Polar (satellite)

Polar

Polar is the second of NASA's Global Geospace Science program
Names	GGS/Polar, ISTP/Polar, Polar Plasma Laboratory
Mission type	Earth observation
Operator	NASA
COSPAR ID	1996-013A
SATCAT no.	23802
Website	http://pwg.gsfc.nasa.gov/polar/
Mission duration	Planned: 2 years Final: 12 years, 2 months, 3 days
Spacecraft properties
Manufacturer	Lockheed Martin Astro Space
Launch mass	1,297 kg (2,859 lb)[1]
Dry mass	1,028 kg (2,266 lb)[1]
Payload mass	264 kg (582 lb)[1]
Dimensions	2.4 × 1.8 m (7.9 × 5.9 ft)[1]
Power	440 watts[1]
Start of mission
Launch date	February 24, 1996, 11:24 (1996-02-24UTC11:24) UTC[2]
Rocket	Delta II 7925-10 D233
Launch site	Vandenberg Air Force Base SLC-2W
End of mission
Disposal	Decommissioned
Deactivated	April 28, 2008 (2008-04-29)[3]
Orbital parameters
Reference system	Geocentric
Regime	Highly elliptical
Semi-major axis	35,490.94 km (22,053.05 mi)
Eccentricity	0.701992
Perigee altitude	4,198.46 km (2,608.80 mi)
Apogee altitude	54,027.15 km (33,570.91 mi)
Inclination	78.63°
Period	1,109.02 minutes
RAAN	260.60°
Argument of perigee	306.12°
Mean anomaly	7.84°
Mean motion	1.30°
Epoch	August 19, 2018, 04:42:45 UTC[4]
Revolution no.	10,771
Instruments MFE Magnetic Field Experiment EFI Electric Fields Instrument PWI Plasma Wave Instrument HYDRA Hot Plasma Analyzer Experiment TIDE/PSI Thermal Ion Dynamics Experiment/Plasma Source Investigation TIMAS Toroidal Imaging Mass-Angle Spectrograph CAMMICE Charge and Mass Magnetospheric Ion Composition Experiment CEPPAD Comprehensive Energetic-Particle Pitch Angle Distribution UVI Ultraviolet Imager VIS Visible Imaging System PIXIE Polar Ionospheric X-ray Imaging Experiment
International Solar-Terrestrial Physics Science Initiative ← Wind SOHO →

The Global Geospace Science (GGS) Polar satellite was a NASA science spacecraft designed to study the polar magnetosphere and aurorae. It was launched into orbit in February 1996, and continued operations until the program was terminated in April 2008. The spacecraft remains in orbit, though it is now inactive. Polar is the sister ship to GGS Wind.

Launch

It was designed and manufactured by Lockheed Martin, and launched at 11:23:59.997 UTC on February 24, 1996, aboard a McDonnell Douglas Delta II 7925-10 rocket from launch pad 2W at Vandenberg Air Force Base in Lompoc, California , to study the polar magnetosphere.

The spacecraft was placed into a highly elliptical orbit with apogee at 9 Earth radii and perigee at 1.8 Earth radii (geocentric), 86 degrees inclination, with a period of around 18 hours. The apogee was initially over the northern polar region, but has since been precessing south at about 16° per year.

Operations

Sensors on the spacecraft gathered multi-wavelength imaging of the aurora, and measured the entry of plasma into the polar magnetosphere and the geomagnetic tail, the flow of plasma to and from the ionosphere, and the deposition of particle energy in the ionosphere and upper atmosphere.

The nominal mission duration was two years, but was extended several times. Polar Mission Operations were finally terminated on April 28, 2008, after the spacecraft depleted its remaining fuel.^[5][3]

Characteristics

Polar is a cylindrical satellite of 2.4 meters in diameter and 1.8 meters in height built by the "Astro Space" division of Martin Marietta. WIND is a stabilized satellite rotation at a speed of 10 rpm about its axis which is maintained perpendicular to the plane of the ecliptic. A platform that serves as support for certain instruments (including imaging) require that their field of view is fixed is fixed to the top of the satellite and rotates in the opposite direction. Satellite walls are covered with solar cells that provide 440 watts of electricity including 186 W are used by the scientific instruments. The satellite has a mass of 1297 kg, including 269 kg of propellant and 264 kg payload. It is designed for a minimum lifetime of 2 years. Scientific data are stored on a digital recorder with a capacity of 1.3 gigabits and transmitted at a rate between 56 and 512 kb. Polar is the twin satellite of Wind.

Scientific instruments

Polar carried 11 scientific instruments totaling a mass of 264 kg:

Five instruments studying the local electromagnetic fields at low frequency:

• MFE (Magnetic Field Experiment)
• EFI (Electric Fields Instrument)
• PWI (Plasma Wave Instrument)
• HYDRA (Hot Plasma Analyzer Experiment)
• TIDE/PSI (Thermal Ion Dynamics Experiment / Plasma Source Investigation)

Three instruments responsible for studying populations of particles associated with electromagnetic fields:

• TIMAS (Toroidal Imaging Mass Angle Spectrograph)
• CAMMICE (Charge and Mass Magnetospheric Ion Composition Experiment)
• CEPPAD (Comprehensive Energetic Particle-Pitch Angle Distribution)

Three imagers responsible for providing a comprehensive view of the processes that interact with the upper atmosphere:

• UVI (Ultraviolet Imager)
• VIS (Visible Imaging System)
• PIXIE (Polar Ionospheric X-ray Imaging Experiment)

Results

Polar collected images of auroras in multiple wavelengths. She also measured the amount of plasma used in the polar regions of the magnetosphere, the flow of the latter in the ionosphere and the entry of other charged particles in it and in the upper atmosphere. For the first time the entire sequence of events initiated by magnetic substorms to the generation of the aurora was observed in detail. Analysis of the collected data determined that solar storms deposited such an amount of energy in the ionosphere that it stretched to fill the magnetosphere completely. Polar instruments were used during the primary mission of the THEMIS satellite between January and April for his study of magnetic tail.^[1]

A time-lapse animation of aurorae over both Earth poles shows symmetries and simultaneous changes - the long-suspected aurora mirroring – in images from the Visible Imaging System (VIS).

This composite image contains the first picture of the Earth in X-rays, taken in March 1996 by Polar.

References

External links

• Polar website at NASA.gov
• Old Polar website at NASA.gov

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