UK Solar Physics Newsletter
Philippa Browning & David Williams, Editors
August 17th 2015
Dear Colleagues,
Here are a few items which have come to our attention since the last
Newsletter.
You can find this news also at the UKSP website:
http://www.uksolphys.org/news/last-15-days/
or the newsletter in full in our JISCMail archive:
http://www.jiscmail.ac.uk/uksp
Dave ([log in to unmask])
Philippa ([log in to unmask])
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General News/UKSP Business:
o Congratulations to Lucie Green!
o Reminder – RCUK Policy Internships for STFC-funded PhD Students
o SunPy 0.6.0 now available
o STFC 2015B Small Awards Scheme
o Announcement of a Special Section in JGR
o STEREO Operations Resume Post Solar Conjunction
o Media & Communications Training
Nuggets:
o New UKSP Nugget #59
o August 2015 – New EIS Nugget – Relative Abundance Measurements in
Plumes and Interplumes
Meetings/Workshops/Summer Schools:
o IFIERI Summer School
o UK Solar Missions Forum 2016 – date for your diary
Jobs/Studentships:
o 5-year research positions in Astrophysics in Portugal (update)
o Solar/Heliophysics Research Associate Position at NOAA/SWPC and
the University of Colorado, CIRES
o Interface Region Imaging Spectrograph (IRIS) post-doctoral
position (Palo Alto, CA, USA)
o NASA Headquarters Heliophysics Visiting Scientist
o Solar Orbiter Instrument Operations Scientist
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Congratulations to Lucie Green
July 28, 2015, from David Williams (UKSP DC)
We’re proud to announce that Lucie Green has just been promoted to
Professor at Mullard Space Science Lab, University College London.
Well done, Prof. Lucie – thoroughly deserved!
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Reminder – RCUK Policy Internships for STFC-funded PhD Students
August 17, 2015, from Dave Godfrey
(Formerly known as POST Fellowships)
STFC participates in the Research Councils Policy Internships scheme, a
programme in which STFC-funded PhD students are given the opportunity to
spend three months working in Parliament. Opportunities are available
with the Parliamentary Office of Science and Technology (POST) or the
Government Office for Science (GO Science).
Applications for the 2016 scheme are now open.
The scheme presents a unique opportunity for PhD students to gain an
insight into the political process. Fellows learn how policy is
developed, interact with policy makers and develop the skills needed to
communicate effectively with non-academic audiences.
• POST is an independent office of the Houses of Parliament whose role
is to provide clear, expert, impartial advice on science to MPs and
Peers. Its goal is to keep them up to date on current scientific issues
and allow them to make informed decisions. Fellows either work on a
‘POST Note’ or research project, or provide specialist advice to a
Parliamentary Select Committee or the House of Commons Library.
• GO Science looks to ensure that government policies and decisions are
informed by the best scientific evidence and strategic long-term
thinking. Placements are likely to involve undertaking research,
drafting briefing notes and background papers, and organising workshops
and meetings. They will offer opportunities to work with a number of
different teams and across a wide range of science and technology policy
topics in GO Science.
The successful applicant will receive funding for their secondment
period and will receive a three-month extension to their STFC PhD
status. Fellows will receive a stipend equivalent to that of a
London-based PhD student for three months. Fellows based at non-London
institutions will receive an additional sum to cover the costs of
relocating to London for three months.
For further information and how to apply, please visit the Research
Councils Policy Internships webpage.
Applications for the 2016 Internships close at 4pm on Friday 28 August
2015. For applications to a placement in POST, interviews will be held
during the week beginning 12 October in Parliament.
Further information:
• Parliamentary Office of Science and Technology
(http://www.parliament.uk/post)
• Government Office for Science
(https://www.gov.uk/government/organisations/government-office-for-
science)
(• STFC Policy Internships
(http://www.stfc.ac.uk/funding/fellowships/policyinternships/)
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SunPy 0.6.0 now available
August 17, 2015, from SunPy Collaboration
The SunPy Community is pleased to announce that SunPy version 0.6.0 is
now available. SunPy is a community-developed, free and open-source
solar data analysis environment for Python. To install (or upgrade
to) SunPy 0.6.0, please follow the instructions at
http://docs.sunpy.org/en/stable/guide/installation/index.html .
In this release, we’ve performed a major overhaul of our documentation
to help new users get started as well as provide better support for
advanced users. We have also added support for using physical
quantities with units, significantly improved map plotting, and now
provide better support for the acquisition of sample data. For an
overview of the improvements to SunPy, please go to
http://sunpy.org/gallery/Introductory/SunPy_0.6_Release.html .
This release contains contributions from 29 people, including 13 new
contributors. We would also like to thank the Python Software
Foundation and the Google Summer of Code 2014 and ESA Summer of Code
in Space 2014 internship programs for their support of SunPy.
We would like to hear your feedback. Please visit sunpy.org for
more information on SunPy, including contact details and how to contribute.
sunpy.org
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STFC 2015B Small Awards Scheme
August 17, 2015, from Dave Godfrey
STFC has announced that the 2015B Small Awards scheme round is open. The
closing date for applications is Thursday 8th October at 4.00pm.
The Public Engagement Small Awards Scheme provides funds for small,
local or ‘pilot’ projects promoting STFC science and technology. Almost
anyone can apply, including grant-funded research groups, STFC research
facility users, schools, museums, etc. Awards range from £500 to £10,000
and the expenditure can go towards materials, salaries and travel &
subsistence.
Projects must be relevant to publicising engagement or teaching about
the STFC science and technology areas, namely:
• particle physics
• nuclear physics
• space, solar and planetary science
• astronomy
• astrophysics
• cosmology
• studying materials with muon and neutron sources
• studying materials with synchrotron light sources
• research using laser facilities
• other science areas
Applicants are advised to consult the STFC Public Engagement Strategy
(http://www.stfc.ac.uk/files/public-engagement-strategic-plan/) in
advance of submitting your proposal and are also encouraged (if
applicable) to consider working with under-represented audiences such as
girls and young women in engineering and physics, groups in areas
geographically remote from STEM activity and underperforming schools.
Please see the notes for guidance
(http://www.stfc.ac.uk/files/pe-small-awards-guidance-notes-2014/)
for further information.
All applications must be submitted through the RCUK Je-S system
(https://je-s.rcuk.ac.uk/JeS2WebLoginSite/Login.aspx). E-mailed or hard
copy applications will not be accepted.
The scheme is administered by the STFC Public Engagement Team.
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Announcement of a Special Section in JGR
July 29, 2015, from Bo Li
Title for Special Section:
Nature of Turbulence, Dissipation, and Heating in Space Plasmas: From
Alfvén Waves to Kinetic Alfvén Waves
Guest Editors:
Dr. De-Jin, Wu (Purple Mountain Observatory, Chinese Academy of Sciences)
Dr. Heng-Qiang, Feng (Institute of Space Physics, Luoyang Normal University)
Dr. Bo, Li (Institute of Space Sciences, Shandong University)
Dr. Jian-Sen, He (School of Earth and Space Sciences, Peking University)
Submission Start Date: 1 September 2015
Submission Deadline: 30 November 2015
We cordially invite you to submit your papers to this Special Section of
JGR-Space Physics, which covers topics across the full spectrum of wave
phenomena from large MHD scales to small kinetic scales relevant to
diverse space plasma regions from the Earth’s magnetosphere and
ionosphere to the solar wind and the solar atmosphere.
In this open duration you can submit your paper by using the regular
submission system of JGR. On the submission page, when drop-down menu
shows up asking if your submission is for a special section, please
select “Yes” with “Our Special Section”.
Although this Special Section is intended for the papers to be presented
at the ST-13 session of the same title during the 12th AOGS Annual
Meeting, other papers not presented in this session are equally welcome.
We would like to emphasize that manuscripts submitted to this special
issue will be peer reviewed as regular JGR submissions and will be
published online as ready. Each accepted paper will immediately be added
to the online table of contents of this special issue. After the last
paper in the issue is published, the collection of papers will appear in
a future print issue.
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STEREO Operations Resume Post Solar Conjunction
July 29, 2015, from David Williams (UKSP DC)
The two NASA STEREO spacecraft have, over the last few months, been in
superior conjunction ─ a time during which they were completely out of
Earth-contact due to their being behind the Sun ─ from which they are
now emerging.
Launched in 2006, the STEREO mission comprises two near-identical
space-based observatories in heliocentric orbits ─ one leading
(STEREO-A) and the other lagging (STEREO-B) the Earth ─ with the aim of
providing the first ever stereoscopic measurements to study the Sun and
the nature of its coronal mass ejections (CMEs). After some 8 years of
highly successful and scientifically productive operation, both
spacecraft passed behind the Sun from the vantage point of Earth.
On approach to superior conjunction, it was, however, found that the
operational temperature of the STEREO high-gain antenna (HGA) on each
spacecraft was increasing markedly, due to their near-Sun pointing. To
mitigate the potentially damaging temperature increase, strategies were
devised for continued operation ─ either side of superior conjunction ─
based on the use of the HGA first and second side-lobes, rather than the
main beam. Off-pointing the HGA away from the Sun has enabled the
continued downlink of an, albeit reduced, data stream either side of the
inevitable, but relatively brief, complete loss of downlink associated
with superior conjunction.
On July 11, the first images in over three months were received from
STEREO-A, the spacecraft having emerged from superior conjunction. The
spacecraft, and all of its instruments, have been deemed fully
operational. It should be noted that, unfortunately, STEREO-B
encountered a severe problem prior to entering superior conjunction ─
associated with a planned reset performed as a test of solar conjunction
operations ─ resulting in a complete loss of contact. NASA will shortly
be resuming efforts to re-establish contact with STEREO-B, and there is
continued hope that the spacecraft will be recovered. However, with or
without STEREO-B, we still have a heliophysics observatory that rated
extremely highly in the recent NASA Senior Review.
All of the imaging instruments on STEREO incorporate UK camera systems
(RAL-e2v) and the STEREO/Heliospheric Imager (HI) instruments are led
from the UK. The STEREO/HI instruments are not only the principal tools
used for imaging CMEs, and other solar wind transients, in the
heliosphere, but are also regularly used for the study of comets,
stellar variability, dust and other phenomena. We look forward to the
continuation of this highly productive mission and, as always, are very
happy to discuss the exploitation of HI and other STEREO data with
potential users.
For additional information on the emergence of STEREO-A from solar
conjunction, please see:
http://stereo.gsfc.nasa.gov/news/news.shtml
and links therefrom.
For additional information regarding the superior conjunction, and the
reduced STEREO science operations associated with HGA side-lobe
operations, please see
http://stereo-ssc.nascom.nasa.gov/solar_conjunction.shtml
and links therefrom.
For additional information regarding the loss of contact with STEREO-B,
please see
http://stereo-ssc.nascom.nasa.gov/behind_status.shtml
and links therefrom.
Richard Harrison, STEREO/HI Principal Investigator
Jackie Davies, STEREO/HI Project Scientist
RAL Space
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Media & Communications Training
July 23, 2015, from Dave Godfrey
The Science and Technology Facilities Council offers free Media Skills
training and Writing about your Research courses for researchers, as
part of its Public Engagement programme.
The Media Skills training develops skills in working with television,
radio, newspapers and other media. The next course date is 7 October
2015, in London
The Writing about your Research course trains researchers to write about
their research for non-specialist readers in a variety of contexts. The
next course date is 2 September 2015, in London.
A two-day residential combination of the courses is also available.
These are held at the Kavli Royal Society International Centre in
Buckinghamshire. The next dates are 2/3 November 2015.
STFC offers bursaries to pay the course fees and T&S costs for eligible
researchers. The courses are run for us by the Royal Society. To book a
place visit the Royal Society website
Once you have a confirmed place, go to the STFC website to apply for an
STFC bursary.
The STFC contact for more information is [log in to unmask] Tel 01793
442030
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New UKSP Nugget #59
July 31, 2015, from Iain Hannah
59. Propagating Sausage Mode Waves Damping in the Chromosphere
by Samuel Grant and David Jess (Queen’s University Belfast)
ROSA observations of energy leaking from MHD waves in pores
http://www.uksolphys.org/?p=10279
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UKSP Nuggets are published on a monthly basis highlighting solar physics
research led from the UK.
http://www.uksolphys.org/uksp-nuggets
Iain Hannah and Lyndsay Fletcher
http://www.uksolphys.org/?p=10279
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August 2015 – New EIS Nugget – Relative Abundance Measurements in Plumes and Interplumes
July 17, 2015, from Deb Baker
We are pleased to announce a new EIS Nuggets for August 2015 entitled –
‘Relative Abundance Measurements in Plumes and Interplumes’
by C. Guennou, M. Hahn, D.W. Savin.
The nugget link is:
http://solarb.mssl.ucl.ac.uk/SolarB/nuggets/nugget_2015aug.jsp
The nugget archive can be found here:
http://solarb.mssl.ucl.ac.uk/SolarB/eisnuggets.jsp
We welcome contributions from the community.
Best wishes,
Deb Baker
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IFIERI Summer School
August 17, 2015, from Dave Godfrey
Dear All
Ian Tomalin is helping to organise this year’s INFIERI summer school
https://indico.desy.de/internalPage.py?pageId=9&confId=12535 in Hamburg,
Germany from 15-25 Sept.
The school is aimed at PhD students and postdocs from the fields of
experimental particle physics, astrophysics & medical physics. It aims
to familiarize them with the most advanced readout electronics and
associated infrastructure used in these three fields. It features lots
of hands-on lab sessions, and also lectures by experts, so should be
very educational. The chance to mix with students from other
fields/experiments can also be interesting.
Please feel free to forward this e-mail to key members of the community
or to anyone who would be interested in attending.
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UK Solar Missions Forum 2016 – date for your diary
July 31, 2015, from Louise Harra
The next UK solar missions forum will be on the 7th January 2016 at the
RAS.
The agenda is yet to be decided, and to some extent will depend on what
input the community may be to provide to STFC. We will keep in contact
with Chris Arridge about this. But we will be discussing current and
future plans for facilities which will include space and ground-based
instruments and also computing needs. We will work with Philippa
Browning, Alan Hood, Jackie Davies and Dave Williams to ensure we cover
all bases.
The website that summarises information, about UK mission involvement
and related meetings, is on:
http://www.mssl.ucl.ac.uk/~lkh/UKsolarmissions/
Please let me know if there are any omissions/updates.
Early career stage solar physicists are warmly welcome – these
instruments are developed over long time periods and we need your input!
Louise Harra & Richard Harrison
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5-year research positions in Astrophysics in Portugal
August 12, 2015, from Ilidio lopes
Multidisciplinary Center for Astrophysics
Instituto Superior Técnico
Lisbon, Portugal
(Deadline: 15th September 2015)
The Multidisciplinary Center for Astrophysics (CENTRA) is accepting
applications for 5-year research positions in Astrophysics for the
forthcoming 2015 FCT call. The COSTAR/CENTRA group is looking for
candidates in the topics of asteroseismology, stellar evolution, solar
physics, observational astrophysics, observational cosmology,
theoretical cosmology and particle physics (focus on dark matter and
neutrinos). Candidates can apply for one of three types of grants,
depending of their expertise and experience. If you are interested in
applying in any of these research topics please contact Ilidio Lopes as
soon as possible (see contact details below).
CENTRA is part of the Department of Physics at Instituto Superior
Técnico (IST). The Institute has been consistently the first Institution
chosen by Portuguese undergraduates to pursue their careers in Science,
Engineering and Technology. IST hosts the Portuguese largest scientific
community in theoretical and experimental physics and related topics,
participating in major international European collaborations including
ESA, ESO and CERN. Presently, IST hosts 8 Research Institutes and 25
Research Centres.
Our research center provides a highly supportive academic and scientific
environment giving Ph.D. students and researchers the opportunity to
develop a successful international scientific career. Students and
researchers that, following their academic experience, opt to follow a
business path, can take advantage of the many links that IST has with
the industry.
Contact:
Ilidio Lopes (email): [log in to unmask]
centra.tecnico.ulisboa.pt/team/?id=1650
CENTRA and COSTAR Websites:
centra.tecnico.ulisboa.pt/
centra.tecnico.ulisboa.pt/network/costar/
FCT Website:
www.fct.pt/apoios/contratacaodoutorados/investigador-fct/2015/index.phtml.en
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Solar/Heliophysics Research Associate Position at NOAA/SWPC and the
University of Colorado, CIRES
August 10, 2015, from Alysha Reinard
The Cooperative Institute for Research in Environmental Sciences (CIRES)
at the University of Colorado Boulder has an immediate opening for a
Research Associate supporting NOAA’s Space Weather Prediction Center in
Boulder, Colorado. This person will be responsible for developing and
maintaining operational solar and heliosphere models used by the Space
Weather Forecast Office to predict solar wind conditions and arrival
times of CMEs at Earth.
The immediate focus of this position will be to maintain and improve the
Wang-Sheeley-Arge and Enlil models currently running operationally on
the National Weather Service super computers. The successful applicant
will work with researchers and modelers who develop the space weather
models as well as the forecasters and customers who use the output and
products from the models. This position is fully funded but there will
be opportunities to conduct solar/heliospheric research.
Applicants are required to have a Ph. D. in space physics or similar
scientific discipline, or equivalent demonstrable experience. Applicants
should have demonstrated experience in scientific research including the
development and use of space weather models which incorporate the MHD
approximations. Applicants for this position must also have significant
computer programming skills and a demonstrated capacity for working with
large computer codes and super computers.
Informal inquiries may be made to [log in to unmask] and/or
[log in to unmask]
Further job details may be found at:
cires.colorado.edu/contact/jobs/job-openings/ciresswpc-
scientistprogrammer-research-associate-swpc-6/
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Interface Region Imaging Spectrograph (IRIS) post-doctoral position
(Palo Alto, CA, USA)
August 7, 2015, from Bart De Pontieu
Position/Title: Interface Region Imaging Spectrograph (IRIS)
postdoctoral position
Institutions: BAER Institute, Lockheed Martin Solar & Astrophysics
Laboratory
A 1-year postdoctoral position is available within the Interface Region
Imaging Spectrograph (IRIS) project.
The IRIS small explorer was launched successfully in June 2013 and is
focused on studying the physics of the interface region between the
photosphere and corona. The IRIS science investigation combines a
high-resolution ultraviolet spectrograph with advanced numerical
modeling to study which types of non-thermal energy dominate in the
chromosphere and beyond, how the chromosphere regulates the mass and
energy supplied to the outer solar atmosphere, and how magnetic flux
rises through the solar atmosphere and powers flares and coronal mass
ejections.
The postdoctoral researcher will work with researchers at Lockheed
Martin’s Solar & Astrophysics Laboratory (LMSAL, which leads the IRIS
mission and is also involved in Hinode, SDO and STEREO), and be part of
the IRIS team (see iris.lmsal.com for details). The work will involve a
combination or subset of: analysis of IRIS data especially in
combination with data from SDO or Hinode, calculation of non-LTE
diagnostics from advanced numerical radiative MHD simulations of the
solar atmosphere, and comparison between observations and numerical
simulations. The candidate is also expected to assist in planning of
IRIS science operations. Candidates should have a PhD (or expect to
complete a PhD in the next 3 months) in solar physics, plasma physics or
a closely related field. The applicant is expected to have experience in
data analysis of solar data, and/or theoretical or numerical modeling.
The initial position is for a 1 year period and will start as soon as
possible after September 18, 2015. The postdoctoral researcher will be
employed by the Bay Area Environmental Research Institute. The salary
range is $70 to $80K. The job benefits include medical, dental, vision,
life, short-term and long-term disability insurance, a 403b defined
contribution plan for which employer contributes 10% of gross salary,
eligibility for participation in optional 403b tax-deferred annuity
plan, 10 paid holidays, and a total of 3 weeks of vacation per year
through accrual of 10 hours of vacation and 8 hours of sick-time per
month.
Closing date for applications is 18 September, 2015. Submit resumes, a
1-2 page research statement and 2 references to: The Bay Area
Environmental Research Institute at: [log in to unmask] Attention:
Dr. Bart De Pontieu Lockheed Martin Solar & Astrophysics Lab, 3251
Hanover St., Org. A021S, Bldg. 252, Palo Alto, CA 94304 [log in to unmask]
Phone 1-650-424-3094 / Fax 1-650-424-3994
More information can be found at: www.baeri.org
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NASA Headquarters Heliophysics Visiting Scientist
August 6, 2015, from Jeffrey Newmark
NASA’s Science Mission Directorate (SMD) seeks one or more experienced
scientists to fill visiting scientist positions within the Heliophysics
Division at NASA Headquarters in Washington, DC. These are typically
two-year positions, with possible extensions, filled by scientists who
take leave from their home institution.
NASA’s Heliophysics Division implements flight missions and sponsors
scientific research, both with the aim to understand, individually and
as a system, the Sun, heliosphere, and space environments of the Earth
and other planets, including space weather. Visiting scientists should
have a broad understanding of the system science nature of Heliophysics,
as well as one or more of the sub-disciplines. At this time there is
particular interest in expertise related to the heliosphere,
magnetosphere, and/or ionosphere/thermosphere/mesosphere, especially
coupling between the Sun-Earth-heliosphere as they form an
interconnected system.
Visiting scientists participate in the management of the Heliophysics
grants (ROSES) programs, the planning, development, and management of
NASA missions, and long-range strategic planning. They serve as
Discipline Scientists to develop research solicitations, conduct
scientific peer reviews, and develop budgets and program plans for the
recommendation of highly rated proposals. Visiting scientists serve as
Program Scientists for NASA space missions, interacting with the science
working groups and ensuring success of the missions. They play a
leadership role in long-range strategic plans to define the future NASA
heliophysics program. Visiting scientists are expected to demonstrate a
high degree of initiative in the execution of the overall SMD science
mission.
Applicants must have a Ph.D. or equivalent in heliophysics or related
discipline, plus relevant experience in instrumental, observational, or
theoretical research. They should be familiar with NASA grants programs,
and be able to communicate effectively with the scientific community,
educators, and the media. There are two pathways, IPA agreements and
Details. Visiting scientists that are funded via an Intergovernmental
Personnel Act (IPA) agreement with their home institution require
current employment with a US institution for at least 90 days prior to
starting at NASA. Visiting scientist detailees are civil servants
employed at a NASA center or another branch of the Federal Government.
Only US citizens and Legal Permanent Residents are eligible to apply.
Positions are available beginning in October 2015, though the starting
date is negotiable. Interested scientists should send a curriculum vitae
and cover letter by September 11, 2015 to Aaluk Edwardson
([log in to unmask]). Please contact Jeffrey Newmark at
202-358-0684 or [log in to unmask] for answers to questions.
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Solar Orbiter Instrument Operations Scientist
August 5, 2015, from Daniel Mueller
Vacancy notice – Solar Orbiter Instrument Operations Scientist in ESA’s
Directorate of Science and Robotic Exploration:
www.esa.int/hr/PDF/ESA-VN-ESAC-2014-002-COR-1-REV-1.pdf
The postholder’s initial assignment is to support the development and
help with the definition of the science operations and data products for
the Solar Orbiter mission, as part of the Solar Orbiter Science
Operations Centre (SOC). The SOC’s tasks include science operations
planning, instrument handling, science data processing and archiving.
This is the third of three Instrument Operations Scientists positions,
and its particular focus will be on the SPICE imaging spectrometer.
Please note: The application deadline for this vacancy is on 27 August 2015.
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Please see:
http://solarnews.nso.edu/current.html
for the latest SPD Newsletter.
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UKSP NEWSLETTER ENDS
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