Month: March 2019

VarSITI Closing Symposium

VarSITI Closing Symposium
June 10-14, 2019
Sofia, Bulgaria
http://newserver.stil.bas.bg/VarSITI2019/

VarSITI, the scientific program of SCOSTEP focuses on the recent and expected future solar activity and its consequences for the Earth, over various time scales from thousands of years to milliseconds, and at various locations from the solar interior to the Earth’s atmosphere. In particular, VarSITI focuses on the interconnections in the Sun-Earth system, and encourages the interaction among scientists working on different aspects of this complex system. The VarSITI program is coming to an end. For five years, more than 1,100 scientists from 71 countries have been working on its four scientific projects:

SEE (Solar Evolution and Extrema),
MiniMax24/ISEST (International Study of Earth-affecting Solar Transients),
SPeCIMEN (Specification and Prediction of the Coupled Inner-Magnetospheric Environment), and
ROSMIC (Role Of the Sun and the Middle atmosphere/thermosphere/ionosphere In Climate)

The purpose of this Closing Symposium is to summarize the results of the program, discuss what progress has been made, what new scientific questions have emerged and what should be the focus of the next scientific program. The community is invited to participate in this closing meeting. Further details are available at the conference web page.

Scientific Organizing Committee

http://newserver.stil.bas.bg/VarSITI2019/continue to the full article

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RHESSI Nuggets in March 2019

No. 347, “Persistent quasi-periodic pulsations detected during the large X8.2 solar flare,” by Laura Hayes and Peter Gallagher: The most beautiful flare has the most beautiful pulsations!

No. 346, “Is the coronal magnetic field braiding?” by Markus Aschwanden. An iconic cartoon does not relate well to the observations.

We welcome contributions to the RHESSI Nuggets, and the topics may wander some distance away from specifically RHESSI results if they are generally interesting. See
http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggetscontinue to the full article

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Two tokamak MHD Physicist positions at UKAEA

UKAEA-CCFE has two positions at the post doc level for MHD Physicists. These roles will look at the MHD stability of the JET and MAST-U tokamaks on the Culham site as well as collaborate internationally.

The successful candidates can be either experimentalists or theoreticians. This is an exciting time for Culham as MAST-U is just coming to the end of a major upgrade and will be operating soon. JET is planning a new set of DT plasmas in the next couple of years.

Please contact Christopher Ham (Christopher.ham@ukaea.uk) for more details or go to https://www.ccfe.ac.uk/Jobs.aspx.

https://www.ccfe.ac.uk/Jobs.aspxcontinue to the full article

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University of Glasgow – PDRA position in Solar Physics

The following position is available at the University of Glasgow, funded from June 2019 to the end of 2020, with an application deadline of 24 April 2019. This project is funded by the Royal Society and is looking at DEM analysis of the solar atmosphere using EUV/X-ray data, as well as some code development. So candidates should have good knowledge of working with astronomical data in IDL and/or Python.

To apply, follow the link below, or https://www.gla.ac.uk/it/iframe/jobs/ using ref 024911.

For further information about the position please contact iain.hannah@glasgow.ac.uk

Job Purpose

You will contribute to a project (Probing the Multi-thermal Solar Atmosphere) working with Dr Iain Hannah. Specifically, the job requires expert knowledge in the astronomical data analysis, particularly of the Sun. The successful candidate will also be expected to contribute to the formulation and submission of research publications and research proposals as well as help manage and direct this complex and challenging project as opportunities allow.

Standard Terms & Conditions

Salary will be on the University’s Research and Teaching Grade, level 6/7, £28,660 – £32,236 / £35,210 – £39,610 per annum.

This post is full time at 35 hours per week with funding up to 19 months in the first instance.

New entrants to the University will be required to serve a probationary period of 6 months.

The successful applicant will be eligible to join the Universities’ Superannuation Scheme. Further information regarding the scheme is available from the Superannuation Officer, who is also prepared to advise on questions relating to the transfer of Superannuation benefits.

All research and related activities, including grants, donations, clinical trials, contract research, consultancy and commercialisation are required to be managed through the University’s relevant processes (e.g. contractual and financial), in accordance with the University Court’s policies.

It is the University of Glasgow’s mission to foster an inclusive climate, which ensures equality in our working, learning, research and teaching environment.

We strongly endorse the principles of Athena SWAN, including a supportive and flexible working environment, with commitment from all levels of the organisation in promoting gender equality.

The University of Glasgow, charity number SC004401.

https://www.jobs.ac.uk/job/BQY372/research-assistant-associate?utm_campaign=google_jobs_apply&utm_source=google_jobs_apply&utm_medium=organiccontinue to the full article

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University of Colorado Boulder (USA) – Postdoctoral Research Position in Solar Physics

JOB DESCRIPTION:
We invite applications for an NSF/NASA-funded postdoctoral position starting June 1, 2019 or later. Application deadline is April 15, 2019 or until filled.

The goal is to improve our understanding of solar active region magnetic structure and energy budget before and during solar eruptions. To address this goal the candidate will assist with the development and performance of data-driven numerical simulations of the solar eruptions and will validate these with high quality observations taken with space and ground-based observatories, including the Daniel K. Inouye Solar Telescope (DKIST), the largest 4-meter solar telescope in the world. This post is a unique opportunity that will bridge expertise of groups with internationally leading competence in areas of data-driven simulations and space and ground-based observations at the National Solar Observatory (headquarters of DKIST), High Altitude Observatory (HAO) and University of California, Berkeley (UC Berkeley). The candidate will participate in collaborative and independent solar physics research, present results at scientific meetings and publish articles in peer-reviewed scientific journals. A key component of this post will be participation in the NSO Community Science Program activities to become a DKIST Level-2 Ambassador, that includes development and application of DKIST data reduction tools and production of level-2 science data from limited sets of DKIST observations.

REQUIREMENTS:
PhD in Physics, Astronomy, or related field (by the start date). One to three (1-3) years of research experience in solar physics or space plasmas, with at least one (1) first-authored, peer-reviewed article in credited scientific journals. Scientific background in solar physics. Full proficiency in scientific programming with Interactive Data Language (IDL) and/or Python, and C and/or Fortran. Demonstrated ability to analyze solar data and/or perform numerical simulations, conduct independent research and collaborate with colleagues, communicate scientific ideas effectively in person and on paper.

DEADLINE: April 15, 2019 or until filled. Applications received after this deadline may be considered only if the position is not filled.

START DATE: June 1, 2019 or later.

INQUIRIES: Dr. Maria Kazachenko, maria.kazachenko@colorado.edu.

APPLICATION LINK AND FURTHER DETAILS: https://jobs.colorado.edu/jobs/JobDetail/Postdoctoral-Research-Position-in-Solar-Physics/16728

https://jobs.colorado.edu/jobs/JobDetail/Postdoctoral-Research-Position-in-Solar-Physics/16728continue to the full article

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UK Solar Orbiter workshop – Registration now open

UK Solar Orbiter Workshop – Second announcement
Date : 3rd-4th June 2019
Venue : UCL Gordon Square 25, London

Registration now open at https://sites.google.com/view/ukso-19/registration

Solar Orbiter is an ESA/NASA mission designed to answer some of the key questions in heliophysics, from the origin and variability of the solar wind to the link between solar eruptions, magnetic fields and energetic particles. Solar Orbiter will have a unique combination of in-situ and remote-sensing instruments, probing the atmosphere close to the Sun in and out of the ecliptic plane. The modeling of the magnetic environment that will be experienced by the satellite and its connection to the Sun will be key to the success of both the in-flight operations as well as to the mission’s scientific goals.

With the launch of Solar orbiter scheduled for February 2020, the UK solar Orbiter Workshop aims to bring together the expertise of the UK solar community in magnetic modeling and model validation, to increase the UK impact on the international efforts in preparation for Solar Orbiter operations, and to coordinate the UK efforts for the exploitation of the satellite observations.

All members of the UK solar physics community interested in the Solar Orbiter mission goals are encouraged to attend.

Registration is now open and will close on May 15th. Due to venue limitations the number of participant is capped, and early registration is encouraged.

For information please email uk-solo@mssl.ucl.ac.uk

https://sites.google.com/view/ukso-19continue to the full article

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“Scintillating Science: Cutting-Edge Science Achieved Through the Observations of Radio Scintillation” Workshop – First Announcement

Dear Colleagues.

Following our save-the-date announcement a few months ago, we would like to provide you with the official first announcement for our upcoming “Scintillating Science: Cutting-Edge Science Achieved Through the Observations of Radio Scintillation” focussed/specialist workshop which will be held in Hermanus (near Cape Town), South Africa, the week of 15th July 2019.

The workshop will cover all aspects of scintillation from the science (including all the domains in which it can be applied, e.g. ionosphere, heliosphere, interstellar) through to engineering concepts/requirements including all aspects of its theory/modelling. We are in the process of putting together more-detailed themes and these will appear on the workshop website before the end of March 2019. In addition, we are in the process of setting out invited speakers and scene-setting speakers.

Early registration and abstract submission opens very soon on 25th March 2019. The full list of deadlines can be found on the workshop website here: https://www.ukssdc.ac.uk/meetings/SSCESATORS/ along with further information about the scope of the workshop and local information.

Best wishes on behalf of the workshop SOC and LOC,

Mario M. Bisi (UKRI STFC RAL Space – SOC Co-Chair)
Mike Kosch (SANSA/Lancaster University – SOC Co-Chair/LOC Chair)

Science Organising Committee (SOC):
Mario M. Bisi (UKRI STFC RAL Space, UK) (Co-Chair)
Michael Kosch (SANSA, South Africa/Lancaster University, UK) (Co-Chair)
Richard A. Fallows (ASTRON, NL)
Daniel Stinebring (Oberlin College and Conservatory, OH, USA)
Anna Bilous (University of Amsterdam, NL)
Ue-Li Pen (University of Toronto, ON, Canada)
Lucilla Alfonsi (INGV, Italy)
Joseph Olwendo (Pwani University, Kenya)
Biagio Forte (University of Bath, UK)
Tshimangadzo Matamba (SANSA, South Africa)
Oyuki Chang (UKRI STFC RAL Space, UK)

Local Organising Committee (LOC):
Michael Kosch (SANSA, South Africa/Lancaster University, UK)
Lee-Anne McKinnell (SANSA, South Africa)
Tshimangadzo Matamba (SANSA, South Africa)

https://www.ukssdc.ac.uk/meetings/SSCESATORS/continue to the full article

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9th Coronal Loops Workshop – St Andrews (UK), 11-14 June 2019

The 9th Coronal Loops Workshop will be held at the School of Mathematics and Statistics at the University of St Andrews from 11th-14th June 2019.

Registration and abstract submission are now open. Please visit https://loops9.wp.st-andrews.ac.uk/

for information on registration, abstract submission, accommodation and travel.

Confirmed Invited Speakers:

Boris Gudiksen (Rosseland Centre for Solar Physics, University of Oslo)
Amy Winebarger (NASA Marshall Space Flight Center)
Will Barnes (Rice University)
Inigo Arregui (Instituto de Astrofísica de Canarias)
David Pontin (University of Dundee)
Moira Jardine (University of St Andrews)
Vanessa Polito (CfA, Harvard)

Important Dates:

Deadline early-career financial support: 29 March 2019
Deadline abstract submission: 29 March 2019
Deadline Early bird registration: 3 May 2019
Final registration date: 17 May 2019

https://loops9.wp.st-andrews.ac.uk/continue to the full article

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CESRA Workshop 2019: – registration and abstract submission are open

Dear Colleagues,

We are pleased to announce registration/abstract submission for the next CESRA Workshop, “CESRA2019: The Sun and the inner heliosphere” which will be held on July 8th – 12th, 2019, at Telegrafenberg, Potsdam, Germany.

http://meetings.aip.de/cesra2019/cms/

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.

To register and to submit the abstract please follow the link: http://meetings.aip.de/cesra2019/registration/

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.

On behalf of the CESRA Board and the local SOC representatives,
Eduard Kontar, Gottfried Mann, Alexander Warmuth

http://meetings.aip.de/cesra2019/cms/continue to the full article

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Partially Ionised Plasmas in Astrophysics PIPA2019 (Mallorca, Spain) — 2nd Announcement: deadline April 1st

It is our pleasure to invite you to participate in the Partially Ionised Plasmas in Astrophysics (PIPA2019) conference, to be held in Mallorca in June 3-7, 2019. The meeting will provide a forum for the exchange of ideas between participants from all areas of Astrophysics in which partially ionised plasmas play a capital role, from the Earth’s ionosphere to partially ionised regions in galaxies, which also includes solar chromosphere, interstellar medium, stellar formation, protostellar discs, planetary magnetospheres and ionospheres, etc.

Information about the venue, accommodation, preliminary invited speakers and talks, etc. is available at:  http://solar1.uib.es/pipa2019/

Registration and Abstract submission deadline — April 1, 2019
Hotel reservation deadline — April 1, 2019

The LOC of the PIPA2019 meeting is looking forward to welcome you to Mallorca,

Ramón Oliver, Elena Khomenko, Istvan Ballai

http://solar1.uib.es/pipa2019/continue to the full article

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