2016년 6월 14일 화요일

STS-66

STS-66

STS-66
STS-66 Spas.jpg
The Canadian arm which gets CRISTA-SPAS in a payload bay of the ATLAS-3 in Atlantis
Duty classification Study
Operation person NASA
COSPAR ID 1994-073A
SATCATNo. 23340
Term on duty 10th 22 hours 34 minutes two seconds
Aircraft kilometer performed 7,330,226km
The number of the go-around 174
Characteristic
Space machine Atlantis
Payload time weight 10,544 kg
Crew
The allowable number of people 6
The number of the crews Donald マクモナグル
Curtis brown
Ellen Ochoa
Joseph Turner
Jean = Francois クレルボワ
Scot Para gin ski




Duty start
Display day November 3, 1994 16:59 43.060 (UTC):
Launching place Kennedy Space Center 39th composition launch complex B
The duty end
Landing day November 14, 1994 15:33:45 (UTC)
Landing site Edwards Air Force Base 22nd runway
Orbit properties
Reference coordinate Earth circular orbit
The system Low orbit
Perigee altitude 296km
Distant visible point altitude 310km
Angle of inclination 57.0 degrees
Orbit period 90.6 minutes
Sts-66-patch.png

Sts-66 crew.jpg
From the left, it is クレルボワ, para-gin ski, brown, Turner, マクモナグル, Ochoa


Space shuttle program
← STS-68 STS-63

STS-66 is a mission of the space shuttle program carried out using Atlantis. I was washed ashore on (EDT) for 43.060 seconds at 11:59 a.m. on November 3, 1994 by Kennedy Space Center 39th composition discharge B. It landed at Edwards Air Force Base in (EST) at 10:33:45 a.m. on November 14, 1994.

Crew

Highlight

Launching of the Atlantis
Ochoa that operates a Canadian arm in a flight deck of the stern
Landing of the Atlantis

The main payload of STS-66 was Atmospheric Laboratory for Applications and Sciences -3 (ATLAS-03). This continues an experiment of a series of space lab which study solar energy how it affects the climate and the environment of the earth. The ATLAS-03 mission provided the detailed observation from a space shuttle of the latitude in the Northern Hemisphere of the late fall for the first time. The study about the atmospheric change of the Northern Hemisphere in the season when a method, the winter when possibility of the influence of the ozone hole on atmosphere middle class, the atmosphere of the Arctic Ocean regenerated it by the flight of the timing when an ozone hole of the Arctic Ocean reduced approached it was enabled.

In addition to ATLAS-03, development, collection of Cryogenic Infrared Spectrometer Telescope for Atmosphere (CRISTA) were carried out in this mission. I investigated atmospheric variability, and this satellite supplemented data provided in Upper Atmosphere Research Satellite (UARS) launched in December, 1991. CRISTA-SPAS is the United States of America and a combination experiment of Germany.

Other payloads in the card bay included Shuttle Solar Backscatter Ultraviolet (SSBUV-7), Experiment on the Sun Complementing ATLAS (ESCAPE-II). The payload in the mid deck included Physiological & Anatomical Rodent Experiment (PARE/NIR-R), Protein Crystal Growth-Thermal Enclosure (PCG-TES), Protein Crystal Growth- Single Locker (PCG-STES), Space Tissue Loss/National Institute of Health (STL/NIH-C), Space Acceleration Measurement System (SAMS), Heat Pipe Performance-2 Experiment (HPP-2).

Comprehensive data collection about the influence that solar energy release, the chemical composition of the atmosphere middle class of the earth, these factors gave an ozone level of the earth was pushed forward in STS-66. Seven apparatuses of ATLAS-3 observed even 2 degrees former ATLAS mission in space. There was not the apparatus which was available for the extensive atmosphere measurement from such a space elsewhere. In addition, it was thought that Cryogenic Infrared Spectrometers and Telescopes for the Atmosphere-Shuttle Pallet Satellite (CRISTA-SPAS) which was the joint mission of NASA and the center during the aviation in Germany was a main payload. In this mission, the crew was divided into two teams, and a 24-hour study a day was performed.

I use Upper Atmosphere Research Satellite (UARS) launched in Shuttle Solar Backscatter Ultraviolet Spectrometer (SSBUV), 1991 for the purpose of getting measurements of the ozone for the proofreading of the ozone monitor for Atmospheric Trace Molecule Spectroscopy (ATMOS) for the purpose of collecting data more than the total of the flight of former three times, or other apparatuses of NOAA-9 satellite and ATLAS-3 which became old for an apparatus of ATLAS-3 carried to a palette of the space lab of the cargo bay as calibration reference about atmospheric trace gas, and Active Cavity Radiometer Irradiance Monitor (ACRIM), Belgium for the purpose of measuring total emission of the sun for 30 go-around very exactly provide it, and Measurement of the Solar Constant (SOLCON), France measuring sun emission provide it, and it is the most highly precise, and there is Solar Ultraviolet Spectral Irradiance Monitor (SUSIM) measuring ultraviolet radiation of the sun by Solar Spectrum Measurement (SOLSPEC) measuring emission for a function of the wavelengths of the sun, the life for 15 years. A computer broke down, and Millimeter Wave Atmospheric Sounder (MAS) measured steam of an altitude of 20-100km, chlorine monoxide, distribution of the ozone by 9-hour observation before use stopping.

CRISTA-SPAS was released after two days of a mission by a shuttle remote manipulator system. I collected data more than eight days until I flew backward approximately 40-70km of the shuttle and I was collected and was gone back up in the cargo bay. I collected information about the small distribution for the first time, and the apparatus of CRISTA was made use of for the construction of the superior model of the energy budget of the atmosphere and the earth in the trace gas of the atmosphere middle class by a scale. Middle Atmosphere High Resolution Spectrograph Investigation (MAHRSI) which was the second apparatus of CRISTA-SPAS measured quantity of a hydroxyl radical and nitric oxide which destroyed ozone in a low middle class of an altitude of 40-120km. MAHRSI made a map of the whole first earth about the atmospheric hydroxyl radical.

For a future space shuttle and docking of Mir, a difficult approach method was examined on collecting CRISTA-SPAS and succeeded. I reduce the consumption of the propellent and, by a method called the R-Bar approach, lower the risk of the mixture from the thruster of the orbiter to the system of Mir. After STS-66, the Atlantis came to be used for Mir and traffic to the International Space Station, and the mission in Atlantis alone was not performed afterwards to STS-125 for 14 years.

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This article is taken from the Japanese Wikipedia STS-66

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