The work will exploit the Group’s involvement in current space missions, including Cassini, Cluster, Rosetta, Stereo, Themis, and Venus Express together with future missions (e.g., NASA’s MMS or the CINEMA/TRIO CubeSat mission).

Our preferred method of application is online via our website http://www.imperial.ac.uk/employment (please select “Job Search” then enter the vacancy reference number NS2012008RD into “Keywords”). Please complete and upload an application form as directed, also providing a CV and list of publications and the names of three referees.

Should you have any queries about the application process please contact the Space and Atmospheric Physics Group Administration office via space.sec@imperial.ac.uk

Closing date: 22nd February 2012 (midnight GMT)

Dr. Jonathan Eastwood
Research Fellow (STFC Advanced Fellow)
The Blackett Laboratory
Imperial College London
SW7 2AZ, UK
tel +44(0)20 7594 8101
fax +44(0)20 7594 7772
email jonathan.eastwood@imperial.ac.uk
www.imperial.ac.uk/people/jonathan.eastwood

The post (Swarm Mission Support Scientist) is funded through a mission support programme run by the UK National Centre for Earth Observation (NERC) and the position is to work within the Space Science Division of the RAL Space Department at the Rutherford Appleton Laboratory. The appointment will be to the STFC band D salary scale as a 2 year initial contract.

The work will be to provide advice to the mission during operations, and to the science team and user community in order to assess the science data quality and develop multi-spacecraft methodology. The programme of work will include:

1. Calibration and validation of the high-precision multi-spacecraft magnetic field data.
2. Verification of the electric field data via coordination with ground based radar networks.

3. The development and application of algorithms for data combination and (multi-point) analysis.

Regular progress reports during the study, which will be provided to the ESA mission management team, will be required. The work will also require the acquisition of level 1b data from the SWARM data system and the development of analysis techniques designed to validate the data.

The successful applicant should hold a PhD, have working experience in a relevant field and be familiar with standard, computer based data processing techniques. Specifically, experience in using, and assessing the data quality, of multi-spacecraft, space plasma measurements would be an advantage. Knowledge of spacecraft operations and data formats (dissemination) is also desirable, as well as some knowledge in the use of ground, incoherent scatter radar observations.

Please contact Malcolm Dunlop (malcolm.dunlop@stfc.ac.uk) tel: 01235-445427 for further information.

Applications are handled by the RCUK Shared Services Centre; to apply please visit our job board at https://ext.ssc.rcuk.ac.uk and complete an online application form. If you are unable to apply online please contact us on 01793 867003 quoting reference IRC42448.
Closing date for applications: 26 February 2012

To apply on line please go to http://www.ucl.ac.uk/hr/jobs/ and search on Reference Number 1230992. A job description and person specification is available in PDF format.
For queries regarding the application process contact Mrs. E. Daghorn (ead@mssl.ucl.ac.uk).
The closing date for applications is 24 February 2012.
UCL Taking Action for Equality

A civil service position is available in the Heliophysics Science
Division, NASA Goddard Space Flight Center, for a supervisory
astrophysicist to serve as Chief of the Space Weather Laboratory. The
mission of the Space Weather Laboratory is to perform fundamental
research and modeling of the coupled Sun-Earth system, with particular
emphasis on the space weather effects important to NASA and the nation.
The Chief develops and maintains the Laboratory’s strategic vision,
provides supervisory and administrative oversight of civil service
personnel, resources, and tasks, and provides scientific and technical
guidance. The Chief also carries out peer-reviewed scientific research
in Heliophysics, and leads in the development of new missions,
instruments, and theoretical investigations to achieve NASA goals.
Evidence of management experience and leadership in the scientific
community is highly desirable.

This appointment will be at the GS-15 level. U.S. citizenship is
required. Please direct technical inquiries to michael.hesse-1@nasa.gov
(301-286-6418) and procedural inquiries to GSFC-TAO@mail.nasa.gov
(301-286-3691).

TO BE CONSIDERED FOR THIS POSITION, YOU MUST APPLY THROUGH USAJOBS.
Please visit http://usajobs.gov, search for vacancy GS12B0016, and
submit your resume. Note that the closing date is 2/2/2012.

Job description:
http://webapps.qmul.ac.uk/hr/vacancies/spec.php?id=2799
Please ensure you read this document before applying.

Overview: The Astronomy Unit (AU) at Queen Mary University of London has a vacancy for a Postdoctoral Research Assistant to work on the Leverhulme Trust Research Grant entitled “Advanced model of solar radio bursts via plasma kinetic simulation”. The AU’s Space and Solar Plasma Physics group carries out research into the naturally occurring plasmas which pervade the solar system, and beyond. We use state of the art numerical simulation and analysis of data from scientific spacecraft. The group has a broad range of interests, including the Sun, solar corona, solar wind, collisionless shocks, plasma waves and instabilities, reconnection, turbulence and particle acceleration.
The successful applicant will be expected to make significant personal contributions to the development of the advanced, multi-dimensional model of solar radio bursts via plasma kinetic simulation, using the existing code EPOCH — a multi-dimensional, fully electromagnetic, relativistic particle-in-cell code, and analysis of the observational data from The Low-Frequency Array (LOFAR).
Applicants should have, or be about to gain, a PhD in solar/space physics with experience in the use/development of particle-in-cell numerical codes. The post will be located at Queen Mary in London but may require some limited travel to Oxford for LOFAR observational data analysis. Queen Mary is a member of the SEPnet, a consortium of six partner universities, www.sepnet.ac.uk. QMUL’s Astronomy Unit is also LOFAR-UK’s member institution, as well as member of SEPnet-Astro, astro.kent.ac.uk/SEPNET/.
The post is full time and fixed term, available from 1 March 2012 or as soon as possible thereafter until 28 February 2015 (36 months). It is funded by the Leverhulme Trust Research Grant. Starting salary will be in the range £30,500 (year 1), £32,173 (year 2), £33,944 (year 3) per annum inclusive of London Allowance. Benefits include 30 days paid annual leave, defined benefit pension scheme and interest-free season ticket loan.

Candidates must be able to demonstrate their eligibility to work in the UK in accordance with the Immigration, Asylum and Nationality Act 2006. Where required this may include entry clearance or continued leave to remain under the Points Based Immigration Scheme.

Informal enquiries should be addressed to the Leverhulme Grant Principal Investigator, Dr David Tsiklauri by email to d.tsiklauri@qmul.ac.uk or on +44 (0)20 7882 5898. Further details about the AU can be found at astro.qmul.ac.uk

Further details/application form can be found at: www.hr.qmul.ac.uk/vacancies or directly
http://webapps.qmul.ac.uk/hr/vacancies/jobs.php?id=2799

Completed application forms, covering letter, CV (which should include the list of publications) and 3 academic references, quoting 12004/NL, should be returned to the Recruitment Administrator, School of Physics and Astronomy, Queen Mary University of London, Mile End Road, London, E1 4NS, or by e-mail to ph-recruit@qmul.ac.uk

The closing date for applications is 9 March 2012 by which ALL materials, including references, should be received. It is anticipated that interviews will be held during the week of 19 – 23 March 2012.

Valuing Diversity & Committed to Equality

http://webapps.qmul.ac.uk/hr/vacancies/jobs.php?id=2799

Northumbria University (School of Computing, Engineering and Information Sciences)

Dear colleagues,

Northumbria University (at Newcastle) is advertising a permanent academic position in its Mathematics and Statistics division (located in the School of Computing, Engineering and Information Sciences). The candidate must be an excellent applied mathematician, and must have a research profile that strengthens the current profile of the School. As you may know, I have recently been appointed to a similar position at Northumbria, and so “Solar Physics”, “Magnetohydrodynamics” and “Mathematical Modelling of Solar Phenomena” are now all active and valid research areas within the School.

Thus, candidates who can demonstrate that they have the necessary skills in applied mathematics, and are active researchers in Solar Physics/Magnetohydrodynamics are strongly encouraged to apply. This is also a real opportunity to kick start a new Solar Physics research group (i.e. the successful candidate would join Dr James McLaughlin, Dr Gary Verth and our solar PhD students). If you are interested, feel free to phone me (0191-227-3667) or email me ( james.a.mclaughlin@northumbria.ac.uk ) and I can let you know more details.

This is a time of strategic recruitment and expansion at Northumbria University and stems from the new Vice-Chancellor. My permanent position (I started in January 2010) came from this new strategic investment, and likewise this lectureship is from the same investment strategy. The School has also been very good to me: I have been given a 3-year research assistant (Dr Gary Verth) and a PhD studentship (Mr Jonathan Thurgood), so they are really serious about investing in their new academics. Above all, the School is looking for high-quality, motivated researchers who are conducting REF-driven research. If this sounds like you, then I encourage you to apply. However, note the deadline of 31st January 2012 !

Please visit :

http://work4.northumbria.ac.uk/hrvacs/cei1108

for full details, job description, application form, etc.

Closing date: 31 January 2012

http://work4.northumbria.ac.uk/hrvacs/cei1108

The first fellowship, on the Chemistry of Planetary Atmospheres, will have two research aims: to study the layers of metallic ions observed in planetary atmospheres, by measuring the rates of dissociative recombination of metallic molecular ions with electrons; and to develop a novel reactor for simulating meteoric ablation in the laboratory.

The second fellowship, on the Chemistry of the Upper Atmosphere, will investigate the chemistry of the metallic layers in the mesosphere, the formation of meteoric smoke, and the nucleation of noctilucent clouds, using a reactor employing laser photo-ionization and time-of-flight mass spectrometry.

Suitable applicants for these positions should have a PhD in experimental physical/atmospheric chemistry, chemical physics, or a closely related discipline. You should be prepared to work as part of a dynamic team and, when appropriate, to use your initiative as an independent researcher.

Both positions are 54-month appointments, available from 1 April 2012. Salary in the range £29,972 – £35,788 depending on experience.

Further information on CODITA and Atmospheric Chemistry at the University of Leeds is available at http://www.leeds.ac.uk/hr/jobs/index.htm.

Informal enquiries to Professor John Plane, email j.m.c.plane@leeds.ac.uk, http://www1.chem.leeds.ac.uk/JMCP/, tel +44 (0)113 343 8044.

Closing Date: 23 January 2012

The full‐time post is for a three‐year period with the possibility of renewal for a further three years. The Director is based at the EISCAT Headquarters in Kiruna, Sweden. However a
considerable amount of international travel should be expected.

Applications should include a resume and a one page statement of the applicant’s vision for EISCAT and should be sent by email to: Director2013@eiscat.se, latest 17:00 (CET) on Wednesday 15 February 2012. Applications will be treated confidentially. Employment terms and conditions will be subject to negotiation with the board of EISCAT, the Council. For more information about the position, please contact the current Director, Dr. Esa Turunen (Esa.Turunen.@eiscat.se) or the Chairperson of Council, Dr. Tomas Andersson (tomas.andersson@vr.se).

Two three-year appointments within the Geomagnetism group of the British Geological Survey,
based in Edinburgh, are now available.

These posts are concerned mainly with research into the internal magnetic field of the Earth, but
one has an external field (space science) aspect to it too. We’re keen to attract enthusiastic, self-
motivated research scientists, with an interest in both pure research and in real-world applications
of geomagnetism science.

Further details may be found at http://www.bgs.ac.uk/news/vacancies.html

Closing date for applications is 27th January 2012.

Post 1: Global Geomagnetic Field Modeller
The post holder will carry out research leading to improved scientific modelling and understanding
of global geomagnetic fields. They will apply the results of that research to improve the products
and services provided by BGS geomagnetism to the oil industry consortium that supports the BGS
Global Geomagnetic Model, the defence industry that supports the World Magnetic Model and
the academic community that uses global magnetic field models. In addition the successful
candidate will maintain and enhance the scientific reputation of BGS geomagnetism by publishing
scientific advances in geomagnetic field modelling and by developing and maintaining links with
other leading research groups in geomagnetism.

Post 2: Geomagnetic Field Researcher
The successful candidate will support BGS research and will investigate the application of potential
field methods to estimate local crustal magnetic field vector anomalies at depth from magnetic
total intensity surveys, in order to improve the magnetic directional referencing services BGS
provides to the oil industry. In addition the post holder will investigate methods to estimate the
time varying ionospheric and magnetospheric magnetic fields and to apply the results of that
research to improve the magnetic directional referencing services BGS provides to the oil industry.
The post holder will also improve the confidence in quoted uncertainties associated with model
estimates of the local crustal and time-varying external magnetic fields and contribute to
geomagnetism team response to oil industry customers.

Enquiries to Dr Alan Thomson (awpt@bgs.ac.uk)

The Fellowship is for a period of two years with a possibility of extension for one more year. Candidates
should be ordinarily below the age of 32 years. The monthly stipend is Rs. 50,000/- to Rs. 55,000/- for
candidates with up to 2 years post-doctoral experience and Rs.55,000/- to 60,000/- for those with more
than 2 years experience. Chandrashekhar Fellows would be entitled to an annual contingency grant of
Rs.200,000/-, as well as to housing, medical and other benefits in accordance with the rules of the
institute. Travel support by economy air fare will be available at the time of taking up the assignment.
Chandrasekhar Fellows may choose their own research topics or collaborate with groups or individuals in the Institute.

Application may be submitted any time of the year by e-mail to: pdf_chandra@iiap.res.in along with a curriculum vitae, list of publications, research proposal and names and addresses of five referees. Processing of the applications takes about three months.

For further details about the Chandrasekhar Fellowships please visit:
http://www.iiap.res.in/postdoc.htm
Details on IIA’s research programs and facilities can be found at http://www.iiap.res.in.

http://www.iiap.res.in/postdoc.htm

=================================================================
Closing Date: Sunday 04 December 2011
Interview Date: Wednesday 21 December 2011
Reference: A321

Applications are invited for a short-term position which has arisen in
the Space Plasma Environment and Radio Science (SPEARS) group at
Lancaster University. The post is fully funded by the UK STFC (Science
and Technology Funding Council) for a period of 10 months.

ACCELERATION AND LOSS PROCESSES AT RELATIVISTIC ENERGIES – Measured
fluxes in the Earth’s radiation belts fluctuate rapidly over many orders
of magnitude. Although the radiation belt response is known to be
correlated with solar wind parameters, the complex interplay between the
various source and loss processes within the belts is not understood in
detail.

You will work on study of the Earth’s radiation belts, source and loss
processes within the belts, and the underlying physical mechanisms
responsible. In particular, it is envisaged that the project will
address if and how relativistic radiation belt particles may be
precipitated into the upper atmosphere, and possible subsequent effects.

You should hold (or shortly expect to be awarded) a Ph.D. in a relevant
field. Previous experience in the above areas will be an advantage.
Salary will be pro-rata within the range £25101-£29099 per year
depending on previous experience.

Lancaster University is an equal opportunity employer. You may find some
helpful information on local amenities here:
http://www.lancs.ac.uk/depts/physics/jobs/amenities/.

Please contact Mick Denton (m.denton@lancaster.ac.uk: +44 (0)1524
510544) for further details.

=================================================================

Further details can be found at the link below:

http://hr-jobs.lancs.ac.uk/Vacancy.aspx?ref=A321

Regards,

Mick

The University of Central Lancashire invites applications for the full professorial post of Director of the Jeremiah Horrocks Institute, based in Preston, UK.

The JHI Institute (http://www.star.uclan.ac.uk) includes around 40 staff and research students in Astrophysics, Solar Physics and related research areas, and achieved internationally excellent and world leading ratings in the UK’s 2008 Research Assessment Exercise.

The JHI is a partner in the Southern African Large Telescope and in the COSMOS HPC project, holds core membership in the Herschel-ATLAS and GAMA survey teams, and hosts the UK data hub for Solar Dynamics Observatory. The University has a Space Act Agreement with NASA that is unique amongst UK Universities.

JHI staff are involved in collaborations active on every continent on Earth. Research interests include: solar and solar-terrestrial physics; stellar and interstellar physics including asteroseismology, evolved stars and pre-stellar objects; galaxy formation and evolution, extragalactic jets and large-scale structure.

The JHI Director reports to the Dean of the School of Computing, Engineering and Physical Sciences, which also hosts teaching in Physics and Astronomy including a highly successful Astronomy distance learning programme (www.studyastronomy.com) attracting around 400 students internationally each year and providing the only BSc(Hons) Astronomy programme by distance learning. Many JHI staff also teach on the School’s Mathematics programme. There are existing and developing synergies with other aspects of physics, mathematics, engineering, computing, nuclear and energy disciplines within the School.

The appointee will be a world-class researcher with excellent leadership abilities, and be responsible for driving an increase in the fraction of JHI research judged to be world leading and internationally excellent. In addition the appointee will work closely with the School Executive Team and Professoriate, and the University Director of Research, to develop inter-disciplinary links including support for activities around teaching and knowledge transfer. Key to the role is leading and further developing the supportive environment for staff and students to enable them to perform to the best of their abilities.

It is envisaged that the appointee would take up a professorial role at the University prior to the current Director retiring in 2012/13, to enable a managed transition into the role. This is a professorial appointment: candidates should meet all the essential criteria on the person specification and the specific professorial criteria as described via the Further Information link at http://www.uclan.ac.uk/information/services/work/191A-22-07.php

The JHI is located on UCLan’s main campus, on a pleasant site near the centre of the city of Preston, which has a rich history dating back over 800 years. Immediately outside the city is the Forest of Bowland Area of Outstanding Natural Beauty, whilst three National Parks (Lake District, Peak District, Yorkshire Dales) are each only an hour away. Preston has excellent communications by rail and motorway with the rest of the country: London, Edinburgh and Glasgow are all less than 2.5 hours away by direct train. The city has many parks and green spaces for outdoor activities, a plethora of pubs and clubs and a vibrant city centre only a few minutes’ walk from the university. There are numerous cultural events, both in Preston itself (e.g. during 2012 with the unique once-every-20-yrs Preston Guild celebrations which have run since the 12th Century) and in nearby cities such as Manchester and Liverpool. Preston is also the European City of Sport for 2012.

Informal enquires regarding this post may be addressed to Robert Walsh, Director of Research rwwalsh@uclan.ac.uk
or Robert Wallace, Dean, rrwallace@uclan.ac.uk

Further Information:
http://www.uclan.ac.uk/information/services/work/191A-22-07.php

Full-time indefinite-term management contract. Reference: 191A-22-07

Closing Date: Wednesday 30th November 2011 at 17:15 UT.

Interviews will be held in Preston in mid-late January.

How to apply: http://www.uclan.ac.uk/information/services/work/apply.php

The National Astronomical Observatory of Japan (NAOJ) invites applications for postdoctoral positions starting from Japanese FY2012 (commencing between April 2012 and September 2012). The Hinode Science Center, NAOJ currently holds one vacant position for the solar physics postdoctoral fellow, and would like to encourage young solar physicists to apply for the position. The contract is essentially for three years with yearly review on research performance. The successful applicant is conducting their own research in observational data analysis, theory/simulation, or experimental solar physics. It is desirable that the research topics are connected to our ongoing and future projects such as Hinode http://hinode.nao.ac.jp/index_e.shtml, CLASP http://hinode.nao.ac.jp/CLASP/, and SOLAR-C http://hinode.nao.ac.jp/SOLAR-C/index_e.html. To complete application, please send your i) CV including a list of publications (refereed and non-refereed articles are to be listed separately), ii) a statement of your research accomplishment, iii) a statement of research plan, iv) copies of up to three papers and iv) letters of reference (not compulsory but strongly advised) to the address below. The deadline for applications is November 30, 2011. The email applications are not accepted. If you have any query, please contact Prof. Saku Tsuneta (email: saku.tsuneta@nao.ac.jp, phone: +81-422-34-3720, fax:+81-422-34-3700)

Prof. Saku Tsuneta
Hinode Science Center
National Astronomical Observatory of Japan
2-21-1 Osawa, Mitaka, Tokyo 181-8588
Japan

Please quote ref no: BAS 75/11
Closing date for applications: 31 Oct 2011

The British Antarctic Survey (BAS), part of the Natural Environment Research Council, aims to undertake a world-class programme of scientific research, and to sustain for the UK an active and influential regional presence and a leadership role in Antarctic affairs.

This project aims to identify if solar variability can influence weather and climate through processes other than direct radiation, and specifically through electric potential variations in the Earth’s ionosphere driven by solar wind-magnetosphere-ionosphere interactions. Your main activity will be to apply statistical data analysis techniques to the analysis of ionospheric electric field data from the SuperDARN high-frequency radar network, as well as meteorological data from the polar regions. This will include developing software packages to identify correlations and the investigation of causal mechanisms. You will also engage in publishing scientific papers and presenting results at international meetings.

With a PhD in physics or mathematics or equivalent postgraduate experience, you will have an interest in space and atmospheric science and experience of software development in a compiled language, preferably for the analysis of experimental data. Effective in working on your own initiative and in collaboration with others, you will also be able to manage resources to meet agreed objectives and deadlines. Experience of working in ionospheric or atmospheric science, of statistical analysis of large data sets, or of analysis of SuperDARN high-frequency radar data would be an advantage.

Qualifications: PhD in physics or mathematics, or equivalent post-graduate experience in these subjects.

Duration: 3 year fixed term appointment

Salary: Salary will be in the range of £26,180 to £29,410 per annum. We offer a generous benefits package including a defined salary pension scheme, free car parking, flexible working hours and 30 days annual leave.

On-line application forms and further information are available on our website at www.antarctica.ac.uk/employment

These are also available from the Human Resources Section, British Antarctic Survey, High Cross, Madingley Road, Cambridge, CB3 0ET. Tel: (01223) 221508.

Please quote reference: BAS 75/11
Closing date for receipt of application forms is 31st October 2011
Interviews are scheduled to be held w/c 21st November 2011

We welcome applications from all sections of the community. People from ethnic minorities are currently under-represented and their applications are particularly welcome.

the 2012 round of the Australian Research Council Future Fellowships was announced several days ago, ahead of expectations. I am writing to ask you to consider applying, if you obtained your PhD between 30 November 1996 and 30 November 2006 inclusive, or to encourage any suitable high quality researchers you know who fall within this category to apply through the School of Mathematical Sciences at Monash University. The commencement date for successful applicants will normally be 1 July 2012.

The School of Mathematical Sciences maintains interests in many areas of pure and applied mathematics and statistics, as well as astrophysics, atmospheric science, and geoscience (see http://www.maths.monash.edu.au/ about the School of Mathematical Sciences, and http://moca.monash.edu/ about the Monash Centre for Astrophysics, which is joint between the Schools of Mathematical Science and the School of Physics).

The prestigious Future Fellowships are 4-year full-time research awards offered at three levels; 1 (senior lecturer level), 2 (associate prof), and 3 (professor). Full details of the scheme (including funding rules) are available at http://www.arc.gov.au/ncgp/futurefel/future_default.htm.

For Future Fellowships commencing in 2010 the national success rates were 32.3% for Level 1; 22.9% for Level 2; and 19.4% for Level 3. Due to the unexpectedly early call for applicants and the short time till submission, success rates may well be greater this time!

Any interested party should send a CV (clearly stating PhD award date) and list of career 10 best publications to Prof Kate Smith-Miles, Head of School, School of Mathematical Sciences (kate.smith-miles@monash.edu) by Friday October 14 at the latest, with a cc to me (paul.cally@monash.edu). If Prof Smith-Miles judges that the application would be competitive and a good fit for the school, an Expression of Interest can be submitted to the Faculty of Science on Monday Oct 17.

Attractive packages may be negotiated in the event of a successful application.

Key Dates (for receipt in Canberra; Monash dates will be earlier)

* Closing time for Eligibility Exemption Requests 5.00 pm (AEDT) 19 October 2011
* Closing time for submission of Proposals 5.00 pm (AEDT) 30 November 2011
* Deadline for Request not to Assess 5.00 pm (AEDT) 30 November 2011

Paul Cally

—–
Prof Paul Cally
Director of Research
School of Mathematical Sciences
Monash University Clayton Victoria, AUSTRALIA 3800
Ph: +61 3 9905-4471 FAX: +61 3 9905-4403

Closing Date: Monday 31st October 2011 at 17:15 GMT. Interviews are expected to be held in early December 2011
How to apply: http://www.uclan.ac.uk/information/services/work/apply.php

The University of Central Lancashire is seeking a successor to Professor Gordon Bromage as Director of the Jeremiah Horrocks Institute, based in Preston, prior to his retirement in 2012/13. The JHI includes around 40 staff and research students in Astrophysics and related research areas, and achieved internationally excellent and world leading ratings in the UK’s 2008 Research Assessment Exercise.

The JHI is a partner in the Southern African Large Telescope and in the COSMOS HPC project, holds core membership in the Herschel-ATLAS and GAMA survey teams, and hosts the UK data hub for Solar Dynamics Observatory. The University has a Space Act Agreement with NASA that is unique amongst UK Universities. JHI staff are involved in collaborations active on every continent on Earth. Research interests include: solar and solar-terrestrial physics; stellar and interstellar physics including asteroseismology, evolved stars and pre-stellar objects; galaxy formation and evolution, extragalactic jets and large-scale structure.

The JHI sits within the School of Computing, Engineering and Physical Sciences, which hosts teaching in Physics and Astronomy including a highly successful Astronomy distance learning programme attracting around 400 students internationally each year and providing the only BSc(Hons) Astronomy programme by distance learning. Many JHI staff also teach on the School’s Mathematics programme. There are existing and developing synergies with other aspects of physics, mathematics, engineering, computing, nuclear and energy disciplines within the School.

The appointee will be a world-class researcher with excellent leadership abilities, and be responsible for driving an increase in the fraction of JHI research judged to be world leading and internationally excellent. In addition the appointee will work closely with the School Executive Team and Professoriate, and the University Director of Research, to develop inter-disciplinary links including support for activities around teaching and knowledge transfer. Key to the role is leading and further developing the supportive environment for staff and students to enable them to perform to the best of their abilities. It is envisaged that the appointee would take up a professorial role at the University prior to the current Director retiring to enable a managed transition into the role. This is a professorial appointment: candidates should meet all the essential criteria on the person specification and the specific professorial criteria as described via the Further Information link at http://www.uclan.ac.uk/information/services/work/191A-22-07.php .

Informal enquires regarding this post may be addressed to Robert Walsh, University Director of Research rwwalsh@uclan.ac.uk or Robert Wallace, Dean of School rrwallace@uclan.ac.uk .

The successful candidate will work on a project within the Solar Group in ARC involving the analysis and interpretation of high spatial and temporal resolution observations of the Sun’s atmosphere. This Group makes extensive use of a wide range of solar and astronomical satellites and ground-based telescopes, with current activities focused on the observations and modelling of oscillatory phenomena and impulsive events in the solar atmosphere. In particular, we constructed the Rapid Oscillations in the Solar Atmosphere (ROSA) imaging system that can observe the solar atmosphere in as many as 6 wavelengths simultaneously, and with a cadence of up to 200 Hz. ROSA is currently at the National Solar Observatory in New Mexico USA. The Group makes extensive use of image reconstruction techniques for the analysis of ground-based solar observations from ROSA and other instruments.

Applicants must have a PhD in the physics of the solar atmosphere either awarded or submitted by the time of taking up the post. Experience is essential in the reduction, analysis and interpretation of observations of the solar atmosphere from satellite-borne or ground-based instruments. Also essential are experience with the IDL computing environment, and a number of high quality refereed publications commensurate with stage of career.

An application pack for the post, containing further details and guidelines on how to submit your application online, is available at:

http://www.qub.ac.uk/sites/QUBJobVacancies/ResearchJobs/

under post reference 11/101783.

Informal enquiries may be directed to Prof Mihalis Mathioudakis (email: m.mathioudakis@qub.ac.uk).

Salary: £29,972 – £34,745 per annum.

Closing date: 4.00 pm, Friday 4th November 2011

http://www.qub.ac.uk/sites/QUBJobVacancies/OtherJobs/ResearchJobs/

PhD Position(s) in Solar/Stellar Astrophysics.

The position(s) may be filled as early as mid November 2011 (the start date is negociable). The salary is 50% of pay grade TV-L 13 of the German civil service, which is sufficient to cover accommodation and living expenses.

The successful candidate(s) will work in the research group “Physics of the Interior of the Sun and Sun-like Stars”. A variety of observational and/or theoretical projects are available:

- Analysis of solar oscillations (SDO space mission)
- Analysis of stellar oscillations (CoRoT and Kepler space missions)
- Models of the Sun and Sun-like stars
- 3D tomography of the solar interior
- Inversions for stellar structure and rotation
- Numerical simulations of seismic waves
- Characterization of planet-host stars (Kepler mission and PLATO project).

The successful candidate(s) will have to meet the formal requirements for admission in the PhD program of the Faculty of Physics, including evidence of a Master’s degree in physics or related disciplines. A background in astrophysics is desirable. An excellent command of the English language is required.

The Faculty of Physics is one of great distinction with a rich history of outstanding research. The University of Goettingen has been rated “excellent” together with only eight other universities in Germany (Exzellenz-Initiative). Together with five Max Planck Institutes, the German Aerospace Center, and other research institutions, the University of Goettingen is a cornerstone of the Goettingen Research Campus, a world-renowned collaboration for innovative research.

The University of Goettingen is an equal opportunities employer and places particular emphasis on providing career opportunities for women. Qualified women are therefore strongly encouraged to apply. At equivalent levels of qualification and experience, persons with disabilities will have preference.

The application should include a full CV, a transcript of your BSc and MSc examinations, and the contact details of three references. The cover letter should state that you apply for a PhD position. Please send your application via post by 22 October 2011 to Klaudia Wolters, Georg-August-Universitaet Goettingen, Institut für Astrophysik, Friedrich-Hund-Platz 1, 37077 Goettingen, Germany and send a copy in electronic form (single PDF file) to sekr@astro.physik.uni-goettingen.de with “IAG-Gizon-4” in the subject line.

If you have any questions, please contact Prof. Laurent Gizon at +49 (0)551 39-5058 or gizon@astro.physik.uni-goettingen.de.

We request that you mail a paper copy of your application. We will destroy the documents after a period of five months. Application documents will only be returned to you if you provide a stamped, self-addressed envelope.

Postdoctoral Position in Solar/Stellar Astrophysics.

This position may be filled as early as mid November 2011. The position is full time (39.8 hours per week) with an initial contract of three years (an extension is possible). The salary will be in the range of pay grade TV-L 13 of the German civil service.

The successful candidate will work in the research group “Physics of the Interior of the Sun and Sun-like Stars”. Various research projects are available is stellar or solar physics, modeling or data analysis. For example, a possible topic of research is the development of consistent models of exoplanets and their host stars using asteroseismology.

In addition to research, duties will include teaching and assistance during examinations.

The successful candidate must hold a PhD in physics, astrophysics, or a related discipline. An excellent command of the English language is required.

The University of Goettingen is an equal opportunities employer and places particular emphasis on providing career opportunities for women. Qualified women are therefore strongly encouraged to apply. At equivalent levels of qualification and experience, persons with disabilities will have preference.

The application should include a full CV, a short description of achievements and interests, and the contact details of three references. The cover letter should state that you apply for postdoctoral position “IAG-Gizon-2”. Please send your application via post by 22 October 2011 to Klaudia Wolters, Georg-August-Universitaet Goettingen, Institut für Astrophysik, Friedrich-Hund-Platz 1, 37077 Goettingen, Germany and send a copy in electronic form (single PDF file) to sekr@astro.physik.uni-goettingen.de with “IAG-Gizon-2” in the subject line.

If you have any questions, please contact Prof. Laurent Gizon at +49 (0)551 39-5058 or gizon@astro.physik.uni-goettingen.de.

We request that you mail a paper copy of your application. We will destroy the documents after a period of five months. Application documents will only be returned to you if you provide a stamped, self-addressed envelope.

Centre for Fusion, Space & Astrophysics, Physics Department, University of Warwick, UK

At the Centre for Fusion, Space & Astrophysics (University of Warwick, UK) we seek candidates for an opening of an STFC-funded postdoctoral vacancy to work on the theoretical and observational study of MHD waves and oscillations in the solar corona. The project comprises of the analysis of data obtained with space-borne telescopes including SDO, Hinode, STEREO and RHESSI, and future missions, and ground-based observational facilities, and analytical and numerical modelling of these phenomena, including high-performance MHD and plasma simulations, and plasma diagnostics. The appointed PDRA will work with Prof V.M. Nakariakov, Prof T.D. Arber and Dr E. Verwichte, and other members of CFSA. The initial contract will be for two years.

You will have, or will expect to attain, a PhD in a relevant discipline.

Informal enquiries may be addressed to Professor V.M. Nakariakov (V.Nakariakov@warwick.ac.uk)
Further details may be found on http://www2.warwick.ac.uk/fac/sci/physics/research/cfsa/pdrawaves

Please quote job vacancy reference number 53241-091.

The closing date for applications is 14 October 2011.

The university values diversity.

http://www2.warwick.ac.uk/fac/sci/physics/research/cfsa/pdrawaves/

http://ig29.i-grasp.com/fe/tpl_universityofleeds01.asp?newms=jj&id=73874&aid=13870

The closing date is 28 Sept.

http://ig29.i-grasp.com/fe/tpl_universityofleeds01.asp?newms=jj&id=73874&aid=13870

The following 2012 Fellowship Programs are now accepting applications online:

CFA POSTDOCTORAL FELLOWSHIP PROGRAM
http://www.cfa.harvard.edu/postdoc/
Deadline: October 31, 2011

CLAY POSTDOCTORAL FELLOWSHIP PROGRAM
http://www.cfa.harvard.edu/clay/
Deadline: October 31, 2011

Information and instructions can be found at the links above.

Best regards,

Christine

_____________________________________
Christine Crowley, Coordinator
Fellowship Program
Smithsonian Astrophysical Observatory
Harvard-Smithsonian Center for Astrophysics
60 Garden Street, MS 67
Cambridge, MA 02138
Tel: 617-495-7103
Fax: 617-496-7589
Email: ccrowley@cfa.harvard.edu
_____________________________________

Postdoctoral Position in Solar/Stellar Astrophysics.

This position may be filled as early as mid October 2011. The position is full time (39.8 hours per week) with an initial contract of three years (an extension is possible). The salary will be in the range of pay grade TV-L 13 of the German civil service.

The successful candidate will develop and compute stellar evolutionary models for applications in asteroseismology, within the research group “Physics of the Interior of the Sun and Sun-like Stars”.

In addition to research, duties will include teaching and assistance during examinations.

The successful candidate must hold a PhD in physics or astrophysics. Past experience in stellar modeling is highly desirable. A background in solar/stellar physics or helio-/asteroseismology is required. An excellent command of the English language is mandatory.

The University of Göttingen is an equal opportunities employer and places particular emphasis on providing career opportunities for women. Qualified women are therefore strongly encouraged to apply. At equivalent levels of qualification and experience, persons with disabilities will have preference.

The application should include a full CV, a ten line description of past research achievements, and the contact details of three references. The cover letter should state that you apply for postdoctoral position “IAG-Gizon-1”. Please send your application via post by 22 September 2011 to Klaudia Wolters, Georg-August-Universität Göttingen, Institut für Astrophysik, Friedrich-Hund-Platz 1, 37077 Göttingen, Germany and send a copy in electronic form (single PDF file) to sekr@astro.physik.uni-goettingen.de with “IAG-Gizon-1” in the subject line.

If you have any questions, please contact Prof. Laurent Gizon at +49 (0)551 39-5058 or gizon@astro.physik.uni-goettingen.de.

We request that you mail a paper copy of your application. We will destroy the documents after a period of five months. Application documents will only be returned to you if you provide a stamped, self-addressed envelope.

Please quote ref no: BAS 46/11a
Closing date for applications: 08 Sep 2011

Main Description

The British Antarctic Survey (BAS) seeks a research scientist to work on electron acceleration in the radiation belts of the Earth, Jupiter and Saturn. The project is to to test the hypothesis that cyclotron resonant wave-particle interactions are a major process for electron acceleration at Earth, Jupiter and Saturn, and plays a major role in the formation of the radiation belts at these planets. The project will require development and adaptation of the BAS global dynamic global radiation belt model from Earth to Jupiter and Saturn, using implicit finite difference methods. It will also require the acquisition of satellite data from CLUSTER at Earth, Galileo at Jupiter, and Cassini at Saturn through existing collaborations. Satellite data will be processed to provide input to the model and the results compared to satellite data and results in peer reviewed literature. The successful candidate will be expected to disseminate results via peer reviewed papers and by giving presentations at conferences and meetings.

The post requires a number of essential requirements, including a 1st or upper second degree in physics, maths or equivalent, three years relevant experience in space (including Astronomy) or plasma physics, or a suitable area of applied maths. The post also requires relevant experience developing numerical methods to solve equations and experience writing a substantial amount of computer code in a high level programming language such as FORTRAN. The candidate must be able to work as part of a small team and must be able to speak and write English fluently. Desirable but not essential requirements include a PhD in space or plasma physics, peer reviewed publications, a background in the radiation belts, experience solving partial differential equations using finite difference methods, and programming in IDL computer language.

The post is based in Cambridge and does not involve Antarctic duties. It is a fixed term appointment for three years with a negotiable starting date October 2011.

Qualifications: 1st or upper second degree in Physics, maths or equivalent and three years relevant experience

Duration: 3-year fixed term appointment

Salary: Salary will be in the range of £26,180 to £29,410 per annum. We offer a generous benefits package including a defined salary pension scheme, free car parking, flexible working hours and 30 days annual leave.

On-line application forms and further information are available on our website at www.antarctica.ac.uk/employment

These are also available from the Human Resources Section, British Antarctic Survey, High Cross, Madingley Road, Cambridge, CB3 0ET. Tel: (01223) 221508.

Please quote reference: BAS 46/11a
Closing date for receipt of application forms is 8th September 2011
Interviews are scheduled to be confirmed

The British Antarctic Survey is part of the Natural Environment Research Council and aims to undertake a world-class programme of scientific research, and to sustain for the UK an active and influential regional presence and a leadership role in Antarctic affairs.

UCL’s Mullard Space Science Laboratory is seeking a postdoctoral scientist to undertake research in the area of solar physics, principally through analysis of Hinode and related datasets. MSSL is the UK’s largest university based space science research institution and is involved in many leading research missions (http://www.mssl.ucl.ac.uk).

The post holder will be expected to work with the Hinode, STEREO and SDO datasets, as well as with other space and ground-based datasets for context, and to work effectively as a member of the Solar Physics group. Future potential missions and observatories such as Solar Orbiter, KuaFu, Solar C and EST will build on the new science being pioneered by Hinode, STEREO and SDO and, in preparation for these, the successful applicant will also be expected to participate in scientific studies defining prospective MSSL involvement in them.

The post is available for a period of 18 months in the first instance from 1 September 2011. Salary will be in the range £29099 – £30870, dependent on experience.

To view Job and Person Specifications go to:
http://www.mssl.ucl.ac.uk/jobs/vacancies/vacancy_ref1105.htm

To apply please go to: http://www.ucl.ac.uk/hr/vacancies/adverts/job-list.html
Job Ref. 1199766

Problems with applying for this post please contact Mrs. Libby Daghorn (ead@mssl.ucl.ac.uk).

For further information contact Dr. Sarah Matthews (sam@mssl.ucl.ac.uk).

Closing Date 19th August 2011.

Please note that further details are available from the vacancies webpage at the University of St Andrews. See

https://www.vacancies.st-andrews.ac.uk/welcome.aspx

and look for the reference

Research Assistant – ML1018

https://www.vacancies.st-andrews.ac.uk/welcome.aspx

Research Assistant- £26,629 pa
Research Fellow- £27,428- £35,788 pa

Fixed Term Contract for 2 Years with possibility of extension from 9 January 2012

This STFC funded project centres on the understanding of turbulence in solar system plasmas such as the solar wind by means of mathematical modelling, large scale simulation, and analysis of in-situ spacecraft data.

For details see:

http://www2.warwick.ac.uk/fac/sci/physics/research/cfsa/turbulencepdra

Prof S. C. Chapman,
CFSA, Physics,
Univ. Of Warwick, UK
www.warwick.ac.uk/go/cfsa

Ref: SEN00207
A research associate is required for an ongoing project studying planetary magnetospheres, in particular focusing on a comparative approach. The specific aim is towards a better understanding of the global magnetosphere and dynamics, and the generation of auroral emissions at multiple wavelengths. This research involves the analysis of spacecraft data from multiple instruments, where applicable in the framework of theoretical modelling, in order to study the processes which connect the solar wind-magnetosphere-ionosphere (or surface) in the outer environments of the planets. You will work closely with Dr. Emma Bunce, and other members of the Leicester team using (for example) Cassini data at Saturn, revisiting Galileo data at Jupiter and the more recent Messenger data at Mercury. Possibilities exist for the development of new research areas, for example in the area of moon-magnetosphere interactions.

See the University website – http://www2.le.ac.uk/offices/jobs/opportunities/jobsearch

DEADLINE for applications: midnight Wed 17th August
Please direct informal enquiries to Emma Bunce (emma.bunce@ion.le.ac.uk)

Helioseismology

Physics of solar flares and CMEs

Coronal and chromospheric structure and heating, including coronal seismology

Automated solar feature recognition and tracking, including space weather prediction

Stellar seismology

Candidates are expected to have a PhD in solar physics or a closely related subject, or expect to obtain one shortly. The earliest start date will be September 2011. Applications should consist of a 3-page CV (including names and contact details of 3 references, one of whom should be your current supervisor), a 1-page research plan including identifying an area (or areas) of study at NMSU, and a list of refereed publications. All applications submitted before August 1 will be assured of equal assessment and both positions will remain open until filled.

Interested applicants should contact James McAteer and/or Jason Jackiewicz at solar “at” astronomy “dot” nmsu “dot” edu for further details and submit their application to the same address.

NMSU is an equal-opportunity employer and encourages applications from underrepresented minorities and female scientists.

http://astronomy.nmsu.edu/solar/index.html

Energy and matter emerge from the Sun and flow through our heliosphere,
interacting with planetary atmospheres and surfaces, powering many of the
processes which shape our world and define the planetary environment we
live in. The Solar System Physics Group, part of the Institute of Maths
and Physics (IMAPS) at Aberystwyth, studies this single system from the
development of eruptive features on the Sun, through the evolution and
structure of material in the solar wind, and the impact of this flow on
the environments of the planets. This science exploitation goes hand in
hand with a programme of solar system exploration, and we also research
the robotic and imaging technology for future missions that will
dramatically improve
their science return.

The studentships provide resources to cover university fees plus a
tax-free stipend. Applicants should hold (or expect to achieve) a first or
upper-second class MPhys or BSc honours degree in physics or a related
subject by the summer of 2011. Applicants must also be able to demonstrate
established UK residency (for more information see
http://www.stfc.ac.uk/Funding+and+Grants/12020.aspx#Residence).

For more information please contact the Department at imaps@aber.ac.uk or
the Postgraduate Admissions Office (pg-admissions@aber.ac.uk) as soon as
possible, to make informal enquiries prior to submitting an application.

Aberystwyth University’s online application system and application forms
are available at
http://www.aber.ac.uk/en/postgrad/howtoapply/
Once this formal application is made, suitable candidates will be invited
to visit the institute to learn at first hand of the research activities,
to meet members of staff and to see the facilities available. The closing
date for applications is 30 June 2011, but the process will run throughout
this period, so early application is advised.

For a list of available projects visit
http://www.aber.ac.uk/en/imaps/prospective/postgrad/solarsystemprojects/

We have two one-year STFC funded postdoc positions at Leeds, starting in September 2011, to work on problems in Astrophysical MHD, with me and Steve Tobias.

The link to the position on jobs.ac.uk is:

http://www.jobs.ac.uk/job/ACU439/research-fellows

The closing date is 11 July.

We would be grateful if you could forward this to anyone you know who may be interested.

Regards,
David Hughes

[NOTE: The closing date for applications: noon 17 June 2011]

See http://www.tcd.ie/vacancies/#Lectureships and http://jobs.tcd.ie/ for details.

Summary
The School of Mathematics is seeking to appoint the Hitachi lecturer, to be held in the School of Mathematics, Trinity College Dublin. The candidate is expected to have a Ph.D. in applied mathematics or a similar discipline at the time of application and a strong track-record of research in applied mathematics, particularly in one or more of the areas of numerical analysis, computational algorithm design and high-performance computing and its applications.

Background to the Post. The School of Mathematics has research interests that include large-scale numerical simulations of physical and complex systems. A lecturer is to be appointed to support and develop this research activity and other activities in the scientific domain. The School runs an M.Sc. programme in High-Performance Computing that aims to train graduate students in the application of advanced methods and algorithms to large-scale problems in numerical simulation. The School is a partner in a new Ph.D. programme in “Simulation Science”, hosted by UCD (http://www.ucd.ie/casl/education/educationprogrammes/phdprogrammeinsimulationscience).

There are further details on the TCD School of Mathematics at www.maths.tcd.ie.

—
Peter T Gallagher

They will appear very soon on jobs.ac.uk also.

Energy and matter emerge from the Sun and flow through our heliosphere, interacting with planetary atmospheres and surfaces, powering many of the processes which shape our world and define the planetary environment we live in. The Solar System Physics Group, part of the Institute of Maths and Physics (IMAPS) at Aberystwyth, studies this single system from the development of eruptive features on the Sun, through the evolution and structure of material in the solar wind, and the impact of this flow on the environments of the planets. This science exploitation goes hand in hand with a programme of solar system exploration, and we also research the robotic and imaging technology for future missions that will dramatically improve their science return.

The studentships provide resources to cover university fees plus a tax-free stipend. Applicants should hold (or expect to achieve) a first or upper-second class MPhys or BSc honours degree in physics or a related subject by the summer of 2011. Applicants must also be able to demonstrate established UK residency (for more information see
http://www.stfc.ac.uk/Funding+and+Grants/12020.aspx#Residence).

For more information please contact the Department at imaps@aber.ac.uk or the Postgraduate Admissions Office (pg-admissions@aber.ac.uk) as soon as possible, to make informal enquiries prior to submitting an application.

Aberystwyth University’s online application system and application forms are available at
http://www.aber.ac.uk/en/postgrad/howtoapply/
Once this formal application is made, suitable candidates will be invited to visit the institute to learn at first hand of the research activities, to meet members of staff and to see the facilities available. The closing date for applications is 30 June 2011, but the process will run throughout this period, so early application is advised.

For a list of available projects visit

http://www.aber.ac.uk/en/imaps/prospective/postgrad/solarsystemprojects/

POST-DOCTORAL POSITION IN SPACE PHYSICS

at the Swedish Institute of Space Physics, Uppsala, Sweden
for Research related to Cluster and Ground-Based Data Assimilation Studies,
in the European Cluster Assimilation Technology (ECLAT) Project

Applications are invited for a post-doctoral position for studies of the magnetosphere of
the Earth, its interaction with the solar wind and the upper atmosphere. Our research group
is a major partner in the research team, which is funded by the EU Seventh Framework
Programme (FP7), which aims to create a data archive and portal for solar terrestrial
data-sets to complement the Cluster Active Archive, currently set up by ESA. In this project
we have very close collaboration with Leicester University, UK, the Finnish Meteorological
Institute, the Space Science Group at St. Petersburg State University, Russia, and the
Institute for Space Research in Graz, Austria. Another group at the Swedish Institute of
Space Physics (IRF) in Uppsala is the Principal Investigator Team for the Cluster EFW
instrument. For further information on the full spectrum of research at IRF-Uppsala, see
http://www.irfu.se.

The successful candidate will be involved in extensive international collaboration. Analysis
of data is an important part of the work and it would be an advantage to have experience in
combining advanced data analysis with modelling of solar wind/magnetosphere/ionosphere
interaction, in particular field line-tracing. Interest and experience in coordination of
scientific activities will also be considered an asset. The research group does parallel
work on closely related problems in the realm of the Martian induced magnetosphere, and is
also preparing to use future SWARM satellite data in studies of magnetosphere-ionosphere
interaction. It is expected that the new work on ECLAT will have cross-fertilisation effects
with the other ongoing research.

Candidates should have completed a PhD no earlier than 30 April 2008. However if the
candidate has an older degree and wants to refer to special circumstances, such as parental
leave, this should be clearly stated. The candidate should not currently be an active
researcher at IRF in Uppsala or the Department of Physics and Astronomy at Uppsala
University, Sweden.

The position is available at IRF-Uppsala, located at the Ångström Laboratory in Uppsala,
Sweden, starting immediately or as soon as the present position of the successful candidate
allows. The position is funded by a grant from the European Commission, under FP7, for
three (3) years. After two (2) years as a postdoctoral fellow the candidate will be employed
for one (1) further year as a research scientist.

Closing date is 30 April 2011.

The ECLAT Project at IRF in Uppsala is coordinated by Professor Hermann Opgenoorth
(opg@irfu.se,Tel. +46-18-471 5912).

Applications should include a CV, a short letter stating the applicant’s research interests
and relevant experience, copies of undergraduate and PhD degree certificates, description
and proof of previous post-doctoral positions and/or similar relevant research work
(if available), names and contact information for two professional references and reprints
of not more than four selected publications.

Applications shall be sent to: Registrator, Swedish Institute of Space Physics, Box 812,
SE-981 28 Kiruna, Sweden, www.irf.se, or by email to: registrator@irf.se
(Tel. +46 980 79061).

Reference: Dnr 32-72/11.

POST-DOCTORAL POSITION IN SPACE PHYSICS

at the Swedish Institute of Space Physics, Uppsala, Sweden
for Research related to Mars Aeronomy and the Interaction between the Martian Atmosphere and
the Solar Wind

Applications are invited for a post-doctoral position for studies of the induced
magnetosphere of Mars and its interaction with the solar wind and the atmosphere of the
planet. Our research group is Co-Investigator of the MARSIS topside sounder instrument on
Mars Express, and has close relations with the Principle Investigator group of the ASPERA
particle experiment at the Swedish Institute of Space Physics (IRF) in Kiruna.
Internationally we chair a research network for the study of Mars Upper Atmospheric physics,
which includes research groups from four plasma-related experiments on Mars Express. In our
research we also have close ties to the research groups at Leicester University and the Max
Planck Institute for Solar System research in Lindau-Katlenburg, Germany. For further
information on the full spectrum of research at IRF in Uppsala, see http://www.irfu.se.

The successful candidate will be involved in extensive international collaboration. Analysis
of data is an important part of the work and experience in combining advanced data analysis
with modelling of atmospheric plasma transport is an advantage. Interest and experience in
coordination of scientific activities will also be considered as an asset. The research group
does parallel work on closely-related problems in the solar terrestrial realm, using Cluster
and, in the future, SWARM data. It is expected that the relatively new work on Mars will
have cross-fertilisation effects with the other ongoing work at Earth.

Candidates should have completed a PhD no earlier than 30 April 2008. However if the
candidate has an older degree and wants to refer to special circumstances, such as parental
leave, this should be clearly stated. The candidate should not currently be an active
researcher at IRF in Uppsala or the Department of Physics and Astronomy at Uppsala
University, Sweden.

The position is available at IRF-Uppsala, located at the Ångström Laboratory in Uppsala,
Sweden, starting immediately or as soon as the present position of the successful candidate
allows. The position is funded for two (2) years, with a certain possibility for extension.
The position is funded by a grant from the Swedish National Space Board (SNSB, Rymdstyrelsen).

Closing date is 30 April 2011.

The Mars Express Project at IRF in Uppsala is coordinated by Professor Hermann Opgenoorth
(opg@irfu.se, Tel. +46-18-471 5912).

Applications should include a CV, a short letter stating the applicant’s research interests
and relevant experience, copies of undergraduate and PhD degree certificates, description
and proof of previous post-doctoral positions and/or similar relevant research work
(if available), names and contact information for two professional references and reprints
of not more than four selected publications.

Applications shall be sent to: Registrator, Swedish Institute of Space Physics,
Box 812,SE-981 28 Kiruna, Sweden, www.irf.se, or by email to: registrator@irf.se
(Tel. +46 980 79061).
Reference Dnr 32-73/11.

Senior Lecturer/Lecturer in Applied Mathematics at Northumbria University

Closing date 5th May 2011

http://work4.northumbria.ac.uk/hrvacs/cei1015

Senior Lecturer/Lecturer in Applied Mathematics
School of Computing, Engineering and Information Sciences
Northumbria University
Ref: CEI10/15
Salary: SL: £36,862 – £45,336; L: £31,798 – £35,788

Working within the Mathematics and Statistics Subject Team you will provide expertise in
areas of Applied Mathematics such as Mathematic Modelling and/or Engineering Mathematics to
further enhance the research, teaching and entrepreneurial activities in this area. This
will include designing, developing and delivering high quality teaching activities,
undertaking individual and joint research to produce quality academic outputs and inform
teaching and participating in external activity to generate income and promote the subject.

You must hold a first degree or equivalent in a relevant discipline and have subject
expertise in Applied Mathematics along with specialist knowledge gained through research
activity, professional practice or consultancy. Experience of teaching within an
appropriate field and the potential to undertake research activity which will contribute to
the School’s research submission is also essential. Expertise in teaching MATLAB is
desirable. Candidates being considered for appointment at Senior Lecturer level must be
qualified to Doctoral level.

For an informal discussion about the post, please contact Dr. Colin Creasy on 0191 2274348.

Closing date: 5 May 2011

Application forms can be found at:

http://work4.northumbria.ac.uk/hrvacs/cei1015

If you would like to apply, please send your completed Application Form to
staffcareers@northumbria.ac.uk quoting the reference number.

Northumbria University is an equal opportunities employer and welcomes applications from
all sectors of the community.

Postdoc in high energy solar physics at Glasgow

University of Glasgow
College of Science and Engineering
School of Physics and Astronomy

Postdoctoral Research Assistant/Associate
Ref: E20075
Salary: Grade 6 £25,854 – £29,099 / Grade 7 £31,798 – £35,788 per annum

You will undertake high-quality research in solar physics, in particular the acquisition,
analysis, interpretation and modelling of solar flare hard X-ray data, in collaboration with
members of the Astronomy and Astrophysics Group, and other members of the FP7-funded HESPE
network (i.e. University of Genova, University of Graz, Fachhochschule Nordwestschweiz,
CNRS and University of California, Berkeley).You will also assist in the activities of the
Astronomy and Astrophysics Group as requested by the Investigators and Head of School.

For further information and informal expressions of interest you may also contact Lyndsay
Fletcher (lyndsay.fletcher@glasgow.ac.uk) and Eduard Kontar (eduard.kontar@glasgow.ac.uk)

For further information on the HESPE project, please see
http://www.hespe.eu/

The post is funded until 30 November 2013, with progress reviewed after one year.

Apply online at www.glasgow.ac.uk/jobs

Closing date: 6th May 2011

The University is committed to equality of opportunity in employment.

The University of Glasgow, charity number SC004401.

JAXA International Top Young Fellowship – deadline extended

<http://www.jaxa.jp/employ/index_e.html>

The Japan Aerospace Exploration Agency (JAXA) International Top Young
Fellowship (ITYF) was established as a prestigious new fellowship
programme in 2009. The ITYF is designed to attract outstanding, highly
motivated, early-career researchers in any of the space science fields
covered by the Institute of Space and Astronautical Sciences (ISAS) to
work in Japan for 3 (extendable to 5) years. The deadline for
applications is now 31 May 2011.

New ad for postdoc position at Leeds

There have been problems with the web address that was given for the NERC funded postdoc
position for 3 years to work in Leeds on

‘Rapid dynamics in the Earth’s core’

If you know young researchers who could be interested, the post is now advertised on the
web site

http://www.leeds.ac.uk/hr/jobs/index.htm

with job reference number MAPMA0004, with the closing date extended to May 13th.

Postdoctoral Research Assistant in Space Plasma Physics

Applications are invited for a Postdoctoral Research
Assistant position to work on a project led by Prof.
David Burgess in the Astronomy Unit, Queen Mary University
of London, to study kinetic effects in turbulence and
shocks in space and astrophysical plasmas.

Candidates should have a research background in space
plasma physics, particularly turbulence, with experience
in large-scale numerical kinetic PIC and/or hybrid plasma
simulation methods, and the applications of linear
theory of kinetic plasma waves. Candidates should have
experience with developing parallel simulation codes
in a programming language such as C++. Applicants should
have, or have recently completed a PhD in space plasma
physics (or related area) at the time of commencing
employment.

This is a full-time, fixed term position for a total
period of 1 year 10 months, starting 1st June 2011 or
as soon as possible thereafter. The starting salary
will be in the range of £30,350 – £35,674 per annum,
inclusive of London Allowance.

The full job advert and application procedure can be
found at http://www.maths.qmul.ac.uk/home/vacancies
or http://webapps.qmul.ac.uk/hr/vacancies/jobs.php?id=2313
Informal enquiries should be addressed to Prof. D. Burgess
via email D.Burgess@qmul.ac.uk

The closing date for applications is 5th May 2011, and
interviews will be held during the week commencing 23
May 2011.

Research Assistant – SK7752

Salary: £24,273-£28,983 pa

The Solar and Magnetospheric Theory Group has an opening for a Research Assistant to work in the field of solar physics, focussing on the analysis of observational data. Funded by an STFC Rolling Grant, this project will mainly be in collaboration with Drs I. De Moortel, C. Parnell, D. Mackay and Prof A. Hood. Experience analysing observational data and running observational compaigns is desirable but not essential. You should have recently completed or expect to obtain shortly a PhD in solar physics or a closely related subject.

This post is initially for a term of 1 year. The start date will be 1 April 2011 or as soon as possible thereafter.

Informal enquiries to Dr Ineke De Moortel, Tel: 01334 463757 or email: ineke@mcs.st-and.ac.uk

Interview Date: Mid/Late February

We encourage applicants to apply online, however if you are unable to do this, please call +44 (0)1334 462571 for an application pack.

The University is committed to equality of opportunity.

The University of St Andrews is a charity registered in Scotland (No SC013532).

Research Assistant –SK7751

Salary: £24,273 – £28,983 pa

The Solar and Magnetospheric Theory Group has an opening for a Research Assistant to work in the field of solar MHD modelling. The preferred area would be coronal seismology and/or MHD wave propagation in the solar atmosphere but other areas of solar research will also be considered. Funded by an STFC Rolling Grant, the coronal seismology project will be led by Dr I. De Moortel and Prof B. Roberts, in collaboration with Prof A. Hood and Dr A. Wright. You will mainly use established analytical and numerical methods. Experience with running and analysing large-scale numerical simulations on parallel computers and analysing observational data is desirable. You should have recently completed or expect to obtain shortly a PhD in solar physics or a closely related subject.

This post is initially for a term of 2 years. The start date will be 1 April 2011 or as soon as possible thereafter.

Informal enquiries to Dr Ineke De Moortel, Tel: 01334 463757 or email: ineke@mcs.st-and.ac.uk

Interview Date: Mid/Late February

We encourage applicants to apply online, however if you are unable to do this, please call +44 (0)1334 462571 for an application pack.

The University is committed to equality of opportunity.

The University of St Andrews is a charity registered in Scotland (No SC013532).

Postdoctoral Research Associate in Solar Physics

University of Sheffield
Department of Applied Mathematics

Closing date: Dec 20 2010

Applications are invited for a postdoctoral position in solar physics
in the Solar Physics and Space Plasma Research Centre (SP2RC), in the
Department of Applied Mathematics, University of Sheffield. This post is
is in the area of transport in the Sun and stars, in particular, in the
solar interior.

Candidates must have a PhD or equivalent (or equivalent experience) and
demonstrable experience of research in solar physics, MHD, turbulence,
astrophysics or a related field. The post-holder will possess excellent
theoretical and/or a high standard of computational MHD skills, and
knowledge of IDL is desirable. The post holder will emphasise leadership
of research into MHD turbulence, dynamo theory, magnetic reconnection,
momentum transport, and nonlinear dynamics.

This post is fixed-term with an immediate start date and an end date of 30th
June 2012. Informal enquiries are welcome to Dr Eun-jin Kim
(e.kim@sheffield.ac.uk).

For post details/application pack visit: https://www.shef.ac.uk/jobs/
or email: jobs@sheffield.ac.uk/tel: 0114 222 1631 (24hr)
Please quote Ref. No.UOS002044 in all enquiries.

Post-Doctoral Position at ISSI, Bern, Switzerland

http://www.issibern.ch/spotlight/PostDoc11.pdf

The International Space Science Institute invites applications for a
Post-Doctoral Position for a two-year period starting in February 2011 or by
agreement. The successful candidate shall have received a Ph.D. within the
last five years in a field relating to the Space Sciences in general.
Applications relating to solar physics, solar system science, planetary
science, or to the heliosphere, are particularly welcome.

Lecturer in Mathematics (one-year appointment)

http://www.uclan.ac.uk/information/services/work/264A-17-09.php

The School of Computing, Engineering and Physical Sciences at the University of Central Lancashire has a vacancy for a Lecturer in Mathematics on a one year limited term contract. The School has a healthy Mathematics programme, and research programmes in people-centred computing, computer networking, astrophysics (including solar physics), applied mathematics, computational physics, nuclear technology, tribology and digital signal & image processing.

The role is to teach undergraduate mathematics, supervise undergraduate and postgraduate projects and pursue relevant research, which could relate to any of the School research areas. Ability to teach on the Mathematics programme as currently validated will be essential. A Bachelors degree in Mathematics (or similar subject) and PhD in an appropriate subject are both essential, as is research or industrial experience relevant to the School activities.

Further information on astrophysics research within the School can be found
at www.star.uclan.ac.uk.

Salary: 32,620-37,839.
Closing Date: 15th October 2010 at 4pm

Web Developer for plasma physics at University of Warwick

Job Advert

http://www.warwick.ac.uk/go/cfsa/webdeveloper

The Centre for Fusion, Space and Astrophysics at the University of Warwick is looking for a innovative and self-motivated person to develop and maintain web-based research and educational applications of various aspects of plasma physics, which will be targeted at undergraduate and postgraduate students as well as researchers in the field.

Applicants should hold a Masters Degree or equivalent in Physics or a related discipline. Knowledge of web programming tools such as javascript, applets, etc. is essential. Experience in plasma physics would be advantageous.

Fixed term contract for 2 years
£27,319 – £35,646 pa

Closing Date: Thursday 14 October 2010

For informal enquiries please contact Dr Erwin Verwichte (Erwin.Verwichte@warwick.ac.uk)

For more information, including how to apply, please visit
http://www.warwick.ac.uk/go/cfsa/webdeveloper

Fixed term Research Associate in Helioseismology at the University of Sheffield

Job advert: http://www.shef.ac.uk/jobs/

Job reference number: UOS001635