GEOSPACE? Observational Gaps Could Make It Tougher to Understand High-Altitude Climate Change and Avoid Catastrophes in Low-Earth Orbit
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Suborbital Platforms and Range Services (SPARS)
Suborbital Capabilities for Science & Technology Small Missions Workshop @ Johns Hopkins University June 10, 2019 Mike Hitch, Giovanni Rosanova Goddard Space Introduction Flight Center AGENDAWASP OPIS ▪ Purpose ▪ History & Importance of Suborbital Carriers to Science ▪ Suborbital Platforms ▪ Sounding Rockets ▪ Balloons (brief) ▪ Aircraft ▪ SmallSats ▪ WFF Engineering ▪ Q & A P-3 Maintenance 12-Jun-19 Competition Sensitive – Do Not Distribute 2 Goddard Space Purpose of the Meeting Flight Center Define theWASP OPISutility of Suborbital Carriers & “Small” Missions ▪ Sounding rockets, balloons and aircraft (manned and unmanned) provide a unique capability to scientists and engineers to: ▪ Allow PIs to enhance and advance technology readiness levels of instruments and components for very low relative cost ▪ Provide PIs actual science flight opportunities as a “piggy-back” on a planned mission flight at low relative cost ▪ Increase experience for young and mid-career scientists and engineers by allowing them to get their “feet wet” on a suborbital mission prior to tackling the much larger and more complex orbital endeavors ▪ The Suborbital/Smallsat Platforms And Range Services (SPARS) Line Of Business (LOB) can facilitate prospective PIs with taking advantage of potential suborbital flight opportunities P-3 Maintenance 12-Jun-19 Competition Sensitive – Do Not Distribute 3 Goddard Space Value of Suborbital Research – What’s Different? Flight Center WASP OPIS Different Risk/Mission Assurance Strategy • Payloads are recovered and refurbished. • Re-flights are inexpensive (<$1M for a balloon or sounding rocket vs >$10M - 100M for a ELV) • Instrumentation can be simple and have a large science impact! • Frequent flight opportunities (e.g. “piggyback”) • Development of precursor instrument concepts and mature TRLs • While Suborbital missions fully comply with all Agency Safety policies, the program is designed to take Higher Programmatic Risk – Lower cost – Faster migration of new technology – Smaller more focused efforts, enable Tiger Team/incubator experiences. -
Measurements of Auroral Particles by Means of Sounding Rockets of Mother-Daughter Type A
MEASUREMENTS OF AURORAL PARTICLES BY MEANS OF SOUNDING ROCKETS OF MOTHER-DAUGHTER TYPE A. Falck KGI REPORT 192 NOVEMBER 1985 KIRUNA U-OI'HYSICAL INSTITITK MKINA N\X|1>I\ MEASUREMENTS OF AURORAL PARTICLES BY MEANS OF SOUNDING ROCKETS OF MOTHER-DAUGHTER TYPE by A. Falck Kiruna Geophysical Institute P.O. Box 704, S-981 27 KIRUNA, Sweden KGI Report 192 November 1985 Printed in Sweden Kiruna Geophysical Institute Kiruna 19^5 ISSN 034/-f 405 Contents Page 1. Presentation of the S17 payioads 3 1.1 The scientific objective of the sounding rockets S17 3 1.2 S17 experiments 3 1.3 Physical characteristics of the payioads 3 1.4 Physical characteristics of the Nike-Tomahawk rocket 5 1.5 Nominal characteristics of flight events 7 1.6 Attitude measurements 8 1.7 Separation of the two payload units 20 1.8 Telemetry and data analyzing technique 33 2. Description of the instrumentation for the particle experiments in the S17 payioads 38 2.1 General theory of CEM - detectors 38 2.2 Calibration of th* CEM - detectors 42 2.3 Solid state detectors in SI7 payioads 44 2.4 Mounting of the detectors 48 2.5 The efficiency of channel multipliers 48 3. Review of the geophysical conditions during the SI7 flights and presentation of some supporting observations 51 j.1 The auroral situation during S17 flights 51 :• 2 Magnetic activity 51 .'.3 Other supporting observations 56 .4 The lowlightlevel-TV-system 56 'K Particle fluxes and electric currents coupling the magnetosphere and the ionosphere during a magnetospheric substorm 66 4.1 Review of some substorm terminology and definitions 66 4.2 Reference and comparisons of SI7-2 measure- ments with the results of the IMS-study 75 4.3 Comparison of simultaneous particle observa- tions at low ionospheric altitude (S17-1) and at the magnetic equatorial region (ATS-6) 91 4.4 Summary and conclusions 99 5. -
Colorado Space Grant Consortium
CO_FY16_Year2_APD Colorado Space Grant Consortium Lead Institution: University of Colorado Boulder Director: Chris Koehler Telephone Number: 303.492.3141 Consortium URL: http://spacegrant.colorado.edu Grant Number: NNX15AK04H Lines of Business (LOBs): NASA Internships, Fellowships, and Scholarships; Stem Engagement; Institutional Engagement; Educator Professional Development A. PROGRAM DESCRIPTION The National Space Grant College and Fellowship Program consists of 52 state-based, university- led Space Grant Consortia in each of the 50 states plus the District of Columbia and the Commonwealth of Puerto Rico. Annually, each consortium receives funds to develop and implement student fellowships and scholarships programs; interdisciplinary space-related research infrastructure, education, and public service programs; and cooperative initiatives with industry, research laboratories, and state, local, and other governments. Space Grant operates at the intersection of NASA’s interest as implemented by alignment with the Mission Directorates and the state’s interests. Although it is primarily a higher education program, Space Grant programs encompass the entire length of the education pipeline, including elementary/secondary and informal education. The Colorado Space Grant Consortium is a Designated Consortium funded at a level of $760,000 for fiscal year 2016. B. PROGRAM GOALS • Population of students engaged in COSGC hands-on programs (awardees and non- awardees) will be at least 40% women and 23.7% from ethnic minority populations underrepresented in STEM fields. • Maintain student hands-on programs at all 8 COSGC Minority Serving Institutions and engaged at least 30 students on MSI campuses. • 30% of COSGC NASA funds will be awarded directly to students. • Award 80 scholarships to support students working on hands-on projects. -
In Search of a Martian Faith
Copyright © 2018 by Hannah Earnshaw. Published by The Mars Society with permission IN SEARCH OF A MARTIAN FAITH Dr Hannah P. Earnshaw Email: [email protected] Abstract When humans go to Mars, they will take religion with them. But what will that look like, and what challenges to religious practice will those future migrants face? In this paper, I describe a little of my personal experience as a scientist and Mars One candidate of faith, and use the religious makeup of the Mars 100 as an example case to explore the implications of practicing religion in space and on Mars, with reference to three main problems: community, time, and space. I explore the importance of community to religious people in space and the difficulty faced by a single member of a faith cut off from the rest of their religious community, and argue that this will require compassionate and respectful interfaith support among Mars migrant crews. Using examples from various religions, I discuss the challenges of timekeeping away from Earth and how it affects time-dependent religious observance, and some of the current proposed solutions for astronauts in orbit as well as how Mars migrants may adapt religious ritual to Martian time. I examine the phenomenon of sacred physical locations and spaces, and how Mars migrants will cope with living apart from the planet where every significant religious event to date has happened. Finally, I offer some speculation on what may develop as the sacred and mythic on Mars, as humans bring their sense of awe, wonder and spirit to a new planet. -
Geochemistry, Geophysics, Geosystems Becoming an Open Access Journal: FAQ
Geochemistry, Geophysics, Geosystems becoming an open access journal: FAQ Why is Geochemistry, Geophysics, Geosystems becoming an open access journal? AGU remains committed to open science and open data. As a part of our mission, we are focused on making science available to the widest possible audience. Since many researchers around the world have open access requirements by funders, this move to an open access model will make compliance easier. Authors will pay an open access article processing charge (APC) and retain copyright of their article which they can publish under a Creative Commons license (choose from CC-BY or CC-BY-NC-ND). There will be no excess page fees or any other additional fees for publication. In addition, there will be no subscription paywall, which means that more people will have access to your research so they can actively cite, read and share data for free. When will Geochemistry, Geophysics, Geosystems become open access? All articles in the journal will be open access as of 1 January 2022. After 8 September 2021, submissions received/accepted must agree to pay the open access article processing charge (APC), but there will be no excess page fees or any other additional fees for publication. What if I already have a paper under consideration to Geochemistry, Geophysics, Geosystems? If your paper: • is under consideration before 8 September 2021 and • publishes after 1 January 2021, then your paper will publish with copyright to the authors under a Creative Commons license for free (the fee will be waived). If your paper publishes in 2021, then the paper will publish as a subscription article (copyright AGU). -
Latex Submission Guidelines
Latex submission guidelines The current version of the zip archive containing all components is marked April 30, 2019 The current version of the main CLS file is April 16, 2019 You are not required to use the newest template, but it is strongly recommended. Zip Contents: April‐30‐2019‐latex‐templates.zip contains these files: agujournaltemplate.tex o This is a “sample” manuscript. It contains commented out instructions and pre‐defined sections to add your work. agujournal2019.cls o This is the primary class file. It corresponds to agujournaltemplate.tex si_template_2019.tex o A “sample” supporting information readme. Like agujournaltemplate.tex, it contains a framework to fill with information about your supplemental files. agutexSI2019.cls o The class file for the supporting information readme file, si_template_2019.tex trackchanges.sty o a third‐party package that facilitates manuscript annotation, usually for tracking changes. Set package options to “inline” to show annotations, “finalnew” to compile an unmarked paper. Complete documentation is here. a directory, trackchanges‐0.7.0 o contains python scripts for automated removal of change tracking commands, if needed o also includes documentation and authorship info for the package above 1 Using agujournaltemplate.tex 1. enter the journal’s name in plain text \journalname{here} 2. enter your paper’s title \title{here} 3. List all authors \authors{here} List authors by first name or initial followed by last name and separated by commas. Use \affil{} to number affiliations, and \thanks{} for author notes. Additional author notes should be indicated with \thanks{} (current addresses, for example). Example: \authors{A. B. -
AGU Electronics Editions Package, AGU
SCHEDULE 3 Addition(s), Deletion(s) to Agreement, Licensed Materials, Subscription Period and Access Method A schedule dated 11'/11./UlfJ to the License dated 1/;-t./u;ot{ between American Geophysical Union and The California Digital Library. ADDITION(s) DELETION(s) TO THE LICENSED MATERIALS AND SUBSCRIPTION PERIOD AND ACCESS METHOD: Addition(s), Deletion(s) made by the Licensee must be approved by Publisher, agreed to, and signed by both parties. Titles(s) Period • • •• Fee AGU Electronics Editions Package* Jan 1 - Dec 31, 2011 AGU Digital Library Jan 1 - Dec 31, 2011 Purchase starting Jan 1, 2011 *Includes the journals titled: Journal of Geophysical Research - All sections Journal of Geophysical Research - Space Physics Section Journal of Geophysical Research - Solid Earth Section Journal of Geophysical Research - Oceans Section Journal of Geophysical Research - Atmospheres Section Journal of Geophysical Research - Planets Section Journal of Geophysical Research - Earth Surface Section Journal of Geophysical Research - Biogeosciences Section Water Resources Research Reviews of Geophysics Geophysical Research Letters Radio Science Tectonics Paleoceanography Global Biogeochemical Cycles Geochemistry Geophysics Geosystems Space Weather Earth Interactions (copublished with AMS and AAG) Chinese Journal of Geophysics (distributed by AGU) Nonlinear Processes in Geophysics (copublished with EGU) **Each year thereafter, a ccess fee would be charged to the Licensee. SUBSCRIBING LOCATION IP ADDRESSES UC Berkeley [Including Lawrence Berkeley Lab] -
Methods of Oabservation at Sea Meteorological Soundings in The
WORLD METEOROLOGICAL ORGANIZATION WORLD METEOROLOGICAL ORGANIZATION TECHNICAL NOTE No. 2 TECHNICAL NOTE No. 60 METHODS OF OABSERVATION AT SEA METEOROLOGICAL SOUNDINGS IN THE PARTUPPER I – SEA SURFACEATMOSPHERE TEMPERATURE by W.W. KELLOGG WMO-No.WMO-No. 153. 26. TP. 738 Secretariat of the World Meteorological Organization – Geneva – Switzerland THE WMO The WOTld :Meteol'ological Organization (Wl\IO) is a specialized agency of the United Nations of which 125 States and Territories arc Members. It was created: to facilitate international co~operation in the establishment of networks of stations and centres to provide meteorological services and observationsI to promote the establishment and maintenance of systems for the rapid exchange of meteorological information, to promote standardization of meteorological observations and ensure the uniform publication of observations and statistics. to further the application of rneteol'ology to Rviatioll, shipping, agricultul"C1 and other human activities. to encourage research and training in meteorology. The machinery of the Organization consists of: The World Nleteorological Congress, the supreme body of the o.rganization, brings together the delegates of all Members once every four years to determine general policies for the fulfilment of the purposes of the Organization, to adopt Technical Regulations relating to international meteorological practice and to determine the WMO programme, The Executive Committee is composed of 21 dil'cetors of national meteorological services and meets at least once a yeae to conduct the activities of the Organization and to implement the decisions taken by its Members in Congress, to study and make recommendations Oll matters affecting international meteorology and the opel'ation of meteorological services. -
Importance Oi Thermistor Mount Configuration to Meteorological
James F. Morrissey importance oi and Andrew S. Carten, Jr. thermistor mount configuration A. F. Cambridge Research Laboratories to meteorological rocket Bedford, Mass. temperature measurements Abstract tions. Thus, we are receiving more data than ever be- A description is given of the original rocketsonde ther- fore—thanks to more successful firings and improved mistor mount, consisting of a 10-mil bead suspended signal reception—but data quality has stayed at a low between two metal posts. The difficulties encountered to medium level. Recent evidence, described later in this with this mount and the subsequent development of article, confirms our belief that caution is in order. the superior "thin-film" mount are also described. The Today's rocketsonde is, for the most part, a more uncertainties associated with the use of the latter mount rugged version of the standard radiosonde. This is only are outlined along with their effect on data acceptance. natural, considering both the effort which has gone into A different approach to the original problem is de- refining radiosonde and associated ground equipment scribed, which employs longer leads for dissipation of design and the success which has crowned that effort. heat conducted to the bead. The uncertainty associated In choosing a sensor for the rocketsonde, it was recog- with the long lead is shown to be minimal. Preliminary nized that the small bead thermistor has the necessary results of a series of 10 rocket flights are presented. response time to provide useful measurements to about These results tend to confirm the advantages of the 60 km. A 10-mil diameter bead, aluminized to minimize long lead mount. -
NASA Sounding Rockets Annual Report 2020
National Aeronautics andSpaceAdministration National Aeronautics NASA Sounding Rockets Annual Report 2020 science payload launched on a Terrier-Improved Malemute provided by NASA, experienced a vehicle failure and science data was not recorded. The Cusp Heating Investigation (CHI) for Dr. Larsen, Clemson University, measured neutral upwelling and high-resolution electric fields over an extended region in the cusp, and was a resound- ing success. Additionally, the Cusp-Region Experiment (C-REX) 2 for Dr. Conde, University of Alaska, was staged and ready to go at Andoya Space Center, Norway, however, science conditions did not materialize, and after 17 launch attempts the window of opportunity closed. C-REX 2 is currently on schedule for launch in December 2020. The final geospace science launch for fiscal year 2020 took place from Poker Flat Research Range, Alaska. Polar Night Nitric Oxide Message from the Chief Message Giovanni Rosanova, Jr. (PolarNOx), for Dr. Bailey, Virginia Tech, was successfully launched Chief, Sounding Rockets Program Office in January 2020. Data from PolarNOx will aid in the understanding of the abundance of NO in the polar atmosphere, and its impact on I will start this year’s message with expressing my gratitude to the peo- ozone. ple supporting the sounding rockets program. Through the challeng- ing time of the CoVid-19 pandemic, the outstanding efforts by the Technology development is a core aspects of the program. This year entire team have enabled us to continue meeting several milestones. we launched the eighth dedicated technology development flight, Our mission meetings have been held using virtual tools. Enhanced SubTEC-8. -
1999 EOS Reference Handbook
1999 EOS Reference Handbook A Guide to NASA’s Earth Science Enterprise and the Earth Observing System http://eos.nasa.gov/ 1999 EOS Reference Handbook A Guide to NASA’s Earth Science Enterprise and the Earth Observing System Editors Michael D. King Reynold Greenstone Acknowledgements Special thanks are extended to the EOS Prin- Design and Production cipal Investigators and Team Leaders for providing detailed information about their Sterling Spangler respective instruments, and to the Principal Investigators of the various Interdisciplinary Science Investigations for descriptions of their studies. In addition, members of the EOS Project at the Goddard Space Flight Center are recognized for their assistance in verifying and enhancing the technical con- tent of the document. Finally, appreciation is extended to the international partners for For Additional Copies: providing up-to-date specifications of the instruments and platforms that are key ele- EOS Project Science Office ments of the International Earth Observing Mission. Code 900 NASA/Goddard Space Flight Center Support for production of this document, Greenbelt, MD 20771 provided by Winnie Humberson, William Bandeen, Carl Gray, Hannelore Parrish and Phone: (301) 441-4259 Charlotte Griner, is gratefully acknowl- Internet: [email protected] edged. Table of Contents Preface 5 Earth Science Enterprise 7 The Earth Observing System 15 EOS Data and Information System (EOSDIS) 27 Data and Information Policy 37 Pathfinder Data Sets 45 Earth Science Information Partners and the Working Prototype-Federation 47 EOS Data Quality: Calibration and Validation 51 Education Programs 53 International Cooperation 57 Interagency Coordination 65 Mission Elements 71 EOS Instruments 89 EOS Interdisciplinary Science Investigations 157 Points-of-Contact 340 Acronyms and Abbreviations 354 Appendix 361 List of Figures 1. -
Radio Science Bulletin Staff
INTERNATIONAL UNION UNION OF RADIO-SCIENTIFIQUE RADIO SCIENCE INTERNATIONALE ISSN 1024-4530 Bulletin Vol. 2020, No. 372 March 2020 Radio Science URSI, c/o Ghent University (INTEC) Technologiepark - Zwijnaarde 126, B-9052 Gent (Belgium) Contents Radio Science Bulletin Staff ....................................................................................... 3 URSI Offi cers and Secretariat.................................................................................... 6 Editor’s Comments ..................................................................................................... 8 Introduction to the URSI-JRSM 2019 SPC Special Issue ..................................... 10 ASIC Waveform Receiver with Improved Environmental Tolerance for Probing Space Plasma Waves in Environments with High Radiation and Wide Temperature Variation ............................................................................... 12 Performance Improvement of Resonator-Coupled Wireless Power Transfer System Using Dual-Spiral Resonator with Angular Misalignments ................ 22 ULF Modulation of Energetic Electron Precipitation Observed by VLF/LF Radio Propagation ................................................................................................ 29 Et Cetera .................................................................................................................... 41 Book Review .............................................................................................................. 42 Solution Box ..............................................................................................................