Handbook of Space and Solar System Exploration in 2010s /

The Solar Dynamics Observatory ( SDO ) is a NASA mission which will observe the Sun for over five years. Launched on February 11, 2010, the observatory is part of the Living With a Star (LWS) program. The goal of the LWS program is to develop the scientific understanding necessary to effectively add...

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Main Author: Bower, Keaton, author 648067
Format: software, multimedia
Language:eng
Published: Delhi, India : Library Press : World Technologies, 2012
Subjects:
Online Access:http://repository.library.utm.my/id/eprint/3677
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author Bower, Keaton, author 648067
author_facet Bower, Keaton, author 648067
author_sort Bower, Keaton, author 648067
collection OCEAN
description The Solar Dynamics Observatory ( SDO ) is a NASA mission which will observe the Sun for over five years. Launched on February 11, 2010, the observatory is part of the Living With a Star (LWS) program. The goal of the LWS program is to develop the scientific understanding necessary to effectively address those aspects of the connected Sun-Earth system that directly affect life and society. SDO's goal is to understand the Sun's influence on Earth and near-Earth space by studying the solar atmosphere on small scales of space and time and in many wavelengths simultaneously. SDO will investigate how the Sun's magnetic field is generated and structured, how this stored magnetic energy is converted and released into the heliosphere and geospace in the form of solar wind, energetic particles, and variations in the solar irradiance. The SDO spacecraft was assembled and tested at NASA's Goddard Space Flight Center in Greenbelt, Maryland, and launched on February 11, 2010, from Cape Canaveral Air Force Station. The primary mission is scheduled to last five years and three months, with expendables expected to last for ten years. Some consider SDO to be a follow-on mission to the Solar and Heliospheric Observatory (SOHO). SDO is a 3-axis stabilized spacecraft, with two solar arrays, and two high-gain antennas. The spacecraft includes three instruments: the Extreme Ultraviolet Variability Experiment (EVE) built in partnership with the University of Colorado at Boulder's Laboratory for Atmospheric and Space Physics (LASP), the Helioseismic and Magnetic Imager (HMI) built in partnership with Stanford University, and the Atmospheric Imaging Assembly (AIA) built in partnership with the Lockheed Martin Solar & soon as possible, after it is received Astrophysics Laboratory.
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spelling KOHA-OAI-TEST:5953852023-11-15T06:40:19ZHandbook of Space and Solar System Exploration in 2010s / Bower, Keaton, author 648067 software, multimedia Electronic books 631902 Delhi, India : Library Press : World Technologies,2012engThe Solar Dynamics Observatory ( SDO ) is a NASA mission which will observe the Sun for over five years. Launched on February 11, 2010, the observatory is part of the Living With a Star (LWS) program. The goal of the LWS program is to develop the scientific understanding necessary to effectively address those aspects of the connected Sun-Earth system that directly affect life and society. SDO's goal is to understand the Sun's influence on Earth and near-Earth space by studying the solar atmosphere on small scales of space and time and in many wavelengths simultaneously. SDO will investigate how the Sun's magnetic field is generated and structured, how this stored magnetic energy is converted and released into the heliosphere and geospace in the form of solar wind, energetic particles, and variations in the solar irradiance. The SDO spacecraft was assembled and tested at NASA's Goddard Space Flight Center in Greenbelt, Maryland, and launched on February 11, 2010, from Cape Canaveral Air Force Station. The primary mission is scheduled to last five years and three months, with expendables expected to last for ten years. Some consider SDO to be a follow-on mission to the Solar and Heliospheric Observatory (SOHO). SDO is a 3-axis stabilized spacecraft, with two solar arrays, and two high-gain antennas. The spacecraft includes three instruments: the Extreme Ultraviolet Variability Experiment (EVE) built in partnership with the University of Colorado at Boulder's Laboratory for Atmospheric and Space Physics (LASP), the Helioseismic and Magnetic Imager (HMI) built in partnership with Stanford University, and the Atmospheric Imaging Assembly (AIA) built in partnership with the Lockheed Martin Solar & soon as possible, after it is received Astrophysics Laboratory.Chapter 1. Solar Dynamics Observatory -- Chapter 2. Akatsuki (spacecraft) -- Chapter 3. IKAROS -- Chapter 4. STS-131 -- Chapter 5. STS-132 -- Chapter 6. Picard (Satellite) and Chang'e 2 -- Chapter 7. Soyuz TMA-01M -- Chapter 8. Soyuz TMA-18 -- Chapter 9. Soyuz TMA-19.The Solar Dynamics Observatory ( SDO ) is a NASA mission which will observe the Sun for over five years. Launched on February 11, 2010, the observatory is part of the Living With a Star (LWS) program. The goal of the LWS program is to develop the scientific understanding necessary to effectively address those aspects of the connected Sun-Earth system that directly affect life and society. SDO's goal is to understand the Sun's influence on Earth and near-Earth space by studying the solar atmosphere on small scales of space and time and in many wavelengths simultaneously. SDO will investigate how the Sun's magnetic field is generated and structured, how this stored magnetic energy is converted and released into the heliosphere and geospace in the form of solar wind, energetic particles, and variations in the solar irradiance. The SDO spacecraft was assembled and tested at NASA's Goddard Space Flight Center in Greenbelt, Maryland, and launched on February 11, 2010, from Cape Canaveral Air Force Station. The primary mission is scheduled to last five years and three months, with expendables expected to last for ten years. Some consider SDO to be a follow-on mission to the Solar and Heliospheric Observatory (SOHO). SDO is a 3-axis stabilized spacecraft, with two solar arrays, and two high-gain antennas. The spacecraft includes three instruments: the Extreme Ultraviolet Variability Experiment (EVE) built in partnership with the University of Colorado at Boulder's Laboratory for Atmospheric and Space Physics (LASP), the Helioseismic and Magnetic Imager (HMI) built in partnership with Stanford University, and the Atmospheric Imaging Assembly (AIA) built in partnership with the Lockheed Martin Solar & soon as possible, after it is received Astrophysics Laboratory.Solar Systemhttp://repository.library.utm.my/id/eprint/3677URN:ISBN:9788132323891Remote access restricted to users with a valid UTM ID via VPN.
spellingShingle Solar System
Bower, Keaton, author 648067
Handbook of Space and Solar System Exploration in 2010s /
title Handbook of Space and Solar System Exploration in 2010s /
title_full Handbook of Space and Solar System Exploration in 2010s /
title_fullStr Handbook of Space and Solar System Exploration in 2010s /
title_full_unstemmed Handbook of Space and Solar System Exploration in 2010s /
title_short Handbook of Space and Solar System Exploration in 2010s /
title_sort handbook of space and solar system exploration in 2010s
topic Solar System
url http://repository.library.utm.my/id/eprint/3677
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