[SPA] SPA SECTION NEWSLETTER, Volume XXX, Issue 2
Newsletter Editor
editor at igpp.ucla.edu
Thu Jan 12 00:18:23 PST 2023
AMERICAN GEOPHYSICAL UNION
SPA SECTION NEWSLETTER
Volume XXX, Issue 2
Jan.12,2023
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Table of Contents
1. Please Support a Final Extension of the Cluster Mission!
2. CALL FOR PAPERS: Special Issue in Frontiers "Particle Precipitation in the Earth and Other Planetary Systems: Souces and Impacts"
3. MEETING: Symposium on the Future of Heliospheric Science: From Geotail and Beyond -- 2nd Circular
4. MEETING: Spacecraft Anomalies and Failures (SCAF) Workshop 2023
5. MEETING: COSPAR Capacity-Building Workshop – IRI 2023 – KASI, South Korea, May 8-19, 2023
6. SESSION: 2023 URSI-GASS Space Weather Session "Ionospheric Space Weather and Impacts on Technological Systems"
7. SESSION: 2023 URSI-GASS HGE Session "Atmospheric, Ionospheric, Magnetospheric and High Energy Effects of Lightning Discharges"
8. First 2023 ISWI WEBINAR SERIES Announcement
9. New Real-time Dst Forecasting Model
10. JOB OPENING: Space Physics Group, Princeton University Department of Astrophysical Sciences
11. JOB OPENING: Postdoctoral Fellow Position in Inner Heliospheric Physics at the Johns Hopkins University (JHU) Applied Physics Laboratory (APL) in Laurel, Maryland, USA
12. JOB OPENING: Post-doctoral Scholarship (2 Years) in Modelling Plasma Interaction with Planetary Bodies
13. JOB OPENING: Post-doctoral Position in Space Weather
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Announcement Submission Website: http://goo.gl/forms/qjcm4dDr4g
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Please Support a Final Extension of the Cluster Mission!
From: Andrew Fazakerley (a.fazakerley at ucl.ac.uk)
We are writing as the Cluster Principal Investigators to inform you that a positive decision by ESA to support a final extension of the Cluster mission during 2023-2025 is in doubt. We would like to ask for your help in our efforts to persuade ESA to support a final extension.
Apologies, if you have seen this message more than once. If you have already responded, thank you!.
If you would like to show your support, please simply visit the following link, and add your name/institute/nation at the very end of the google document that you find there, at your earliest convenience.
https://docs.google.com/document/d/13sEBJh4A_TkiRO6i_LUJ6F_nfJkKnFqFFAU5smoM99g/edit
The document that you will find there consists of a letter that the Cluster PIs have drafted to send to ESA's Director of Science and the members of its Science Programme Committee (SPC). We aim to send the completed letter in mid-January, ahead of a key SPC Workshop in early February (which itself precedes the SPC meeting in March at which the extension decision is expected to be formalised).
Please feel free to share this email with colleagues that may be interested; our mailing list is not comprehensive!
Thank you in advance, if you choose to indicate your support.
best wishes
The Cluster Principal Investigators
Mats Andre, Michael Balikhin, Patrick Canu, Chris Carr, Patrick Daly,
Iannis Dandouras, Andrew Fazakerley, Jolene Pickett, Jean-Louis Rauch,
Roy Torbert, Klaus Torkar, Rob Fear
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CALL FOR PAPERS: Special Issue in Frontiers "Particle Precipitation in the Earth and Other Planetary Systems: Souces and Impacts"
From: Yiqun Yu, Dogacan Ozturk, Yoshizumi Miyoshi, Jim Raines, Hui Wang, Dedong Wang (yiqunyu17 at gmail.com)
Dear Colleagues,
We cordially invite your contributions to a special issue of "Particle Precipitation in the Earth and Other Planetary Systems: Sources and Impacts" in Frontiers in Astronomy & Space Sciences and Frontiers in Physics.
This research topic seeks contributions in revealing sources, characteristics, and responsible processes of particle precipitation, and consequent impacts on planets’ thermosphere and ionosphere, as well as the feedback effects within the integrated system.
We look for original research papers, commentaries, and review papers mainly focusing on:
(1) Physical processes associated with various types of particle precipitation in both the Earth and other planet systems (e.g., Mars, Mercury, Jupiter, Saturn), including plasma waves, pulsating aurora, different types of auroral forms, SEP events, and other potential mechanisms.
(2) The wide range of responses in the planets' thermosphere-ionosphere system to particle precipitation, including variations of neutral/electron density and velocity, temperature variability and irregularity, ion upwelling and outflow, composition variation, energy deposition and dissipation, electromagnetic and ground magnetic fluctuations.
Please goto the webpage for more details:
https://www.frontiersin.org/research-topics/52051/particle-precipitation-in-the-earth-and-other-planetary-systems-sources-and-impacts
Abstract Submission Deadline: 04 March 2023
Manuscript Submission Deadline: 04 July 2023
Best Regards,
Yiqun Yu, Dogacan Ozturk, Yoshizumi Miyoshi, Jim Raines, Hui Wang, Dedong Wang
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MEETING: Symposium on the Future of Heliospheric Science: From Geotail and Beyond -- 2nd Circular
From: Yoshifumi Saito (saito at stp.isas.jaxa.jp)
This is a reminder of an international symposium “Symposium on the Future of Heliospheric Science: From Geotail and Beyond” to be held at Koshiba-Hall, University of Tokyo, between 28 -31 March 2023.
The Geotail satellite, launched in July 1992 from Florida, U. S. A., as a joint project between ISAS (now JAXA) and NASA, has been studying the structure and dynamics of the magnetotail and other key regions of the magnetosphere. It has achieved epoch-making results, including numerous discoveries in magnetospheric physics. After more than three decades in operation, a failure of the onboard data recorder that occurred at the end of June has considerably reduced the amount of data that can be received, while data from some onboard instruments are no longer available. Therefore, we decided to end Geotail’s operation and the operation was terminated in the end of November, 2022.
The purpose of this symposium is to link the tremendous results of Geotail to the future by reviewing the achievements of Geotail to date and looking forward to the exploration of the inner heliosphere system that consists of several sub-systems, Geospace, planetary system, interplanetary space, and the Sun in the late 2020s. The exploration will further expand its area to the whole heliosphere beyond that time frame. The future exploration will also contribute to the space weather research/forecast that supports human activities in Geospace, Moon and other planets.
The symposium will be held in a hybrid format. In addition to invited talks, we plan to call for contributed papers (mainly poster papers). The call for contributed papers is scheduled to open on 16 January. We are also planning to publish the proceedings of the symposium as a special issue of T.B.D. journal.
Place: Koshiba Hall, Hongo Campus, The University of Tokyo
Date: March 28(Tuesday) to 31(Friday) 2023
Registration fee: Free
Symposium Web (abstract submission site is also here): https://sprg.isas.jaxa.jp/Geotail30/
to be open on 16 January 2023
Important Dates:
Registration: 16 January 2023 – 14 March 2023
Abstract submission: 16 January 2023 – 15 February 2023
Release of program: 1 March 2023
Tentative Sessions:
• Geotail Memorial Session
• Geotail to Future Heliospheric System Science1:
Plasma Universe and basic plasma processes
• Geotail to Future Heliospheric System Science2:
Geospace 1/2
• Geotail to Future Heliospheric System Science3:
Heliospheric system science, Planetary magnetosphere, and beyond 1/2/3
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MEETING: Spacecraft Anomalies and Failures (SCAF) Workshop 2023
From: Joseph Minow (joseph.minow at nasa.gov)
The Spacecraft Anomalies and Failures (SCAF) Workshop 2023 will be held 29-30 March 2023 using a hybrid in-person and virtual format. Hosted by NASA and the NRO, the workshop is two days of invited presentations and discussions on improvements in space system anomaly and failure attribution and methodologies to refine and document best practices for anomaly and failure root cause determination. Day 1 (unclassified, public session) will be held at NASA’s Goddard Space Flight Center in Greenbelt, Maryland and Day 2 (classified session) will be held at NRO Headquarters in Chantilly, Virginia. There is no fee to register, but registration is required to attend. Please visit the workshop website for additional workshop information including the agenda and registration links:
https://www.nasa.gov/nase/conferences/SCAF2023
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MEETING: COSPAR Capacity-Building Workshop – IRI 2023 – KASI, South Korea, May 8-19, 2023
From: Dieter Bilitza (dbilitza at gmu.edu)
The 2023 International Reference Ionosphere (IRI) Workshop will take place at the Korea Astronomy and Space Science Institute (KASI) in Daejeon, South Korea from May 8 to 19, 2023. The 2-week workshop is supported under the COSPAR Capacity-Building Workshop program and consists of student-oriented lectures and tutorials during the first week followed by the IRI science meeting in the second week. The first week activities will introduce graduate students and young researchers to the basics of ionospheric monitoring and modeling and related online resources. The students will work on specific modeling problems in small groups and report their results at the end of the second week to the full IRI workshop audience. The second week (15-19 May) will be organized as a regular IRI workshop with oral and poster presentations on the topic of ‘Improved Real-time Ionospheric Predictions with Data from Space-borne Sensors and GNSS’. Presentations on general IRI-related topics are also welcome including new data sources and improvements and new additions for the IRI model. Of special interest are applications of the IRI model in all areas of technology, science and education. Organizing Committee: Young-Sil Kwak (Korea Astronomy and Space Science Institute, KASI), Dieter Bilitza (George Mason University, USA), Yong-Ha Kim (Chungnam National University), Jaejin Lee (KASI), Wookyoung Lee (KASI), Gweonhwa Jee (Korea Polar Research Institute), Suyeon Oh (Cheonnam National University), Kyoung-Wook Min (KASI), and Jeong-Heon Kim (KASI). DEADLINE for submission of ABSTRACTS is March 31, 2023
Students and Young Researchers are encouraged to apply for financial support. Living expenses and partial travel support will be provided for up to 35 competitively selected students and young researchers.
DEADLINE for FINANCIAL SUPPORT APPLICATIONS is February 28, 2023
The workshop website is at http://iri2023.kasi.re.kr/. If you have questions, please contact Young-Sil Kwak <yskwak at kasi.re.kr> or Dieter Bilitza <dbilitza at gmu.edu>.
The IRI homepage is at http://irimodel.org.
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SESSION: 2023 URSI-GASS Space Weather Session "Ionospheric Space Weather and Impacts on Technological Systems"
From: Anthea Coster (ajc at haystack.mit.edu)
Please consider submitting an extended abstract or paper to the our Space Weather session in commission G at the upcoming URSI 2023 General Assembly in Sapporo Japan August 19-26, 2023. This will be an in-person event. Paper/extended abstract submission deadline: January 25, 2023.
https://www.ursi-gass2023.jp/
https://www.ursi-gass2023.jp/paper_submission.html
G03 : Ionospheric Space Weather and Impacts on Technological Systems Conveners:
Iwona Stanislawska, Space Research Centre Polish Academy of Science, Vincenzo Romano, Istituto Nazionale di Geofisica e Vulcanologia, Anthea Coster, MIT Haystack Observatory, Yury Yasyukevich, Institute of solar-terrestrial physics SB RAS.
Session Description:
This session will focus on ionospheric and space weather events that
may impact telecommunications and navigation systems. Studies on the
impact of ionospheric effects on technological systems and services
are welcome. The session will also cover all areas of ionospheric
space weather research including modelling, data assimilation, and
novel observations, specially those using radio wave techniques. Of
special interest are papers describing the assessment and validation
of space weather models, and the justification of the need for new
ground and space-borne measurements. Studies and investigations
addressing the modelling, forecasting and/or mitigation of
ionospheric phenomena due to space weather events, such as large
scale ionospheric gradients or medium- and small-scale
irregularities, are also welcome.
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SESSION: 2023 URSI-GASS HGE Session "Atmospheric, Ionospheric, Magnetospheric and High Energy Effects of Lightning Discharges"
From: Sebastien Celestin, Ningyu Liu, Martin Fullekrug, Ivana Kolmasova (sebastien.celestin at cnrs-orleans.fr)
General Assembly and Scientific Symposium of International Union of Radio Science (URSI-GASS) –- 19-26 August, 2023, Sapporo, Japan
Joint Session Organized by Commissions H, G and E: Atmospheric, Ionospheric, Magnetospheric and High Energy Effects of Lightning Discharges
The recent discovery that lightning discharges can cause energetic radiation, relativistic particles, and transient luminous events has marked a profound progress in our understanding of the Earth's atmospheric electrodynamic behavior. This session explores these novel processes and their impact on the atmosphere and the near-Earth environment. The session solicits contributions that advance knowledge in the areas of the global atmospheric electric circuit, lightning physics, transient luminous events, energetic radiation, relativistic particles, and their impact on the Earth's atmosphere, ionosphere and magnetosphere. One key focus of the session will be novel observations from space platforms and related ground based observations. Interdisciplinary studies that emphasize the connection between atmospheric layers and the relation between atmospheric electricity and climate change are particularly welcome.
The DEADLINE for receipt of abstracts, for application for Young Scientists Award, and for Student Paper Competition is JANUARY 25, 2023.
The abstracts submission website is the following:
https://www.eventure-online.com/eventure/login.form?A1c4fbc04-5ebf-4a04-a174-0447a681f5d9
We particularly encourage students to participate to the URSI-GASS 2023 Student Paper Competition.
Please note that we will ACCEPT USUALLY FORMATTED ABSTRACTS prepared in the template for "extended abstracts". Authors who wish to submit a longer "Summary Paper" with figures and references to the proceedings still have the opportunity to do so but THIS IS NOT COMPULSORY. The authors applying for a Young Scientists Award must submit a full paper. See https://www.ursi-gass2023.jp/paper_submission.html for more information.
The webpage https://www.ursi-gass2023.jp contains general information and abstract submission instructions and guidelines.
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First 2023 ISWI WEBINAR SERIES Announcement
From: María Graciela Molina (gmolina at herrera.unt.edu.ar)
Dear Colleagues,
We are pleased to announce the first 2023 ISWI Seminar by Dr Ivan Galkin scheduled for January 25th at 3 PM Central European Time (9 AM EDT; 6:30 PM IST).
To register for this virtual seminar, please send an email to: iswisupport at bc.edu. Please include “ISWI Seminar Registration” in the subject line. There is a limit of 300 participants, so please register your interest as soon as possible. The MS Teams link will be sent to registered participants 2 days before the event.
Seminars will be recorded. Please visit the youtube channel of the United Nations Office for Outer Space Affairs where the recording of the seminars from 2022 are available. The playlist which will also include future sessions can be accessed through the following link: https://youtube.com/playlist?list=PLaOqa4cng0GF3cKuj6Yz5kqG1BQ-Akkhr
With kind regards,
Graciela Molina
on behalf of the ISWI Seminar Committee
Title: Realistic Ionosphere (RION): data fusion project of GIRO and GNSS
Speaker: Dr Ivan Galkin
Abstract: RION is an ISWI project that involves 69 ionosonde observatories in 32 countries with established agreements to share real-time data for continuous monitoring of the ionosphere. The RION's ionosonde network "GIRO" (Global Ionosphere Radio Observatory) has been in coordinated operation since 2004. Its Lowell GIRO Data Center (LGDC) operates nine online central data repositories and several data sharing and dissemination services. In addition to the public ionosonde data provision, LGDC operates assimilative real-time models of the ionosphere and trans-ionospheric signal propagation that constitute RION. The models include GAMBIT (Global Assimilative Modeling of Bottomside Ionosphere with Topside extension) that interfaces one the International GNSS Service centers in Olsztyn, Poland to build global maps of the effective ionospheric slab thickness. Current state of art and prospective way forward will be presented, including an upcoming Pan-European alert system T-FORS for forecasting TID activity based on Deep Learning techniques.
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New Real-time Dst Forecasting Model
From: Enrico Camporeale (enrico.camporeale at noaa.gov)
We are very excited to present to the Space Weather community a new real-time model for predicting the Dst geomagnetic index, based on multi-fidelity neural networks and uncertainty quantification methods.
LiveDst is currently the only model that makes 1-to-6 hours forecasts of the “quick-look” Dst, with estimated uncertainties, in real-time. It is freely available here:
https://swx-trec.com/dst/
The LiveDst forecast is a research product and is provided to the public on an "as is" basis with no guarantees of completeness, accuracy, usefulness or timeliness.
Please contact me for questions or feedback.
We acknowledge funding from NASA under the “Space Weather with Quantified Uncertainty” program, grant 80NSSC20K1580
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JOB OPENING: Space Physics Group, Princeton University Department of Astrophysical Sciences
From: Dan White (spacephysics at princeton.edu)
The Space Physics Group in the Department of Astrophysical Sciences, Princeton University, anticipates offering one or more postdoctoral or more senior research positions in experimental/observational space physics.
The Space Physics Group conducts research in many aspects of space physics (aka heliophysics), with a strong emphasis on experimental and observational space plasma physics. Among others, the Group currently leads NASA's Interstellar Boundary Explorer (IBEX) mission, the Parker Solar Probe (PSP) Integrated Science Investigation of the Sun (ISIS) instrument suite, and the Interstellar Mapping and Acceleration Probe (IMAP) mission, in development for launch in 2025 to explore the details of particle acceleration and the Sun's interaction with the local interstellar medium. See https://spacephysics.princeton.edu/ for more information about the Space Physics Group at Princeton University.
The successful candidate(s) can play a major role in one or more of the following: 1) analysis and publication of Energetic Neutral Atom (ENA) and other observations from IBEX, 2) analysis and publication of energetic particle observations from ISIS, 3) development of the experimental capability of the Group, and development of space flight instrumentation for IMAP, and 4) other funded space physics research in the Group. Preferred qualifications include having prior experience in the development of space flight instrumentation, analyzing ENA and/or energetic particle data, and the proven ability to lead/participate in the rapid development and publication of numerous excellent research articles. A Ph.D. in Space Physics or a related field is required. Appointments are for one year, renewable annually based on satisfactory performance and continued funding, with the expectation of up to three years. Positions are available regularly so that starting dates may be negotiated.
Interested persons must apply online at https://www.princeton.edu/acad-positions/position/26909 and submit a curriculum vitae, bibliography, a brief statement of research interests, and provide contact information for three references. Letters of recommendation will also be handled through this site. Applications will continue to be accepted until positions are filled. For further inquiries, contact spacephysicsATprinceton.edu.
These positions are subject to the University's background check policy.
Princeton University is an Equal Opportunity/Affirmative Action employer, and all qualified applicants will receive consideration for employment without regard to age, race, color, religion, sex, sexual orientation, gender identity or expression, national origin, disability status, protected veteran status, or any other characteristic protected by law.
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JOB OPENING: Postdoctoral Fellow Position in Inner Heliospheric Physics at the Johns Hopkins University (JHU) Applied Physics Laboratory (APL) in Laurel, Maryland, USA
From: Matthew E. Hill (matt.hill at jhuapl.edu)
The JHU/APL Space & Solar Physics Group (SRP) seeks a Postdoctoral Fellow to conduct basic research with an emphasis on inner-heliospheric physics and the analysis of suprathermal and energetic particle data from the ISOIS/EPI-Lo instrument on Parker Solar Probe (PSP). The successful candidate will work in an exciting environment, with experts in comprehensive data analysis and instrument development for many space missions as well as state-of-the-art modeling of the space environment. The SRP group has a broad and active basic research program that includes data analysis, theory and modeling studies of Earth's magnetosphere and Sun-Earth connections, planetary magnetospheres throughout the solar system, and heliospheric and solar physics. SRP has a significant and long-running history of developing space instrumentation hardware. Current and future active science and instrument participation includes ACE, Geotail, Juno, MMS, New Horizons, PSP, Solar Orbiter, STEREO, Voyager, Europa Clipper, EZIE, JUICE, and IMAP. SRP also leads the multi-institutional Center for Geospace Storms, and partners with Our Heliospheric Shield, two of the three recently selected NASA DRIVE Science Centers.
If successful the candidate will publish original research in peer-reviewed journals and team with SRP and other APL Space Exploration Sector staff to pursue external support for continued research and instrument development. Duties include: conducting original research and analysis of the ISOIS/EPI-Lo particle data; authoring papers for publication in peer-reviewed journals; preparing for and participating in scientific conferences; and developing innovative scientific research and instrument development efforts and proposing to competed solicitations. Required qualifications include: a PhD in Physics or related technical field or equivalent experience; in-depth knowledge of space plasma physics; experience in analysis and scientific interpretation of space physics data; proficiency with advanced technical computing using languages such as Python, IDL, Matlab, or another comparable programming language; and a record of published first author scientific papers in peer-reviewed journals. Experience with space hardware is a plus.
Please contact Matt Hill for more information about the exciting science or other aspects of this position (matt.hill at jhuapl.edu). The complete job posting and a link for submitting an application can be found at https://careers.jhuapl.edu/jobs/51892.
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JOB OPENING: Post-doctoral Scholarship (2 Years) in Modelling Plasma Interaction with Planetary Bodies
From: Shahab Fatemi (shahab.fatemi at umu.se)
Dear all,
The Department of Physics at Umeå University in Sweden is offering a postdoctoral scholarship in modeling plasma interaction with planetary bodies. The scholarship is full-time for two years and the start date will be 1 April, 2023 or by agreement. The aim of our project is to advance our current understanding on the kinetic interaction between the solar wind and planetary bodies of different sizes and characteristics with the main focus on atmospheric evolution using a hybrid model of plasma. Application deadline is 10 Feb 2023.
For more information, please see the job advertisement in the link below:
https://www.umu.se/en/work-with-us/postdoctoral-scholarships/7-1639-22/
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JOB OPENING: Post-doctoral Position in Space Weather
From: Dr Peter Wintoft (peter.wintoft at irf.se )
Post-doctoral position in space weather
Swedish Institute of Space Physics is looking for a post-doctoral position, placed in Lund, in space weather with focus on detection and characterization of coronal mass ejections.
Space weather impacts technology through physical processes originating from the Sun and its interaction with the Earth’s magnetosphere and ionosphere. The effects on technology are well-known and may influence the operation and performance of satellites, communication, navigation, and electrical power distribution.
A key component in the solar-terrestrial system is the detection and characterization of coronal mass ejections.
The work will include analysis of coronal images from various spacecraft, analysis of in-situ solar wind data, and development of methods and algorithms. The goal is to develop models for automatic detection of coronal mass ejections as part of IRF’s space weather system.
The postdoctoral position will be part of IRF’s group on space weather, which includes scientists, software developers, and engineers from IRF’s different offices. IRF is a member of the International Space Environment Service and is responsible for Regional Warning Centre Sweden.
IRF also takes part in ESA’s Space Safety Programme within the Geomagnetic Expert Service Centre. The position will be part of international collaborations through existing networks but will also include the development of new networks.
We expect that you have relevant knowledge of plasma physics, solar-terrestrial physics, and space weather. Further, knowledge in one or several fields of statistical data analysis, machine learning, image analysis, and time series analysis is a merit. Our main programming language is Python.
For more information contact:
Dr Peter Wintoft, +46-46 286 21 21, peter.wintoft at irf.se
Closing date for applications is 31 January 2023.
Read more: https://www.irf.se/en/news/2023/01/02/post-doctoral-position-in-space-weather-ref-2-2-1-474-22/
Swedish Institute of Space Physics (IRF) is a governmental research institute that conducts postgraduate education and research in space physics, atmospheric physics and space technology. Many of IRF’s projects are run as large international projects in collaboration with other research institutes and space agencies. IRF has about one hundred employees and offices in Kiruna (headquarters), Umeå, Uppsala and Lund. www.irf.se
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