[GEM] THE GEM MESSENGER, Volume 28, Number 63

[Newsletter Editor]

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     THE GEM MESSENGER
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Volume 28, Number 63
Dec.21,2018

Announcement submission website: http://aten.igpp.ucla.edu/gem/messenger_form/

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Table of Contents

1. Harnessing the Data Revolution (HDR): Institutes for Data-Intensive Research in Science and Engineering - Ideas Labs

2. EGU 2019 Session ST3.3/EMRP2.6/G4.5: Dynamics and interaction of processes in Earth and its space environment

3. EGU 2019 Session NP6.7/PS4.4/ST2.8  Turbulence, magnetic reconnection, shocks and particle acceleration: nonlinear processes in space, laboratory and astrophysical plasmas

4. EGU 2019 Session PS4.1: Planetary Space Weather: fundamental plasma interactions in space environments

5. JOB OPENING: Postdoctoral Positions in Magnetospheric Physics at Rice University

6. JOB OPENING: Post-Doctoral Associate at New Jersey Institute of Technology

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1. Harnessing the Data Revolution (HDR): Institutes for Data-Intensive Research in Science and Engineering - Ideas Labs
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From: Michael Wiltberger (mwiltber at nsf.gov)

The overarching goal of the HDR Institutes DIRSE Ideas Labs is to foster convergent approaches to enable data-intensive research in science and engineering through a series of facilitated activities bringing together scientists and engineers working on important data-intensive science and engineering problems with data scientists, e.g., computer and computational scientists, mathematicians, statisticians, and information scientists with expertise in different aspects of modeling and data analysis as well as systems and cyberinfrastructure specialists with expertise in open source software development, reproducibility, and transfer learning.  The Ideas Labs will focus on areas that: (1) are at a “tipping point” where a timely investment in data-intensive approaches has the maximum potential for a transformative effect; (2) have needs that can benefit from interdisciplinary investments in data analytics infrastructure; and (3) represent investment priorities for NSF science and engineering directorates during, and beyond, the lifetime of the HDR Big Idea. 

US researchers may submit preliminary proposals for participating in the Ideas Labs only via Fastlane.  Based on the number of preliminary proposals and the science and engineering areas and data science expertise represented by the applicant pool, one or more Ideas Labs may be scheduled in parallel. Participation in an Ideas Lab is required to be eligible to submit a full conceptualization proposal pursuant to this solicitation. Multidisciplinary ideas developed in an Ideas Lab will be submitted as full conceptualization proposals to NSF by invitation only. Interdisciplinary collaboration among researchers is required in the invited full conceptualization proposals.

The deadline for preliminary proposals by individuals wishing to participate is January 28, 2019.  The full Ideas Lab itself will occur on April 22-26, 2019.

Full solicitation at

HTML - https://nsf.gov/pubs/2019/nsf19543/nsf19543.htm 
PDF - https://nsf.gov/pubs/2019/nsf19543/nsf19543.pdf


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2. EGU 2019 Session ST3.3/EMRP2.6/G4.5: Dynamics and interaction of processes in Earth and its space environment
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From: Claudia Stolle, Patrick Alken, Alexander Grayver, Adrian Jaeggi, Rumi Nakamura (cstolle at gfz-potsdam.de)

Dear colleagues,

We would like to draw your attention to the following interdisciplinary session at the EGU General Assembly 7-12 April 2019 in Vienna and invite you to consider submitting an abstract:

ST3.3/EMRP2.6/G4.5:
Dynamics and interaction of processes in Earth and space environment: global observations and modelling

Many recent advances in space sciences, geomagnetism, and gravity arose from combining specific knowledge of these areas in interdisciplinary research. Questions addressed are, for example: What features of ionospheric currents do we discover when we understand the shape, strengths, and variation of the geomagnetic background field, e.g., with respect to influences by upward propagating atmospheric waves? Which ionospheric processes need to be better quantified to achieve complete knowledge of global core or crustal field variations? How does knowledge of the geometry of ionospheric and magnetospheric sources help in determining Earth’s conductivity in the geomagnetic field? How strongly do we need to consider Earth’s conductivity in quantifying ionospheric currents? How can we quantify and correct for ionospheric perturbations to achieve the best gravity field solutions? Finally, what can we learn about space sciences by studying ionospheric effects on geodetic measurements?

The session invites contributions on any of the subjects and in particular on results that benefit from interdisciplinary works in the areas of space science, geomagnetism, and gravity. Submissions are welcomed that contain analyses of global satellite or ground observations or modelling studies, including a combination of both.

Abstracts can be directly submitted from
https://meetingorganizer.copernicus.org/EGU2019/session/31918

The abstract submission deadline is 10 January 2019, 13:00 CET.

Kind regards,
the conveners Claudia Stolle, Patrick Alken, Alexander Grayver, Adrian Jaeggi, Rumi Nakamura


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3. EGU 2019 Session NP6.7/PS4.4/ST2.8  Turbulence, magnetic reconnection, shocks and particle acceleration: nonlinear processes in space, laboratory and astrophysical plasmas
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From: Giovanni Lapenta (giovanni.lapenta at kuleuven.be)

Dear colleagues,

we would like to draw your attention to the following EGU 2019 session:

NP6.7/PS4.4/ST2.8

Title: Turbulence, magnetic reconnection, shocks and particle acceleration: nonlinear processes in space, laboratory and astrophysical plasmas 

Abstract link: https://meetingorganizer.copernicus.org/EGU2019/session/30643

Abstract: Turbulence, reconnection and shocks are fundamental non-linear processes observed in solar, heliospheric, magnetospheric and laboratory plasmas. These processes are not separate, but rather appear to be interconnected. For instance, a close link exists between reconnection and turbulence. On the one hand the turbulence cascade favors the onset of magnetic reconnection between magnetic island and, on the other hand, magnetic reconnection is able to trigger turbulence in the reconnection outflows and separatrices. Similarly, shocks may form in collisional and collisionless reconnection processes and can be responsible for turbulence formation, as for instance in the turbulent magnetosheath.
This session welcomes simulations, observational and theoretical works relevant for the study of these non-linear phenomena. Particularly welcome will be works focusing on the link between them in a range of scale going from fluid MHD to kinetic. The topic of this session is relevant for the understanding of solar atmosphere (from the photosphere to the solar wind), interaction of solar wind with planetary magnetospheres, planetary magnetospheric physics and particle acceleration and transport throughout the heliosphere. The session is also relevant to past and present space missions in plasma astrophysics such as Cluster, MMS and Parker Solar Probe.

The EGU 2019 will take place in Vienna on 7-12 April. The deadline for abstract submission is 10 January 2019, 13:00 CET.

We hope to see you in Vienna,

Best regards,

Francesco Pucci, Maria Elena Innocenti, Alexandros Chasapis, Giovanni Lapenta


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4. EGU 2019 Session PS4.1: Planetary Space Weather: fundamental plasma interactions in space environments
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From: Zhonghua Yao, Philippe Garnier, Valeria Mangano (zhonghua.yao at uliege.be)

As conveners of the session PS4.1 entitled “Planetary Space Weather” at EGU 2019 conference to be held on 7 - 12 April in Vienna, Austria, we would like to invite researchers in the planetary space weather community to submit abstracts to the above session.

For detailed information, see: 
https://meetingorganizer.copernicus.org/EGU2019/abstractsubmission/31979

The emphasis of the session is on crucial processes of planetary space weather, that is, plasma physics and interactions of the interplanetary medium with the Solar System bodies, including:
(a) magnetosphere-ionosphere coupling dynamics and auroras: from the Earth to other planets
(b) the solar wind interaction with planets, moons, asteroids and comets
(c) plasma interactions with exospheres, dust and surfaces
(d) surface space weathering
(e) potential impact of planetary environment on technological space systems
(f) inter-comparisons of planetary environments

Contributions are welcome which address previous (e.g. Chandrayaan-1, KAGUYA, Venus Express, MESSENGER, Rosetta, Cassini), present (e.g. Juno,
Mars Express, MAVEN, CHANG'E 2), forthcoming (e.g. BepiColombo, Parker Solar Probe) and planned (e.g. JUICE, Solar Orbiter) observations from space. Analyses of ground-based observations of neutral and ionized environments are welcome, as well as laboratory studies aiming to simulate the interactions on planetary analogues in space. Theoretical modeling and simulations are also strongly encouraged, both in themselves and as a basis for inter-comparisons and interpretation of measurements. Regarding that major breakthroughs on terrestrial space weather have been made with measurements from THEMIS, Cluster, AMPERE, MMS and Van Allen Probes, we very welcome the relevant topics at the Earth too, as comparative study has proven to be a powerful tool in understanding planetary space weather.

The deadline for abstract submission is 10 Jan 2019, 13:00 CET. We appreciate for your consideration of submission of your relevant research to our session. 

Hope to see you in Vienna! 


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5. JOB OPENING: Postdoctoral Positions in Magnetospheric Physics at Rice University
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From: Frank Toffoletto and Stanislav Sazykin (toffo at rice.edu)

The magnetospheric modeling group at Rice University expects one or two postdoctoral openings to begin in early 2019 to work on fundamental physics of the inner magnetosphere and plasmasheet, the ring current and magnetosphere-ionosphere coupling. One position would be in model development. For this position, experience in magnetospheric model development, parallel programming and running large computer codes on supercomputers is highly desirable. The second position is in model-data comparisons. Proficiency in using computer models as is experience analyzing spacecraft and ground based-data is desirable. Candidates who have experience in both areas are also encouraged to apply. A Ph.D. in space physics is required for both positions. Initial appointment is anticipated for one year, with renewal likely for a second year, contingent on performance and availability of research funds.

Candidates should supply a curriculum vitae, a brief statement of research interests, and names of three references online at: https://jobs.rice.edu/postings/17876. 

Information on the group’s research activities can be found at http://physics.rice.edu/Space.aspx.  

Rice University is an affirmative-action/equal-opportunity employer.


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6. JOB OPENING: Post-Doctoral Associate at New Jersey Institute of Technology
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From: Hyomin Kim (hmkim at njit.edu)

Position Summary:
The Center for Solar-Terrestrial Research (CSTR) of the New Jersey Institute of Technology (NJIT) invites applications for a postdoctoral position in data analysis for magnetospheric and ionospheric studies. The successful candidate will make use of various data sets including, but not limited to,  spacecraft data such as Van Allen Probes, MMS, THEMIS, and Cluster, and ground-based instruments such as magnetometers, auroral imagers, riometer, GPS and incoherent scatter radars to investigate solar wind-magnetosphere-ionosphere coupling processes. CSTR operates ground-based geospace science instruments at high latitudes. Thus, experience in science instrument development, testing and installation is highly desired. Occasional domestic or international travel for instrument installation and service may be expected. 

The successful applicant will be expected to perform the duties of a post-doctoral fellow, including the publication of original research, submission of proposals, and the support of CSTR projects.
Applicants should have obtained by the starting date a PhD in plasma physics, space physics, geophysics, or related field. The start date of the appointment is flexible, however, earlier dates are preferred. The appointment is for one year, with a possible renewal for two more years based on successful applicant performance. Benefits are competitive and salary will be commensurate with applicant experience. 

The successful applicant will work primarily with Dr. Hyomin Kim, Assistant Professor of NJIT as well as the other CSTR faculty members including Drs. Andrew Gerrard, Louis Lanzerotti, Rualdo Soto-Chavez and Nathaniel Frissell. 

Candidates will need to submit a curriculum vitae, a list of publications, a brief statement of research interests, and the names of three professional references. Questions may be directed to Dr. Hyomin Kim (hmkim at njit.edu). 

The Center for Solar-Terrestrial Research (CSTR) of the New Jersey Institute of Technology, in Newark, NJ, is a worldwide leading institution in solar and space physics. CSTR is a PI organization in the NASA Van Allen Probes mission, manages the Polar Engineering Development Center, and operates the Big Bear Solar Observatory (BBSO) and the Owens Valley Solar Array (OVSA) in California. For more information visit http://centers.njit.edu/cstr/

To build a diverse workforce, NJIT encourages applications from individuals with disabilities, minorities, veterans and women. EEO employer.

Essential Functions:
Data analysis utilizing programming languages such as Python and/or IDL.  
Presentation of results at professional meetings.
Presentation of result via peer-review journal papers.
Occasional domestic/international travel for instrument installation/service

Prerequisite Qualifications:
Ph.D. in Space Physics or related field.
Background in magnetospheric/ionospheric physics.
Experience in data analysis using programming languages.

Preferred Qualifications:
Experience in electronics lab experiment and field work is highly desired.


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