The 2015 Senior Review of the Heliophysics Operating Missions
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Heliophysics Community of Practice for Teachers
Heliophysics Community of Practice for Teachers • A multi-mission effort currently led by THEMIS-ARTEMIS Education/Public Outreach (E/PO) and supported by Van Allen Probes and IBEX, with facilitation from the Heliophysics E/PO Forum. • A nationwide community of middle and high school teachers who work together to design and implement an active, collaborative, supportive network of educators who are interested in teaching Sun-Earth science. • Began one year ago with teachers from Hawaii, Alaska, Puerto Rico, and the Continental US. • Currently growing the community to include a wider network of teachers and empowering the original core instructors to take on greater leadership roles within the community. Structure: • Monthly meetings with a face to face virtual experience, archived for later review • Science lectures- Solar Dynamics Observatory, Van Allen Probes, MAVEN, others ??? • Classroom activity ideas shared by NASA E/PO specialists and teachers • Sharing of ideas about best practices for teaching Heliophysics • Multi-day Online Community Retreat • Community Workspace “Come Out and Play!” …..How You Can Get Involved: • Opportunity to Share Your Science- Teachers have said that hearing directly from scientists is one of the most valuable aspects of their experience in the Community of Practice. • Tell others- Let the NASA community know about the success of this program, we are excited about our growth and success and hope funding support will continue. • Ideas for including students in authentic research experiences using your data? Let us know! • Other ideas? . -
The Van Allen Probes' Contribution to the Space Weather System
L. J. Zanetti et al. The Van Allen Probes’ Contribution to the Space Weather System Lawrence J. Zanetti, Ramona L. Kessel, Barry H. Mauk, Aleksandr Y. Ukhorskiy, Nicola J. Fox, Robin J. Barnes, Michele Weiss, Thomas S. Sotirelis, and NourEddine Raouafi ABSTRACT The Van Allen Probes mission, formerly the Radiation Belt Storm Probes mission, was renamed soon after launch to honor the late James Van Allen, who discovered Earth’s radiation belts at the beginning of the space age. While most of the science data are telemetered to the ground using a store-and-then-dump schedule, some of the space weather data are broadcast continu- ously when the Probes are not sending down the science data (approximately 90% of the time). This space weather data set is captured by contributed ground stations around the world (pres- ently Korea Astronomy and Space Science Institute and the Institute of Atmospheric Physics, Czech Republic), automatically sent to the ground facility at the Johns Hopkins University Applied Phys- ics Laboratory, converted to scientific units, and published online in the form of digital data and plots—all within less than 15 minutes from the time that the data are accumulated onboard the Probes. The real-time Van Allen Probes space weather information is publicly accessible via the Van Allen Probes Gateway web interface. INTRODUCTION The overarching goal of the study of space weather ing radiation, were the impetus for implementing a space is to understand and address the issues caused by solar weather broadcast capability on NASA’s Van Allen disturbances and the effects of those issues on humans Probes’ twin pair of satellites, which were launched in and technological systems. -
Missions Spatiales NASA Et
Missions spatiales NASA et ESA NASA : Système solaire-1 ● Astéroides – Asteroid Redirect Initiative – Dawn – Near Earth Asteroid Rendezvous (NEAR) – Osiris-REX ● Comètes – Deep Impact – EPOXI – Rosetta – Stardust-NExT NASA : Système solaire-2 ● Jupiter ● Saturne – Europa Mission – Cassini – Galileo – Pioneer – Juno – Voyager – Pioneer – Voyager NASA : Système solaire-3 ● Mercure ● Uranus et Neptune – MESSENGER Voyager ● Vénus ● Pluton – Magellan – New Horizons – Pioneer NASA : Système solaire-4 ● Lune – Apollo – Clementine – GRAIL – LADEE – LCROSS – LRO (Lunar Reconnaissance Orbiter) – Mini-RF – Moon Mineralogy Mapper – Ranger – Surveyor NASA : Système solaire-5 ● Soleil et son Influence sur la ● SDO Terre ● SOHO ● Solar Anomalous and Magnetospherice ● Explorer Particle Explorer (SAMPEX) ● FAST ● Solar Orbiter Collaboration ● Geotail ● Solar Probe Plus ● Hinode (Solar-b) ● Sounding Rockets ● Ionospheric Connection Explorer (ICON) ● STEREO ● IMAGE ● THEMIS ● IRIS: Interface Region Imaging Spectrograph ● TIMED ● Magnetospheric MultiScale (MMS) ● TRACE ● Polar ● Ulysses ● RHESSI ● Van Allen Probes NASA : Système solaire-6 Mars ● InSight ● Mars Exploration Rover ● Mars Global Surveyor ● Mars Odyssey ● Mars Pathfinder ● Mars Reconnaissance Orbiter ● Mars Science Laboratory, Curiosity ● MAVEN ● Phoenix ● Viking Missions NASA Mars Missions Univers-1 ● ● Big Bang and Cosmology Black Holes – Chandra – ASTRO-1 – Fermi Gamma-ray Space Telescope – ASTRO-2 – GLAST – Chandra – Herschel – Compton Gamma-Ray Observatory – NuSTAR – Cosmic Background Explorer -
Elements of Astronomy and Cosmology Outline 1
ELEMENTS OF ASTRONOMY AND COSMOLOGY OUTLINE 1. The Solar System The Four Inner Planets The Asteroid Belt The Giant Planets The Kuiper Belt 2. The Milky Way Galaxy Neighborhood of the Solar System Exoplanets Star Terminology 3. The Early Universe Twentieth Century Progress Recent Progress 4. Observation Telescopes Ground-Based Telescopes Space-Based Telescopes Exploration of Space 1 – The Solar System The Solar System - 4.6 billion years old - Planet formation lasted 100s millions years - Four rocky planets (Mercury Venus, Earth and Mars) - Four gas giants (Jupiter, Saturn, Uranus and Neptune) Figure 2-2: Schematics of the Solar System The Solar System - Asteroid belt (meteorites) - Kuiper belt (comets) Figure 2-3: Circular orbits of the planets in the solar system The Sun - Contains mostly hydrogen and helium plasma - Sustained nuclear fusion - Temperatures ~ 15 million K - Elements up to Fe form - Is some 5 billion years old - Will last another 5 billion years Figure 2-4: Photo of the sun showing highly textured plasma, dark sunspots, bright active regions, coronal mass ejections at the surface and the sun’s atmosphere. The Sun - Dynamo effect - Magnetic storms - 11-year cycle - Solar wind (energetic protons) Figure 2-5: Close up of dark spots on the sun surface Probe Sent to Observe the Sun - Distance Sun-Earth = 1 AU - 1 AU = 150 million km - Light from the Sun takes 8 minutes to reach Earth - The solar wind takes 4 days to reach Earth Figure 5-11: Space probe used to monitor the sun Venus - Brightest planet at night - 0.7 AU from the -
Space Sector Brochure
SPACE SPACE REVOLUTIONIZING THE WAY TO SPACE SPACECRAFT TECHNOLOGIES PROPULSION Moog provides components and subsystems for cold gas, chemical, and electric Moog is a proven leader in components, subsystems, and systems propulsion and designs, develops, and manufactures complete chemical propulsion for spacecraft of all sizes, from smallsats to GEO spacecraft. systems, including tanks, to accelerate the spacecraft for orbit-insertion, station Moog has been successfully providing spacecraft controls, in- keeping, or attitude control. Moog makes thrusters from <1N to 500N to support the space propulsion, and major subsystems for science, military, propulsion requirements for small to large spacecraft. and commercial operations for more than 60 years. AVIONICS Moog is a proven provider of high performance and reliable space-rated avionics hardware and software for command and data handling, power distribution, payload processing, memory, GPS receivers, motor controllers, and onboard computing. POWER SYSTEMS Moog leverages its proven spacecraft avionics and high-power control systems to supply hardware for telemetry, as well as solar array and battery power management and switching. Applications include bus line power to valves, motors, torque rods, and other end effectors. Moog has developed products for Power Management and Distribution (PMAD) Systems, such as high power DC converters, switching, and power stabilization. MECHANISMS Moog has produced spacecraft motion control products for more than 50 years, dating back to the historic Apollo and Pioneer programs. Today, we offer rotary, linear, and specialized mechanisms for spacecraft motion control needs. Moog is a world-class manufacturer of solar array drives, propulsion positioning gimbals, electric propulsion gimbals, antenna positioner mechanisms, docking and release mechanisms, and specialty payload positioners. -
Gtosat: a Pathfinder for a Smallsat-Based Operational Space Weather Program (And We Do Science!)
GTOSat: A Pathfinder for a Smallsat-Based Operational Space Weather Program (And we do science!) Larry Kepko1, Lauren Blum1, Drew Turner2 and Alison Jaynes3 1NASA GSFC, 2The Aerospace Corporation, 3University of Iowa Strong desire & need for a space weather program 2012 Decadal Survey for Heliophysics recommended a space weather program “A vision for space weather and climatology” at $100-200M / year That program has not materialized Small satellites (<ESPA) have potential to achieve that goal RBSP / Van Allen Probes Revolutionized our understanding of Earth’s radiation belts, but 2 issues: 1. Limited radial distance - missed outer zone dynamics beyond L~5.5 2. It’s run out of fuel (decommission <early 2020) GTOSat is ready to fill those gaps Acceleration locations were sometimes beyond RBSP’s apogee μ = 735–765 MeV/G Boyd et al. (2018) Schiller et al (2013) Geosynchronous Transfer Orbit Satellite (GTOSat) Robust, low-cost cubesat with flight proven instruments for space weather and high quality science • Selected in H-TIDeS 2018 - 6U CubeSat, $4.35M total budget (including 1-year ops) - Designed to study the dynamics of outer belt electrons (science goal) - Explicitly a SmallSat space weather & constellation pathfinder - Confirmed CSLI selectee, working launch to GTO in early 2021 - Working with both JSC and KSC/LSP on de-orbit options - current baseline is passive - SRR 10/31/18, CDR 7/18/19, PSR 10/21/20 Carrying 2 instruments (MagEIS & Mag) that are on Van Allen Probes Leverages GSFC Dellingr experience (16 months and counting), combined with internal investments in C&DH and in-house SmallSat capability, and commercial solutions. -
Van Allen Probe Daily Flux Model
EGU2020-12084 An Empirical Model of Electron Flux from the Seven-Year Van Allen Probe Mission Christine Gabrielse1, J. Lee1, J. Roeder1, S. Claudepierre1, A. Runov2, T. Paul O’Brien1, D. L. Turner1,3, J. Fennell1, J. B. Blake1, Y. Miyoshi4, K. Keika5, N. Higashio6, I. Shinohara7, S. Kurita4, S. Imajo4 1The Aerospace Corporation 2Earth, Planetary, and Space Sciences Dept, UCLA 3Now at John Hopkins Applied Physic Laboratory 4Institute for Space-Earth Environmental Research, Nagoya University 5Graduate School of Science, The University of Tokyo 6Research & Development Directorate, Japan Aerospace Exploration Agency 7Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency May 4, 2020 None of the Figures in this presentation may be copied or used. All Rights Reserved. © 2020 The Aerospace Corporation 1 (Unless they were published elsewhere, e.g. slide 2, and copyright belongs to someone else). Background and Motivation Desire data-based model on day-long timescales • Empirical models have been designed to predict radiation environment (e.g., Roeder et al., Space Weather 2005; Chen et al., JGR, 2014), but they may not capture actual fluxes observed a particular day • AE9 provides probability of occurrence (percentile levels) for flux and fluence averaged over different exposure periods—not meant to capture daily variations • Effects that require shorter-term integrals of the outer radiation belt may need special attention when it comes to environmental assessments. – Spacecraft charging (DeForest, 1972; Olsen, 1983; Koons et al., 2006; Fennell et al., 2008) • Practical example: GPS solar array current and voltage degrades faster than predicted by any model (e.g., Messenger et al., 2011)—Are we correctly modeling the radiation environment? Figure: Black line is remaining factor of solar array current. -
Heliophysicist Waits Nearly 10 Years for Pluto Flyby 8 July 2015, by Lori Keesey
Heliophysicist waits nearly 10 years for Pluto flyby 8 July 2015, by Lori Keesey heliophysicist Nikolaos Paschalidis will be one happy man: he created a mission-enabling technology that will help uncover details about the atmosphere of the never-before-visited dwarf planet. "We have been waiting for this for a long time," said the Greek native, who now works as a scientist at NASA's Goddard Space Flight Center in Greenbelt, Maryland. "That's what happens when it takes more than nine years to get to your destination." When employed by the Maryland-based Johns Hopkins Applied Physics Laboratory (APL), which is operating the New Horizons mission for NASA, Paschalidis designed five application-specific integrated circuits—some now patented—for the mission's Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI), developed by APL Principal Investigator Ralph McNutt. The instrument, one of seven flying on New Horizons, is designed to measure the composition and density of material, such as nitrogen and carbon monoxide, which escapes from Pluto's atmosphere and subsequently is ionized by solar Artist’s concept of the New Horizons spacecraft as it ultraviolet light. The atmospheric chemicals pick up approaches Pluto and its largest moon, Charon, in July energy from the solar wind and stream away from 2015. The craft's miniature cameras, radio science Pluto. experiment, ultraviolet and infrared spectrometers and space plasma experiments will characterize the global Until now, knowledge about the mysterious planet's geology and geomorphology of Pluto and Charon, map atmosphere has come mainly from stellar their surface compositions and temperatures, and occultation, when the planet passes in front of examine Pluto's atmosphere in detail. -
Voyager 1 Encounter with the Saturnian System Author(S): E
Voyager 1 Encounter with the Saturnian System Author(s): E. C. Stone and E. D. Miner Source: Science, New Series, Vol. 212, No. 4491 (Apr. 10, 1981), pp. 159-163 Published by: American Association for the Advancement of Science Stable URL: http://www.jstor.org/stable/1685660 . Accessed: 04/02/2014 18:59 Your use of the JSTOR archive indicates your acceptance of the Terms & Conditions of Use, available at . http://www.jstor.org/page/info/about/policies/terms.jsp . JSTOR is a not-for-profit service that helps scholars, researchers, and students discover, use, and build upon a wide range of content in a trusted digital archive. We use information technology and tools to increase productivity and facilitate new forms of scholarship. For more information about JSTOR, please contact [email protected]. American Association for the Advancement of Science is collaborating with JSTOR to digitize, preserve and extend access to Science. http://www.jstor.org This content downloaded from 131.215.71.79 on Tue, 4 Feb 2014 18:59:21 PM All use subject to JSTOR Terms and Conditions was complicated by several factors. Sat- urn's greater distance necessitated a fac- tor of 3 reduction in the rate of data transmission (44,800 bits per second at Saturn compared to 115,200 bits per sec- Reports ond at Jupiter). Furthermore, Saturn's satellites and rings provided twice as many objects to be studied at Saturn as at Jupiter, and the close approaches to Voyager 1 Encounter with the Saturnian System these objects all occurred within a 24- hour period, compared to nearly 72 Abstract. -
In Situ Exploration of the Giant Planets Olivier Mousis, David H
In situ Exploration of the Giant Planets Olivier Mousis, David H. Atkinson, Richard Ambrosi, Sushil Atreya, Don Banfield, Stas Barabash, Michel Blanc, T. Cavalié, Athena Coustenis, Magali Deleuil, et al. To cite this version: Olivier Mousis, David H. Atkinson, Richard Ambrosi, Sushil Atreya, Don Banfield, et al.. In situ Exploration of the Giant Planets. 2019. hal-02282409 HAL Id: hal-02282409 https://hal.archives-ouvertes.fr/hal-02282409 Submitted on 2 Jun 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. In Situ Exploration of the Giant Planets A White Paper Submitted to ESA’s Voyage 2050 Call arXiv:1908.00917v1 [astro-ph.EP] 31 Jul 2019 Olivier Mousis Contact Person: Aix Marseille Université, CNRS, LAM, Marseille, France ([email protected]) July 31, 2019 WHITE PAPER RESPONSE TO ESA CALL FOR VOYAGE 2050 SCIENCE THEME In Situ Exploration of the Giant Planets Abstract Remote sensing observations suffer significant limitations when used to study the bulk atmospheric composition of the giant planets of our solar system. This impacts our knowledge of the formation of these planets and the physics of their atmospheres. A remarkable example of the superiority of in situ probe measurements was illustrated by the exploration of Jupiter, where key measurements such as the determination of the noble gases’ abundances and the precise measurement of the helium mixing ratio were only made available through in situ measurements by the Galileo probe. -
Celebrating 40 Years of Voyager Wonders Mission Veterans Recall the Dedication of the Team; Rock Concert Looks Back Four Decades
SEPTEMBER Jet Propulsion 2017 Laboratory VOLUME 47 NUMBER 9 Celebrating 40 years of Voyager wonders Mission veterans recall the dedication of the team; rock concert looks back four decades By Mark Whalen JPL’s iconic explorers, the twin Voyag- ers, continue on their journey at the edge of the solar system started 40 years ago. JPL celebrated Voyager in late August with a series of events befitting one of the most accomplished and revered robotic space missions of all time. On Friday, Aug. 25, Lab Director Mi- chael Watkins welcomed JPLers, Voyager veterans and political representatives to a commemoration on the Mall. Voyager has been not only a great voy- Josh Krohn / JPL Photo Lab From left: Voyager Project Manager Suzy Dodd, Project Scientist Ed Stone, Communications and Education Director age of exploration, but one of the great- Blaine Baggett, JPL Chief Engineer Chris Jones and John Casani, Voyager’s first project manager. est engineering feats of all time, Watkins noted. “I hope all of us here today feel a told the commitment was for four years. we had ever been,” said Casani. “So it part of the Voyager project,” he said. Hardly, as it turns out. was quite a challenge.” Congresswoman Judy Chu, elected in “There was no way to know whether a But JPLers were up to it. 2009 to represent the 27th district that spacecraft — never mind two — could go The panel chat was interspersed with includes JPL and Caltech, presented a for 40 years,” said Stone, Voyager’s only video clips featuring historic interviews, Congressional certificate of recognition to project scientist since 1972, who still re- launch footage, and Voyager team mem- the Laboratory. -
Revisiting Decades-Old Voyager 2 Data, Scientists Find One More Secret About Uranus 26 March 2020, by Miles Hatfield
Revisiting decades-old Voyager 2 data, scientists find one more secret about Uranus 26 March 2020, by Miles Hatfield Three decades later, scientists reinspecting that data found one more secret. Unbeknownst to the entire space physics community, 34 years ago Voyager 2 flew through a plasmoid, a giant magnetic bubble that may have been whisking Uranus's atmosphere out to space. The finding, reported in Geophysical Research Letters, raises new questions about the planet's one-of-a-kind magnetic environment. A wobbly magnetic oddball Planetary atmospheres all over the solar system are leaking into space. Hydrogen springs from Venus to join the solar wind, the continuous stream of particles escaping the Sun. Jupiter and Saturn eject globs of their electrically-charged air. Even Earth's atmosphere leaks. (Don't worry, it will stick around for another billion years or so.) Voyager 2 took this image as it approached the planet The effects are tiny on human timescales, but given Uranus on Jan. 14, 1986. The planet’s hazy bluish color long enough, atmospheric escape can is due to the methane in its atmosphere, which absorbs fundamentally alter a planet's fate. For a case in red wavelengths of light. Credit: NASA/JPL-Caltech point, look at Mars. "Mars used to be a wet planet with a thick atmosphere," said Gina DiBraccio, space physicist Eight and a half years into its grand tour of the at NASA's Goddard Space Flight Center and solar system, NASA's Voyager 2 spacecraft was project scientist for the Mars Atmosphere and ready for another encounter.