The Solar System School invites applications for several PhD positions, including projects in asteroseismology, helioseismology and solar physics.
The scientific topics in solar physics/heliophysics and solar and stellar interiors range from the Sun’s interior and subsurface dynamics investigated via global and local helioseismology (Gizon, Duvall, Birch, Schou) to the asteroseismology of solar-like and evolved stars (Hekker), and include among other things the investigations of solar magnetic fields and the multitude of dynamic solar features (Solanki and others).
Deadline: 15 November 2015
Apply online: https://www.mps.mpg.de/phd/applynow
Call for applications 2015 [pdf]
Poster Solar System School [pdf]
Specific applications from candidates with expertise relevant for the thematic line on “Towards a Comprehensive Study of Stars“, including Helio and Asteroseismology are very much welcome and solicited.
This is a very competitive annual call by FCT for postdoc fellowship. Candidates with a highly competitive CV are welcome to submit a pre-application. If you need further details regarding the topics on stars, please contact the thematic line leader Mario Monteiro (email@example.com).
Details can also be found at official announcement by IA.
Deadline: 30th of April 2015.
Job opening for one post-doctoral and one PhD positions in MHD of stellar interiors, tidal interactions in stellar systems, and dynamical stellar evolution in Service d’Astrophysique at CEA Saclay (France) in support of the ERC project SPIRE
We invite applications for one 4-year post-doctoral position and one 3-year PhD position in stellar magnetohydrodynamics, dynamical stellar evolution and ab-initio modelling of tidal interactions in star-planet and multiple star systems in support of the European ERC-CoG project SPIRE (Stars: dynamical Processes driving tidal Interactions, Rotation and Evolution).
The objective of the project is to contribute to interpret new ground breaking high-resolution observations provided by asteroseismology on stellar interiors and their dynamics and planetary system discoveries and characterization (e.g. CoRoT and Kepler and in a near future CHEOPS, TESS, SPIRou, PLATO). To reach this ambitious objective, it is necessary to develop now new frontier theoretical and numerical long-term evolution models of rotating magnetic stars and of their systems. In this framework, the members of the SPIRE project will develop new state-of-the-art equations, prescriptions, and scaling laws that describe coherently dynamical mechanisms that transport angular momentum and drive tidal dissipation in stars using advanced ab-initio semi-analytical modelling and numerical simulations. They will be implemented in the new generation dynamical stellar evolution code STAREVOL and N-body code ESPER to provide realistic integrated and coupled models for the long-term evolution of stars and of their systems, which cannot be directly simulated in 3D yet.
The positions will be held in Service d’Astrophysique (SAp) at CEA-Saclay (France). SAp is a world class astrophysical and space science department with more than 180 faculty and staff members, studying stellar and planetary physics, astrophysical fluid and plasma dynamics, planets and stars formation, high energy astrophysics, galactic and extragalactic astrophysics, cosmology. The PI of the SPIRE project, Dr. S. Mathis, is permanent researcher in the Laboratory of Dynamics of Stars and their Environment. The team hosts recognized experts in stellar systems who carry research at the forefront of their theoretical and numerical modelling and characterization thanks to asteroseismology. CEA possesses large computer facilities and expertise that represent a strong asset for the development of (MHD) numerical simulations and advanced stellar modelling.
The growing SPIRE team focuses mostly on ab-initio semi-analytical and numerical modelling of the exchanges of angular momentum within stars and their planetary systems and of their impact on their evolution. The successful candidates will benefit from our existing and productive scientific national and international collaborations in stellar and planetary physics, in the study of Star-Planet Interactions, and in fluid dynamics.
Position A 3-year PhD position in stellar magnetohydrodynamics: the successful candidate will collaborate with the PI, Dr. A.-S. Brun and members of the SPIRE project to establish new semi-analytical and numerical models of the excitation, propagation, and damping/resonances/instabilities of internal gravity waves in differentially rotating magnetic stars along their evolution. Obtained equations, prescriptions and scaling laws will be implemented in complete 2D secular transport equations for angular momentum, heat and chemicals in stars, which will be implemented in the dynamical stellar evolution code STAREVOL used by SPIRE members. Applicants should have a Master in astrophysics, geophysics, fluid dynamics or plasma physics.
Position B 4-year post-doc position in modelling tidal flows and their dissipation in stars: the successful candidate will collaborate with the PI and the members of the team to establish new ab-initio semi-analytical and numerical models of tidal torques/dissipation in rotating magnetic stars. She/he will study tidally excited magneto-gravito-inertial waves and their interactions with mean flows, turbulence and magnetic fields in stellar interiors. She/he will contribute to provide prescriptions and scaling laws that will be implemented in STAREVOL and ESPER. The required profile is a candidate with a strong background in theoretical and numerical astrophysical/geophysical fluid dynamics or/and stellar/planetary physics.
For the post-doc position, applicants should have a PhD in astrophysical/geophysical fluid dynamics, theoretical stellar or planetary physics, fluid mechanics or plasma physics. They should have a very good record of research and publications and real interest in theoretical and numerical astrophysics, fluid dynamics and applied mathematics.
These positions funded for at least 3 years (and up to 4 years) by the European Commission via the grant ERC-CoG SPIRE will be reniewed on a yearly basis depending on scientific progress and achievement. The salary will be commensurate to the competitive standard scale for PhD and post-doctoral researchers at CEA. A minimum of 5,000 Euros per year of travel money for each position will also be provided, in addition to the usual funding support of any French institution.
The preferred starting date is 1 September 2015, but can be discussed depending on the availability of selected candidates. Candidates are thus requested to indicate their preferred starting date in their application.
The application for the PhD position must include
– A Curriculum Vitae
– A letter detailing your motivation and qualifications for the position (maximum 1 page)
– Two letters of references. The letters are to be submitted separately to Dr. Stéphane Mathis.
The application for the post-doctoral position must include
– A Curriculum Vitae including publication list
– A statement of research experience, interests and future plans (maximum 3 pages)
– A letter detailing your motivation and qualifications for the position and your career objectives (maximum 1 page)
– Three letters of references. The letters are to be submitted separately to Dr. Stéphane Mathis.
Applications sent before 15 May 2015 for the post-doctoral positions and before 20 April 2015 for the PhD position will be given top priority but applications will be considered until positions are filled.
Laboratory Dynamics of Stars and their Environment CEA/DSM/IRFU/SAp & UMR AIM Paris-Saclay
CEA, Saclay, France
Please contact: firstname.lastname@example.org
Type and duration: 12 months (with possible renewal for a second year)
Project: Exploitation of Space Data for Innovative Helio- and Asteroseismology (SPACEINN – FP7-SPACE-2012-312844)
The Centro de Astrofisica da Universidade do Porto (CAUP) opens a call for one Postdoc Fellowship to work in the thematic line on Towards a Comprehensive Study of Stars. The position is offered with funds provided by the project ‘Exploitation of Space Data for Innovative Helio- and Asteroseismology (SPACEINN FP7-SPACE-2012-312844)’ with financial support provided by European Commission.
The position is to be started by the end of 2014, and no later than January 2015, for one year with the possibility of renewal for a second year depending on performance and the funds available in the project.
The successful candidate is expected to pursue research in the development of asteroseismic diagnostic tools and their application to real data. Other topics associated with CAUP contribution to SPACEINN may also be considered. Previous expertise in stellar physics, seismic interpretation of stellar data and stellar modeling is welcomed. The fellow will also be involved in the other activities and deliverables of SPACEINN to be implemented by CAUP, namely within Work-Package 6 (Training, Outreach & Dissemination).
According to the rules of the National Science Foundation FCT, the yearly income is 17940,00 euro (tax free).
The application should include the following:
- Cover letter/e-mail with a brief description of the candidate’s experience and motivation;
- Short Curriculum Vitae (up to 4 pages) including a list of previous research experience, description of relevant competencies/experience and possible relevant scientific publications (up to 1 additional page);
- Name and contact details (position, email, address) of two referees, available to provide information about the candidate (to be contacted if considered necessary).
The applicant must have completed a PhD degree in astronomy or a related field (physics, mathematics, etc) in a topic relevant for the SPACEINN project. Only applications from candidates having an adequate experience will be considered.
A short-list of candidates will be defined in the first stage of the evaluation based on the submitted application. The short-listed applicants will be required to attend an interview at CAUP for the second stage of the evaluation. If necessary the interview will be done by video- or tele- conference. The contracts will then be offered according to the ordering proposed by the selection committee.
For inquires please contact Mário J. P. F. G. Monteiro.
The deadline for application is the 30th of September 2014.
The positions will be granted only if suitable candidates are found.
- Mário J. P. F. G. Monteiro (Chair)
- Margarida S. Cunha
- Nuno C. Santos
The Max Planck Institute for Solar System Research (MPS) in Goettingen, Germany, invites applications for a postdoctoral position in the framework of EU FP7 Collaborative Project “Exploitation of Space Data for Innovative Helio- and Asteroseismology” (SPACEINN) comprising 17 international research institutions. The position is available immediately for a period of ca. three years. The ideal candidate is an active researcher in helioseismology familiar with SDO/HMI observations. Applications should include a CV and a short statement of research interests. Applications should be sent as a single PDF file to Gizon@mps.mpg.de with the mention “SPACEINN Job” in the subject line. Applications received by 15 September 2013 will receive full consideration. Remuneration of postdoctoral scientists at the MPS is according to the German public salary scale TVoeD. The MPS is an equal opportunity employer and places particular emphasis on providing career opportunities for women.
Max-Planck-Institut für Sonnensystemforschung
Please contact: Gizon@mps.mpg.de
Ref: PostDoc (SpaceInn)
Applications are invited for the full-time position of a post-doctoral scientist at the Kiepenheuer-Institut für Sonnenphysik (KIS), Freiburg, Germany. The position will be part of the collaborative project “Exploitation of Space Data for Innovative Helio- and Asteroseismology – SpaceInn” which is funded under EU’s Framework Programme 7 and aims at an optimal use of existing and planned data in helio- and asteroseismology (http://www.spaceinn.eu).
The successful candidate will join the vibrant research group on helio- and asteroseismology led by Dr. Markus Roth within the Kiepenheuer-Institut für Sonnenphysik in Freiburg. This research group is currently composed of 2 staff scientists, 3 postdocs, 4 Phd students, 2 master students and a number of visiting scientists.
Based on the existing Fourier-Legendre analysis pipeline for helioseismic data at KIS, the successful candiate will work on improving the parameter estimation of p modes, inversions, and implementing the pipeline at the German data center for SDO hosted at the Max-Planck institute for Solar System Research in Katlenburg-Lindau.
Applicants should have a PhD in physics or astrophysics and research experience in helioseismology. Knowledge of programming computer codes and webinterfaces, as well as of helioseismic inversions are of advantage.
KIS is a Foundation of Public Law of the state of Baden-Württemberg with the mission to perform fundamental astrophysics research with an emphasis on solar physics. Current research foci include the Sun, the stars, and advanced instrumention development. KIS operates the German solar facilities at the Teide Observatory on Tenerife, including the new 1.5m Gregor solar telescope, to carry out observations at visible and near-infrared wavelengths. Further information can be obtained at the institute’s webpage (http://www.kis.uni-freiburg.de/).
KIS is committed to increasing the number of female scientists and therefore encourages
qualified women to apply.
The position is available immediately. Starting date can be negotiated. The initial appointment is for 2 years.
The employment, salary, and benefits are according to the rules of the “Tarifvertrag für den
öffentlichen Dienst der Länder” (collective agreement for public services of the Federal States). Full-time positions can be shared, if there is no conflict with official and legal reasons.
Severly handicapped people with equal qualifications will be employed with preference.
The application should include a curriculum vitae, university degree, PhD certificate, a list of publications, copies of three relevant publications, and a list of three potential referees.
Candidates that match the required profile will be continuously interviewed until the position is filled.
Kiepenheuer-Institut für Sonnenphysik
Please contact: email@example.com
SOLARNET will support the mobility of young researchers. This task is supervised by the Mobility Evaluation Committee (MEC), which evaluates and selects the submitted applications. Call for proposals is officially open and will be kept open until the last deadline (see http://www.solarnet-east.eu/networking-activities/mobility for more details).
All proposals received prior to September 15th will be considered by the MEC for the second period (January 1st – June 30th 2014). The decision for this second period will be made on September 30th
Please contact: Francesca.Zuccarello@ct.infn.it
The Centro de Astrofisica da Universidade do Porto (CAUP) opens a call for one Research Fellowship to work in solar and stellar physics including the exploitation of seismic space data. The position is offered with financial support provided by the project ‘Exploitation of Space Data for Innovative Helio- and Asteroseismology (SPACEINN)’ with financial support provided by European Commission. The researcher will be integrated in the team “Origin and Evolution of Stars and Planets”.
Centro de Astrofisica da Universidade do Porto (CAUP)
Please contact: Mario.Monteiro@astro.up.pt