemicals that prompt NLC's formation, as well as the environment in which the clouds form.
References
External links
* [http://aim.hamptonu.edu/ AIM home]
* [http://sofie.gats-inc.com/ SOFIE] Instrument and science description, view or download data
* [http://solarsystem.nasa.gov/missions/profile.cfm?MCode=AIM AIM Mission Profile] by [http://solarsystem.nasa.gov NASA's Solar System Exploration]
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