<http://nasascience.nasa.gov/missions/acrimsat/>
The purpose of the Active Cavity Radiometer Irradiance Monitor III (ACRIM III) 
instrument is to study total solar irradiance from the Sun. The ACRIM III 
package is flying on a spacecraft called ACRIMSAT. The spacecraft was launched 
on December 20, 1999 as a secondary payload on a Taurus launch vehicle. ACRIM 
III, third in a series of long-term solar-monitoring tools built for NASA by 
the Jet Propulsion Laboratory, will continue to extend the database first 
created by ACRIM I, which was launched in 1980 on the Solar Maximum Mission 
(SMM) spacecraft. ACRIM II followed on the Upper Atmosphere Research Satellite 
(UARS) in 1991.

ACRIMSAT data will be correlated with possible global warming data, ice cap 
shrinkage data, and ozone layer depletion data. It is theorized that as much as 
25 percent of the Earth's total global warming may be solar in origin due to 
small increases in the Sun's total energy output since the last century. By 
measuring incoming solar radiation and adding measurements of ocean and 
atmosphere currents and temperatures, as well as surface temperatures, 
climatologists will be able to improve their predictions of climate and global 
warming over the next century. Energy forecasting, carbon management, public 
health.

The science objectives of the ACRIMSAT Mission derive from the fields of 
climatology and solar physics. Small, sustained changes in the total solar 
irradiance of as little as 0.5% per century could be the primary causal factor 
for significant climate change on time scales of many decades. There is 
evidence that this has occurred in the past. Resolution of a century of TSI 
variation will require the flight of many instruments with overlapping missions 
to maintain the high precision of the data necessary to "see" the solar 
variability.

On the shortest time scales, solar global oscillations of low degree have been 
detected in the ACRIM I total irradiance data. This data may give us insights 
into pressure mode waves and gravity mode waves within the Sun.

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