Postdoc – Ionospheric radio occultations at Saturn, Titan, and Mars

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Current state: Approved and Notify DPS Secretary
Department: Center for Space Physics
City: Boston
State/Province: MA
Country: USA
Contact Person: Paul Withers
Contact Email: [email protected]
Institution: Boston University
Application Due Date: Friday, July 01 2016

The Center for Space Physics at Boston University invites applications for a postdoctoral researcher position supervised by Professor Paul Withers. The research will involve the analysis of radio occultation observations of the ionospheres of Saturn, Titan, and Mars. Candidates should possess a PhD degree in a relevant field. Experience conducting research on planetary ionospheres is desirable. The salary offered will be competitive and commensurate with experience. Funding is available for two years with the possibility of extension. The appointment is expected to begin as soon as possible after 1 September 2016. Please contact Paul Withers ([email protected]) for further information.

Applications should be sent by email to Paul Withers ([email protected]). The application should be submitted in PDF format and contain a curriculum vitae, statement of research interests, and contact information for three referees. Review of applications will begin on 1 July 2016. Women and underrepresented minorities are particularly encouraged to apply. Boston University is an equal opportunity/affirmative action employer.

Postdoctoral Research Assistant in Planetary Science: Titan’s Atmosphere

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Current state: Approved and Notify DPS Secretary
Department: School of Earth Sciences
City: Bristol
Country: UK
Contact Person: Nick Teanby
Contact Email: [email protected]
Institution: University of Bristol
Application Due Date: Monday, April 13 2015
Web Link: http://www.bristol.ac.uk/jobs/find/details.html?nPostingID=3021&nPostingTargetID=10847

Postdoctoral Research Assistant in Planetary Science: Titan’s Atmosphere

University of Bristol, UK, School of Earth Sciences

Closing date:    13-Apr-2015
Salary:        £31,342 – 39,685, depending on experience

Applications are invited for a three year Post-doctoral Research Assistant/Associate in Planetary Sciences, within the School of Earth Sciences, to study the atmosphere of Saturn’s largest moon, Titan, using remote sensing data.

The successful applicant will study seasonal changes in Titan’s complex atmosphere based on data from the Cassini spacecraft’s Composite InfraRed Spectrometer (CIRS), which is sensitive to stratospheric composition and temperature. However, the project may also involve using data from Cassini’s other remote sensing instruments, or ground-based and space-based telescope data to allow more complete interpretations. Spectroscopic observations will be analysed using radiative transfer, inverse theory, and time series analysis techniques. These observational analyses will be used to investigate atmospheric changes over the course of the Cassini mission and constrain dynamical and chemical atmospheric models.

For further details and application procedure see:
http://www.bristol.ac.uk/jobs/find/details.html?nPostingID=3021&nPosting…

Jovian Magnetic Field and Magnetosphere Postdoctoral Researcher

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Current state: Approved and Notify DPS Secretary
Department: Planetary Magnetospheres Laboratory (GSFC); Dept. of Astronomy (UMD)
City: Greenbelt
State/Province: MD
Country: USA
Contact Person: Tracy Huard
Contact Email: [email protected]
Institution: NASA-GSFC/CRESST/University of Maryland
Application Due Date: Saturday, January 24 2015
Web Link: http://www.astro.umd.edu/employment/index.html#Juno

Applications are now being accepted for a Postdoctoral Research Associate, funded through the University of Maryland College Park (UMCP) and the Center for Research and Exploration in Space Science and Technology (CRESST), to work in the Planetary Magnetospheres Laboratory of the NASA Goddard Space Flight Center (GSFC) in the area of Jupiter’s magnetic field and magnetosphere, using data from the Juno (New Frontier) mission.

The Juno spacecraft arrives at Jupiter in July 2016. Juno is the first spacecraft to explore Jupiter from a close-in, polar orbit, seeking to unlock secrets about its origin and the origin of the solar system. Juno will probe deep into Jupiter’s interior by mapping the giant planet’s magnetic and gravity fields, peering well below the clouds to determine atmospheric composition, with particular interest in water abundance. Juno will also conduct a study of the polar magnetosphere and auroral phenomena, with fields and particles instruments and both infrared and ultraviolet spectrometers among the payload. Juno’s Magnetic Field Investigation (MAG) employs two identical measurement platforms occupying a 4-meter magnetometer boom mounted at the outer end of one of Juno’s three solar arrays. Each MAG optical bench supports a high-accuracy vector fluxgate magnetometer and a pair of star camera sensors for precision inertial attitude reference. These data and the global coverage of Jupiter provided by the mission plan will result in a detailed model of the Jovian internal field and an unprecedented view of the dynamo.

The selectee will work on site at GSFC in the Solar System Exploration Division as a member of the Juno Magnetometer Investigation Team, participating in data analysis and scientific studies, leading to publication of results in scientific journals. Candidates for this position should have a Ph.D. in a relevant scientific discipline with prior experience conducting scientific research. Experience with magnetometer instrumentation and data, disciplined programming skills (primarily Fortran and IDL), and scientific writing experience are desired.

The appointment will be initially for one year, with the possibility of renewal in subsequent years.  Applicants may be new postdocs or may be more senior. Each applicant should send a Curriculum Vita, list of publications, statement of research interests, and contact information for three references to:

Juno Magnetometer
CRESST/UMCP
Mail Code 660.8, NASA/GSFC
Greenbelt, MD 20771,
or Via e-mail to [email protected]

Information regarding the Juno mission is found at http://missionjuno.swri.edu/ and http://www.nasa.gov/mission_pages/juno/main/. Information on the Planetary Magnetospheres Laboratory is found at http://science.gsfc.nasa.gov/solarsystem/magnetospheres/. For information on CRESST and the UMCP’s Department of Astronomy, please contact Tracy Huard ([email protected]).

The University of Maryland is an Affirmative Action, Equal Opportunity Employer. Women and minorities are encouraged to apply. Applications will be accepted on an ongoing basis until the position is filled.

Jovian Magnetic Field and Magnetosphere Post-doc Researchers

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Current state: Approved and Notify DPS Secretary
Department: Planetary Magnetospheres Laboratory (GSFC); Dept. of Astronomy (UMD)
City: Greenbelt
State/Province: MD
Country: USA
Contact Person: Tracy Huard
Contact Email: [email protected]
Institution: NASA-GSFC/CRESST/University of Maryland
Application Due Date: Friday, September 26 2014
Web Link: http://www.astro.umd.edu/employment/#Juno

Applications are now being accepted for a Postdoctoral Research Associate, funded through the University of Maryland College Park (UMCP) and the Center for Research and Exploration in Space Science and Technology (CRESST), to work in the Planetary Magnetospheres Laboratory of the NASA Goddard Space Flight Center (GSFC) in the area of Jupiter’s magnetic field and magnetosphere, using data from the Juno (New Frontier) mission.

The Juno spacecraft arrives at Jupiter in July 2016. Juno is the first spacecraft to explore Jupiter from a close-in, polar orbit, seeking to unlock secrets about its origin and the origin of the solar system. Juno will probe deep into Jupiter’s interior by mapping the giant planet’s magnetic and gravity fields, peering well below the clouds to determine atmospheric composition, with particular interest in water abundance. Juno will also conduct a study of the polar magnetosphere and auroral phenomena, with fields and particles instruments and both infrared and ultraviolet spectrometers among the payload. Juno’s Magnetic Field Investigation (MAG) employs two identical measurement platforms occupying a 4-meter magnetometer boom mounted at the outer end of one of Juno’s three solar arrays. Each MAG optical bench supports a high-accuracy vector fluxgate magnetometer and a pair of star camera sensors for precision inertial attitude reference. These data and the global coverage of Jupiter provided by the mission plan will result in a detailed model of the Jovian internal field and an unprecedented view of the dynamo.

The selectee will work on site at GSFC in the Solar System Exploration Division as a member of the Juno Magnetometer Investigation Team, participating in data analysis and scientific studies, leading to publication of results in scientific journals. Candidates for this position should have a Ph.D. in a relevant scientific discipline with prior experience conducting scientific research.  Experience with magnetometer instrumentation and data, disciplined programming skills (primarily Fortran and IDL), and scientific writing experience are desired.  

The appointment will be initially for one year, with the possibility of renewal in subsequent years.  Applicants may be new postdocs or may be more senior.  Minority candidates are encouraged to apply. Each applicant should send a Curriculum Vita, list of publications, statement of research interests, and contact information for three references to:

Juno Magnetometer
CRESST/UMCP
Mail Code 660.8, NASA/GSFC
Greenbelt, MD  20771, or
Via e-mail to [email protected]

Information regarding the Juno mission is found at http://missionjuno.swri.edu/ and http://www.nasa.gov/mission_pages/juno/main/ .  Information on the Planetary Magnetospheres Laboratory is found at http://science.gsfc.nasa.gov/solarsystem/magnetospheres/ .  For information on CRESST and the UMCP’s Department of Astronomy, please contact Tracy Huard ([email protected]).  The position will remain open until filled.

The University of Maryland is an equal opportunity employer.  All applications received by September 26, 2014 will receive full consideration.

IMPRS PhD Scholarships in Solar System Science at MPS in Göttingen, Germany

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Current state: Approved
Department: International Max Planck Research School for Solar System Science at the University of Göttingen
City: Göttingen
Country: Germany
Contact Person: Sonja Schuh
Contact Email: [email protected]
Institution: Max Planck Institute for Solar System Research
Application Due Date: Friday, November 15 2013
Web Link: http://www.solar-system-school.de/application.html

 The International Max Planck Research School for Solar System Science at the University of Göttingen (“Solar System School”) offers a research-oriented doctoral program covering the physical aspects of Solar system science. It is jointly run by the Max Planck Institute for Solar System Research (MPS) and the University of Göttingen.

Learn more about the International Max Planck Research Schools (IMPRS) of the Max Planck Society.
Learn more about the Max Planck Institute for Solar System Research (MPS).
Research at the MPS covers three main research areas:

Sun and heliosphere Planets and Comets Stellar and Solar Interiors
Solar System School students collaborate with leading scientists in these fields and graduates are awarded a doctoral degree from the renowned University of Göttingen or, if they choose, another university.

Learn more about the University of Göttingen:
Georg-August-University of Göttingen Brochure
Georg-August-University of Göttingen Short profile
The Solar System School is open to students from all countries and offers an international three-year PhD program in an exceptional research environment with state-of-the-art facilities on the Göttingen Research Campus. Successful applicants receive an attractive scholarship covering relocation support, housing and living expenses and are exempt from tuition fees.

Learn more about IMPRS PhD scholarships (grants).
The language of the structured graduate program is English, with complimentary German language courses offered (optional). The program includes an inspiring curriculum of scientific lectures and seminars as well as advanced training workshops and provides travel funds to attend international conferences.

Applicants to the Solar System School should have a keen interest in Solar system science and a record of academic excellence. They must have, or must be about to obtain, an M.Sc. degree or equivalent in physics or a related field, including a written Masters thesis (or a scientific publication), and must document a good command of the English language.

Review of applications for a starting date of September 2014 will begin on 15 November 2013, but other starting times are also negotiable. Scholarships are awarded on a competitive basis.

Applications should be prepared following the instructions below and must include:

a curriculum vitae;
a completed application form in PDF format, including a list of all courses with credits and grades;
a transcript of all academic records, including copies of High School Diploma, B.Sc., and M.Sc. or equivalent degree, with English or German translations.
Download the application form (PDF)
It is highly recommended to also send

GRE Physics test scores or equivalent for candidates who have obtained their Master’s degree at a university outside of Europe;
Certificate to prove proficiency in the English language, for candidates whose native language is not English or German (e.g. transcript of TOEFL / IELTS scores or equivalent).
Link to GRE subject tests
Link to TOEFL
Link to IELTS
The completed application must be sent by email in one single PDF file as an attachment to the address [email protected].

Two letters of recommendation prepared using the PDF form should be emailed to the same address by the referees.
For referees: Download the letter of recommendation form (PDF)
The Solar System School is committed to increase the diversity of its student body and particularly encourages applications from members of under-represented groups.

Further information:

Download the Call for applications (pdf).
Download the Solar System School Poster (pdf).
Browse answers to Frequently Asked Questions.
Please direct any further inquiries to the IMPRS scientific coordinator, Dr. Sonja Schuh, at [email protected].

Postdoctoral researcher in Planetary Sciences

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Current state: Approved
Department: Applied Physics I
City: Bilbao
Country: Spain
Contact Person: Agustin Sánchez Lavega
Contact Email: [email protected]
Institution: University of the Basque Country UPV/EHU
Application Due Date: Monday, July 15 2013
Web Link: http://www.ajax.ehu.es/

Applications are invited for a postdoctoral position at the University of the Basque Country (UPV/EHU), working with Prof A. Sánchez Lavega on Planetary Atmospheres. The successful candidate will join the Planetary Science Group at the Applied Physics Department in the Faculty of Engineering of the UPV/EHU, located in central Bilbao. The Planetary Science Group (http://www.ajax.ehu.es/) is a consolidated research group of the highest rank within the Basque Government Research System, and it is presently involved in several international space missions and proposals. Candidates with proven expertise in one of the following areas will be considered: – Dynamical modeling of planetary atmospheres (numerical methods) – Radiative transfer in planetary atmospheres (optical and infrared). Successful candidates must have a PhD in astrophysics, geophysics (planets) or a related discipline. They must be able to work independently, have a high degree of computer literacy and a proven ability to reduce scientific data. Proficiency in high level programming is essential and experience with parallelization desirable. The post is funded by the Directorate for Science Policy of the Basque Government. The initial appointment is for one year, but it is renewable until December 2015. Gross salary is of approximately 32000 € per year. The position will be open until we find a suitable candidate. Informal enquiries are welcomed and should be addressed to Dr. T. del Río Gaztelurrutia ([email protected]) and Prof. A. Sánchez Lavega ([email protected]) including a curriculum vitae and a statement of research experience and interests. Applicants should arrange for two academic references to be sent to [email protected] and [email protected].