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SSC Tenant Meeting: NASA Near Earth Network (NENJ Overview
https://ntrs.nasa.gov/search.jsp?R=20180001495 2019-08-30T12:23:41+00:00Z SSC Tenant Meeting: NASA Near Earth Network (NENJ Overview --- --- ~ I - . - - Project Manager: David Carter Deputy Project Manager: Dave Larsen Chief Engineer: Philip Baldwin Financial Manager: Cristy Wilson Commercial Service Manager: LaMont Ruley ============== February ==============21, 2018 Agenda > NEN Overview > NEN / SSC Relationship > NEN Missions > Future Trends S1ide2 The Near Earth Network (NEN) consists of globally distributed tracking stations that are strategically located throughout the world which provide Telemetry, Tracking, and Commanding (TT&C) services support to a variety of orbital and suborbital flight missions, including Low Earth Orbit (LEO), Geosynchronous Earth Orbit (GEO), highly elliptical, and lunar orbits Network: The NEN is one of.three networks that together comprise the NASA1s Space Communications and Navigation (SCaN) Networks The NEN provides cost-effective, high data rate services from a global set of NASA, commercial, and partner ground stations to a mission set that requires hourly to daily contacts Missions: The NEN provides communication services to: - Earth Science missions such as Aqua, Aura, OC0-2, QuikSCAT, and SMAP - Space Science missions including AIM, FSGT, IRIS, NuSTAR, and Swift - Lunar orbiting missions such as LRO - CubeSat missions including the upcoming CryoCube, iSAT, and SOCON Stations: The NEN consists of several polar stations which are vital to polar orbiting missions since they enable communications services -
A Decadal Strategy for Solar and Space Physics
Space Weather and the Next Solar and Space Physics Decadal Survey Daniel N. Baker, CU-Boulder NRC Staff: Arthur Charo, Study Director Abigail Sheffer, Associate Program Officer Decadal Survey Purpose & OSTP* Recommended Approach “Decadal Survey benefits: • Community-based documents offering consensus of science opportunities to retain US scientific leadership • Provides well-respected source for priorities & scientific motivations to agencies, OMB, OSTP, & Congress” “Most useful approach: • Frame discussion identifying key science questions – Focus on what to do, not what to build – Discuss science breadth & depth (e.g., impact on understanding fundamentals, related fields & interdisciplinary research) • Explain measurements & capabilities to answer questions • Discuss complementarity of initiatives, relative phasing, domestic & international context” *From “The Role of NRC Decadal Surveys in Prioritizing Federal Funding for Science & Technology,” Jon Morse, Office of Science & Technology Policy (OSTP), NRC Workshop on Decadal Surveys, November 14-16, 2006 2 Context The Sun to the Earth—and Beyond: A Decadal Research Strategy in Solar and Space Physics Summary Report (2002) Compendium of 5 Study Panel Reports (2003) First NRC Decadal Survey in Solar and Space Physics Community-led Integrated plan for the field Prioritized recommendations Sponsors: NASA, NSF, NOAA, DoD (AFOSR and ONR) 3 Decadal Survey Purpose & OSTP* Recommended Approach “Decadal Survey benefits: • Community-based documents offering consensus of science opportunities -
Solar Activity Affecting Space Weather
March 7, 2006, STP11, Rio de Janeiro, Brazil Solar Activity Affecting Space Weather Kazunari Shibata Kwasan and Hida Observatories Kyoto University, Japan contents • Introduction • Flares • Coronal Mass Ejections(CME) • Solar Wind • Future Projects Japanese newspaper reporting the big flare of Oct 28, 2003 and its impact on the Earth big flare (third largest flare in record) on Oct 28, 2003 X17 X-ray Intensity time A big flare on Oct 28, 2003 (third largest X-ray intensity in record) EUV Visible light SOHO/EIT SOHO/LASCO • Flare occurred at UT11:00 on Oct 28 Magnetic Storm on the Earth Around UT 6:00- Aurora observed in Japan on Oct 29, 2003 at around UT 14:00 on Oct 29, 2003 During CAWSES campaign observations (Shinohara) Xray X17 X6.2 Proton 10MeV 100MeV Vsw 44h 30h Bt Bz Dst Flares What is a flare ? Hα chromosphere 10,000 K Discovered in Mid 19C Near sunspots=> energy source is magnetic energy size~(1-10)x 104 km Total energy 1029 -1032erg (~ 105ー108 hydrogen bombs ) (Hida Observatory) Prominence eruption (biggest: June 4, 1946) Electro- magnetic Radio waves emitted from a flare (Svestka Visible 1976) UV 1hour time Solar corona observed in soft X-rays (Yohkoh) Soft X-ray telescope (1keV) Coronal plasma 2MK-10MK X-ray view of a flare Magnetic reconneciton Hα X-ray MHD simulation of a solar flare based on reconnection model including heat conduction and chromospheric evaporation (Yokoyama-Shibata 1998, 2001) A solar flare Observed with Yohkoh soft X-ray telescope (Tsuneta) Relation between filament (prominence) eruption and flare A flare -
Should We Manage to a Single Data Point? a NASA/Goddard Space Flight Center Perspective
Goddard Space Flight Center Flight Projects Directorate Performance Management Should We Manage to a Single Data Point? A NASA/Goddard Space Flight Center Perspective Dr. Wanda Peters Deputy Director for Planning and Business Management 2019 Project Management Symposium Turning Knowledge into Practice University of Maryland May 10, 2019 Goddard Overview Project Management at Goddard Business Change Initiative Optimization State of Business Why is this Important? 2 Best Place to Work in the Federal Government 2018 3 Goddard Overview 4 Goddard Space Flight Center ONE World-Class Science and Engineering Organization SIX Distinctive Facilities & Installations Independent Greenbelt Wallops Flight White Sands Test Columbia Goddard Institute Validation & Main Campus Facility Facility Ground Balloon for Space Studies Verification 1,270 Acres 6,188 Acres Stations Facility Facility Executing NASA’s most Launching Payloads for Understanding our Providing Software Communicating with Directing High Altitude complex science missions NASA & the Nation Planet Assurance Assets in Earth’s Orbit Investigations Est. 1959 Est. 1945 Est. 1961 Est. 1993 Est. 1963 Est. 1982 MARYLAND VIRGINIA NEW YORK WEST VIRGINIA NEW MEXICO TEXAS 2 Who We Are THE GODDARD COMMUNITY Technicians and Others 6% Clerical 5% Professional & Administrative 28% Scientists & Engineers GSFC CS Employees 61% with Degrees Bachelors – 37% Advanced Degrees – 48% Associate/Technical – 2% Number of Employees High School – 13% A diverse community of scientists, engineers, ~3,000 Civil Service technologists, and administrative personnel ~6,000 Contractor dedicated to the exploration of space ~1,000 Other* Total - ~10,000 *Including off-site contractors, interns, and Emeritus The Nation’s largest community of scientists, engineers, and technologists Goddard Space Flight Center Employees Receive Worldwide Accolades for Their Work Dr. -
Optical and Radio Solar Observation for Space Weather
2 Solar and Solar wind 2-1 Optical and Radio Solar Observation for Space Weather AKIOKA Maki, KONDO Tetsuro, SAGAWA Eiichi, KUBO Yuuki, and IWAI Hironori Researches on solar observation technique and data utilization are important issues of space weather forecasting program. Hiraiso Solar Observatory is a facility for R & D for solar observation and routine solar observation for CRL's space environment information service. High definition H alpha solar telescope is an optical telescope with very narrow pass-band filter for high resolution full-disk imaging and doppler mapping of upper atmos- phere dynamics. Hiraiso RAdio-Spectrograph (HiRAS) provides information on coronal shock wave and particle acceleration in the soar atmosphere. These information are impor- tant for daily space weather forecasting and alert. In this article, high definition H alpha solar telescope and radio spectrograph system are briefly introduced. Keywords Space weather forecast, Solar observation, Solar activity 1 Introduction X-ray and ultraviolet radiation resulting from solar activities and solar flares cause distur- 1.1 The Sun as the Origin of Space bances in the ionosphere and the upper atmos- Environment Disturbances phere, which in turn cause communication dis- The space environment disturbance phe- ruptions and affect the density structure of the nomena studied in space weather forecasting Earth's atmosphere. CME induce geomagnet- at CRL include a wide range of phenomena ic storms and ionospheric disturbances upon such as solar energetic particle (SEP) events, reaching the Earth's magnetosphere, and are geomagnetic storms, ionospheric disturbances, believed to be responsible for particle acceler- and radiation belt activity. All of these space environment disturbance events are believed to have solar origins. -
LCS Onepager
National Aeronautics and Space Administration NASA’s Launch communications segment: Advanced Communications Capabilities for the Florida Spaceport NASA Goddard Space Flight Center’s Near Earth Network Launch Communications Segment (LCS) consists of two modern ground stations designed to complement the U.S. Air Force’s Eastern Range, enabling next-generation space missions and launch vehicles departing from, or returning to, the Florida spaceport. The LCS stations provide the critical link between astronauts and mission controllers on crewed flights, and augment FEATURED launch vehicle telemetry and orbital tracking communications CAPABILITIES for robotic missions. LCS provides a broad array of communications services: • Pre-launch, launch, ascent and landing communications services • Agile, tailored and robust solutions for a variety of customer needs • Simultaneous transmitting and receiving via S-band • Support of IRIG and CCSDS space link standards, advanced modulation and encoding, and 2 Mbps data rates • Remote monitor and control for routine events and pre-mission testing • Common Space Link Extension (SLE) user gatewayIP baseband data interfaces • Orbital communications services to near-Earth users • Standard service scheduling through the Near Earth Network Scheduling Office • Antenna auto-tracking with automatic fail-over to Launch Trajectory Acquisition System (LTAS) or predicted vectors • Doppler and ranging capabilities Strategic Locations LCS consists of two strategically placed permanent ground stations: the Kennedy Uplink Station on site at NASA’s Kennedy Space Center (KSC) and the Ponce de Leon Station 40 miles north in New Smyrna Beach, Florida. Each of these sites has a 6.1-meter antenna capable of simultaneously transmitting and receiving S-band signals. The two-site architecture ensures continuous signal coverage during launch, as well as for vehicles returning to the launch site or the Shuttle Landing Facility. -
Scan-MOCS-0001
SCaN-MOCS-0001 SPACE COMMUNICATIONS AND NAVIGATION PROGRAM Space Communications and Navigation (SCaN) Mission Operations and Communications Services (MOCS) Revision 2 Effective Date: March 15, 2019 Expiration Date: March 15, 2024 National Aeronautics and NASA Headquarters Space Administration Washington, D. C. CHECK THE SCaN NEXT GENERATION INTEGRATED NETWORK (NGIN) AT: https://scanngin.gsfc.nasa.gov TO VERIFY THAT THIS IS THE CORRECT VERSION PRIOR TO USE. Space Communications and Navigation (SCaN) Mission Operations and Communications Services (MOCS) Effective Date: March 15, 2019 Approved and Prepared by: John J. Hudiburg 3/15/19 J ohn J. Hudiburg Date Mission Integration and Commitment Manager, SCaN Network Services Division Human Exploration and Operations Mission Directorate NASA Headquarters Washington, D. C. SCaN-MOCS-0001 Revision 2 Preface This document is under configuration management of the SCaN Integrated Network Configuration Control Board (SINCCB). This document will be changed by Documentation Change Notice (DCN) or complete revision. Proposed changes to this document must be submitted to the SCaN Configuration Management Office along with supportive material justifying the proposed change. Comments or questions concerning this document and proposed changes shall be addressed to: Configuration Management Office [email protected] Space Communications and Navigation Office NASA Headquarters Washington, D. C. ii SCaN-MOCS-0001 Revision 2 Change Information Page List of Effective Pages Page Number Issue Title Rev 2 iii -
Coordinate Systems for Solar Image Data
A&A 449, 791–803 (2006) Astronomy DOI: 10.1051/0004-6361:20054262 & c ESO 2006 Astrophysics Coordinate systems for solar image data W. T. Thompson L-3 Communications GSI, NASA Goddard Space Flight Center, Code 612.1, Greenbelt, MD 20771, USA e-mail: [email protected] Received 27 September 2005 / Accepted 11 December 2005 ABSTRACT A set of formal systems for describing the coordinates of solar image data is proposed. These systems build on current practice in applying coordinates to solar image data. Both heliographic and heliocentric coordinates are discussed. A distinction is also drawn between heliocentric and helioprojective coordinates, where the latter takes the observer’s exact geometry into account. The extension of these coordinate systems to observations made from non-terrestial viewpoints is discussed, such as from the upcoming STEREO mission. A formal system for incorporation of these coordinates into FITS files, based on the FITS World Coordinate System, is described, together with examples. Key words. standards – Sun: general – techniques: image processing – astronomical data bases: miscellaneous – methods: data analysis 1. Introduction longitude and latitude – only need to worry about two spatial dimensions. The same can be said for normal cartography of Solar research is becoming increasingly more sophisticated. a planet such as Earth. However, to properly treat the complete Advances in solar instrumentation have led to increases in spa- range of solar phenomena, from the interior out into the corona, tial resolution, and will continue to do so. Future space mis- a complete three-dimensional coordinate system is required. sions will view the Sun from different perspectives than the Unfortunately, not all the information necessary to determine current view from ground-based observatories, or satellites in the full three-dimensional position of a solar feature is usually Earth orbit. -
The Decade of Light: Innovations in Space Communications and Navigation Technologies
Journal of Space Operations & Communicator (ISSN 2410-0005) Vol. 16, No. 1, Year 2019 The Decade of Light: Innovations in Space Communications and Navigation Technologies Philip Liebrecht Donald Cornwell David Israel Gregory Heckler NASA Headquarters NASA Headquarters Goddard Space Flight Center NASA Headquarters 300 E Street SW 300 E Street SW 8800 Greenbelt Road 300 E Street SW Washington, D.C Washington, D.C. Greenbelt, Md. 20771 Washington, D.C. 202-358-1701 202-358-0570 301-286-5294 202-358-1626 [email protected] [email protected] [email protected] [email protected] INTRODUCTION NASA’s Space Communications and Navigation (SCaN) program office’s vision of a fully interoperable network of space communications assets is known as the Decade of Light. Through relentless advancement of current technologies, NASA is progressing toward a future of seamless mission enabling space communications and navigation. This futuristic, interoperable system will include the development of optical communications, wideband Ka-band, hybrid optical and radio frequency (RF) antennas, user- initiated services (UIS), a cognitive network with disruption-tolerant networking (DTN) capabilities and autonomous navigation. This vision, although vastly complex, will introduce dramatic increases in performance and is already being worked at NASA Headquarters, NASA’s Goddard Space Flight Center, NASA’s Glenn Research Center, and Jet Propulsion Laboratory. Teams from around the country continue to investigate and strive for innovative solutions to the many complex challenges space communications and navigation faces. CURRENT CAPABILITIES For the past 50 years, NASA has primarily used RF to communicate mission data from satellites orbiting in our solar system to data users on Earth. -
Communications Enabling Science from the 2050 Heliophysics System Observatory 1 2 3 4 2 Authors: S
Heliophysics 2050 White Papers (2021) 4119.pdf Communications Enabling Science from the 2050 Heliophysics System Observatory 1 2 3 4 2 Authors: S. J. Schonfeld , W. D. Pesnell , J. L. Verniero , Y. J. Rivera , A. J. Halford , S. K. 5 4 Vines , S. A. Spitzer 2 6 7 Cosigners: A. K. Higginson , B. L. Alterman , M. J. Weberg 1 2 3 I nstitute for Scientific Research, Boston College, N ASA Goddard Space Flight Center, U niversity of 4 5 California, Berkeley, U niversity of Michigan, J ohns Hopkins University Applied Physics Laboratory, 6 7 S outhwest Research Institute, N RC postdoc at U.S. NRL The difficulties associated with receiving telemetry from satellites severely limits the volume of scientific data that can be downlinked to scientists on the ground. Current missions must employ many techniques to reduce the data they transmit, such as compressing and pruning datasets, to meet the current restrictions of limited telemetry budgets. Yet future Heliophysics System Observatory missions will produce ever larger data volumes with higher resolution and cadence observations from constellations of satellites spread throughout the heliosphere1. In addition, heliophysics missions often produce data for the Space Weather community that requires a low latency between observation and downlink. In light of current limitations, the infrastructure to receive NASA satellite telemetry must be expanded and modernized to support future science needs and the data-rich missions of the 2050 Heliophysics System Observatory. The current communications landscape: Communications with NASA science missions are primarily routed through the Deep Space Network (DSN), Near Earth Network (NEN), and Space Network (SN) using S, X, and Ka band radio transmissions. -
CESRA Workshop 2019: the Sun and the Inner Heliosphere Programme
CESRA Workshop 2019: The Sun and the Inner Heliosphere July 8-12, 2019, Albert Einstein Science Park, Telegrafenberg Potsdam, Germany Programme and abstracts Last update: 2019 Jul 04 CESRA, the Community of European Solar Radio Astronomers, organizes triennial workshops on investigations of the solar atmosphere using radio and other observations. Although special emphasis is given to radio diagnostics, the workshop topics are of interest to a large community of solar physicists. The format of the workshop will combine plenary sessions and working group sessions, with invited review talks, oral contributions, and posters. The CESRA 2019 workshop will place an emphasis on linking the Sun with the heliosphere, motivated by the launch of Parker Solar Probe in 2018 and the upcoming launch of Solar Orbiter in 2020. It will provide the community with a forum for discussing the first relevant science results and future science opportunities, as well as on opportunity for evaluating how to maximize science return by combining space-borne observations with the wealth of data provided by new and future ground-based radio instruments, such as ALMA, E-OVSA, EVLA, LOFAR, MUSER, MWA, and SKA, and by the large number of well-established radio observatories. Scientific Organising Committee: Eduard Kontar, Miroslav Barta, Richard Fallows, Jasmina Magdalenic, Alexander Nindos, Alexander Warmuth Local Organising Committee: Gottfried Mann, Alexander Warmuth, Doris Lehmann, Jürgen Rendtel, Christian Vocks Acknowledgements The CESRA workshop has received generous support from the Leibniz Institute for Astrophysics Potsdam (AIP), which provides the conference venue at Telegrafenberg. Financial support for travel and organisation has been provided by the Deutsche Forschungsgemeinschaft (DFG) (GZ: MA 1376/22-1). -
IWPSS 2013 Multi-Mission Scheduling Operations at UC Berkeley Bester
Proceedings of the 2013 International Workshop on Planning & Scheduling for Space, Mountain View, CA, USA, March 25-26, 2013, Paper AIAA-2013-XXXX. THIS SPACE MUST BE KEPT BLANK] Multi-Mission Scheduling Operations at UC Berkeley Manfred Bester, Gregory Picard, Bryce Roberts, Mark Lewis, and Sabine Frey Space Sciences Laboratory, University of California, Berkeley [email protected], [email protected], [email protected], [email protected], [email protected] Abstract completed in 2011 when both probes were inserted into The University of California, Berkeley conducts mission stable lunar orbits (Cosgrove et al. 2012, Bester et al. operations for eight spacecraft at present. Communications 2013). with the orbiting spacecraft are established via a multitude of network resources, including all NASA networks, plus • The Nuclear Spectroscopic Telescope Array (NuSTAR) – assets provided by foreign space agencies and commercial a NASA SMEX mission launched in June 2012 – is a companies. Mission planning is based on the science re- high-energy X-ray observatory carrying twin telescopes quirements as well as accessibility to communications net- with focusing optics (Kim et al. 2013). work resources. The integrated scheduling process is com- plex and is supported by partly automated software tools. • The CubeSat for Ion, Neutral, Electron, and MAgnetic Challenges encountered and lessons learned are described. fields (CINEMA) – the first CubeSat built in-house at SSL – launched in September 2012. The project home page can be found at http://sprg.ssl.berkeley.edu/cinema. Introduction A summary of these missions and their characteristics is The University of California, Berkeley (UCB) currently provided in Table A1 in the Appendix.