SolarNews
The Electronic Newsletter of the
Solar Physics Division
American Astronomical Society
Volume 2014 Number 22
Yuhong Fan, editor
15 November 2014


NOAA Small Business Innovation Research Solicitation: far-side solar active region monitoring
Tom Berger
03 Nov 2014

The NOAA FY2015 Small Business Innovation Research (SBIR) Solicitation is< now open.

Research topics for FY15 can be found in Section 8 starting on page 51. The FY15 Space Weather subtopic – “Monitoring Active Region Development on the Far Side of the Sun ” – starts on page 60.

*Proposals are due January 15, 2015 at 4:30pm Central time.*

For more information, please refer to the website: www.fbo.gov/index?s=opportunity&mode=form&id=7bf9e70eced0f04a406664d82572040f&tab=core&_cview=1

Please circulate this widely among your colleagues, and let me know if you have any questions.

Thank you,

Tom Berger
Director
NOAA/NWS/NCEP Space Weather Prediction Center


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Solar Physics Topical Issue “Probe the Sun Inside and Out” – First Announcement
Deborah Baker
09 Nov 2014

During Solar Cycle 24, our star went through an unusual period of low solar activity. This extended solar minimum was the first during the space age.  We are able to explore this extended minimum with an unprecedented set of space-based helioseismic and atmospheric data available from the Hinode spacecraft, SOHO, TRACE and SDO.  In addition we have access to historical and contemporaneous data from many ground-based observatories including BISON and GONG.  This wealth of data allows us to connect up unusual behavior in the interior to that of the solar atmosphere and in so doing provide a firm foundation for advances in the understanding of the cyclic behavior of the Sun.

The main objective of this Topical Issue (TI) of Solar Physics is to highlight recent findings achieved by a series of Leverhulme Trust sponsored workshops which combined the skills of helioseismologists and atmospheric scientists to probe the Sun from the inside to outside.  However, this TI will implement an open policy, so will not be limited to Leverhulme Trust workshop contributions.  We also welcome original and relevant manuscripts that were not presented during the workshops.

All submitted manuscripts will be fully refereed. To assist the Solar Physics Guest Editors, Dr Deborah Baker, Dr Rachel Howe, and Prof Louise Harra will act as Guest Editors for this Topical Issue.

We solicit manuscripts on various aspects of solar physics research coupling the various regions of the Sun for inclusion in this TI of Solar Physics. Submission via the Solar Physics on-line submission system will end on 31 January 2015.  In order to assist in the planning, please email Deb Baker (deborah.baker@ucl.ac.uk) to submit a statement of intent describing your article by 31 December 2014, with the following information:

i) title and provisional abstract,
ii) name and e-mail of corresponding author,
iii) author list, and
iv) three suggestions for referees.

Deadlines for submission will be strictly observed and the anticipated publication date for all accepted contributions included in the TI is 31 July 2015. Accepted late papers may appear individually in later Solar Physics volumes.


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Rapidly growing NOAA AR12192 about to rotate back into Sun's near hemisphere
Charlie Lindsey
10 Nov 2014

Its seismic signature having grown considerably during its ongoing transit of the the Sun’s far hemisphere, NOAA AR12192 is now approaching the Sun’s east limb and about to rotate back into direct view from Earth in a few days. This was the active region that presented a monster sunspot in the southern hemisphere during the partial solar eclipse of last October 23. The far-side seismic monitor shows a signature even more intense than in the region’s previous transit of the far hemisphere. Indeed, the seismic signature has grown considerably throughout just the current transit of the far hemisphere.
We have to be careful about predicting what a strong seismic signature actually means. However, there is a strong consensus that it is worth the effort to prepare for something possibly major for any number of purposes. The far-side signature is presently centered at Carrington (247W,14S), which is scheduled to rotate across the east limb at about 00:00 UT of 2014-11-13. Given the 30-degree span in latitude of the seismic signature, the western extremity of the region can be expected to pass across the east limb about a day before this, i.e., at about 00:00 UT of 2014-11-12.

Helioseismic maps of showing AR12192 and other regions in the Sun’s far hemisphere can be accessed at Stanford’s Joint Science Operations Center: “jsoc.stanford.edu/data/farside” updated twice daily.


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Thomas Metcalf SPD Travel Awards for 2015 - Call for Proposals from Meeting Organizers
J. Todd Hoeksema
14 Nov 2014

The Solar Physics Division (SPD) of the American Astronomical Society is pleased to announce the Thomas Metcalf SPD Travel Award program for 2015. The Thomas Metcalf SPD Travel Fund was established in 2007 with generous contributions from his family and many others to help newer members attend meetings relevant to solar physics. Meeting Organizers will select Metcalf Lecturers who can make significant contributions to the meeting.

One or two meetings will be selected for support by the Fund on the basis of brief proposals from meeting organizers. Use of the Fund is not limited to meetings of the SPD. The amount available this year for all awards is expected to be at least $7000.

Organizers of solar physics meetings that will take place before December 31, 2015 are encouraged to submit proposals to the Chair of the Metcalf Travel Award Committee by 7 January, 2015.

Meeting organizers must:

Metcalf Lecturers must:

For additional information about the program, please see spd.aas.org/spd_metcalf_travel.html

If you would like to contribute to the fund, see
members.aas.org/services/aas_member/Donate_Now/GiveNowSingle/AAS_Member/Fundraising/GiveNowSingle.aspx?ItemID=D_TMETCALF

Metcalf Travel Award Committee:


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Employment Opportunities

Tenure track faculty position in space physics at Univ. of Minnesota
Cynthia Cattell
05 Nov 2014

Faculty Position in Space Plasma Physics
University of Minnesota

The School of Physics and Astronomy at the University of Minnesota, Twin Cities invites applications for a tenure track position in the area of Experimental Space Plasma Physics. The appointment is expected to be at the Assistant Professor level. This position is supported by a grant from the National Science Foundation for Faculty Development in the Space Sciences. Candidates are expected to hold a Ph.D. in physics, astrophysics or a related discipline and should have demonstrated the potential to conduct a vigorous and significant experimental research program as evidenced by their publication record and supporting letters from recognized leaders in the field. The ability to teach physics effectively at both the graduate and undergraduate levels is required.  The successful applicant will be joining a department with active programs in both experimental and theoretical space plasma physics. The experimental space physics group has played important roles in instrument development and/or scientific analysis of data from NASA and ESA funded projects including Ulysses, Polar, FAST, Wind, Cluster, and rocket flights. The group is currently involved in the Van Allen Probes Mission, STEREO, and Solar Probe Plus. Experimentalists in any field in space plasma physics are encouraged to apply. Applicants in Solar Physics, Heliospheric Physics, Planetary and Terrestrial Magnetospheric Physics, and Ionospheric Physics are of special interest. The successful applicant will be expected to play a leadership role in new programs involving spacecraft, Cube-Sats, sub-orbital rockets, or balloons. The starting date for the position is negotiable and could be as early as July 1, 2015.
Candidates for this position (Requisition # 193936) must go to employment.umn.edu/applicants/Central?quickFind=123909
and submit an application online. Application materials must include a cover letter, a current C.V. including a list of publications, a statement of research interests, a statement of teaching interests, and a list of at least three references including complete addresses and contact information.

Candidates must arrange to have letters of reference (signed and on official letterhead) sent directly to spacephys14@physics.umn.edu as PDF files. Alternatively, letters of reference may be sent to

Professor Ronald Poling
School of Physics and Astronomy
University of Minnesota
116 Church St. SE
Minneapolis, MN 55455

To ensure full consideration, applications should be received before December 22, 2014. 

The University of Minnesota shall provide equal access to and opportunity in its programs, facilities, and employment without regard to race, color, creed, religion, national origin, gender, age, marital status, disability, public assistance status, veteran status, sexual orientation, gender identity, or gender expression. 


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Ph.D. Position (3 years), solar sciences, Institute of Environmental Physics, University of Bremen, Germany
Mark Weber
07 Nov 2014

Within the new BMBF project SCIASOL (Long-term trends in solar spectral irradiances (SSI) from satellite observations during solar cycles 23 and 24), a detailed re-calibration of SSI data from three European satellite sensors GOME, SCIAMACHY, and GOME-2,covering the time period since 1995 (nearly two solar cycles), shall be carried out. Using these re-calibrated SSI data, extending from the UV to the near IR, changes and variability of solar activity on various time scales from solar rotations to the 11-year solar cycle are to be investigated. The goal is to further reduce uncertainties in changes of solar radiation with the solar cycle which is an important driver of earth’s climate. This project is part of the national (German) research priority program ROMIC (The role of the middle atmosphere in climate).

Prerequisites for this position are:

* a M.Sc. degree or equivalent in physics, astronomy, or (optical) engineering with a grade point average equal or better than B (English grade) or 2.0 (German grade)

* excellent expertise in at least one of the following areas: solar physics, optics, spectrometry, instrument calibration, and satellite remote sensing

* good programming skills in a high level programming language

* very good command of English in writing and speaking (level B2)

Salary is about 1200€ per month after taxes. The PhD student is expected to work halftime in this project (paid) and the other half on his thesis work related to the project (unpaid). 

Electronic applications (cover letter, CV, copies of your certificates, possibly in a single PDF file) are preferred. In case of an application using regular mail, please send us your application in plain paper (no folders) and do not send us original certificates as we are not able to return your applications. Please indicate the job id A167/14 in your application. Deadline for application is December 1, 2014.

The complete job advert in English and German you can find at www.iup.uni-bremen.de/UVSAT/jobs


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Max Planck Research Group Leader Position in Solar Physics at the Max Planck Institute for Solar System Research
Johannes Stecker
11 Nov 2014

The Max Planck Institute for Solar System Research (MPS) offers the opportunity to set up a Max Planck Research Group in the field of Solar Physics to an outstanding young scientist.

MPS (www.mps.mpg.de/en) is the leading German research institute in the field of solar system science. Its three scientific departments are devoted to solar physics, planets and minor bodies, and the interior of the Sun and stars, respectively. The solar department has leading participations in high-profile solar space missions, is involved in several ground-based observational programs, has successfully flown the Sunrise balloon-borne observatory and provides outstanding opportunities for theoretical and numerical work. The research fields include dynamo processes, solar variability and climate, solar magnetic fields, physics of the photosphere, chromosphere, transition region, corona and solar wind, as well as stellar magnetism (further details can be found at www.mps.mpg.de/1762321/sonne).

The successful candidate is expected to pursue a research program that fits or complements the current topics of the department. He/she will be offered a Max Planck Research Group for a period of five years (with the possibility of an extension after successful evaluation pending availability of funding). This includes a W2 position equivalent to the associate professor level and a grant that covers postdoc and PhD student positions, a budget for travel, publication costs and other expendables and additional funds for equipment. For more information on Max Planck Research Groups please see www.mpg.de/max_planck_research_groups

The group will benefit from the institute’s excellent technical infrastructure, as well as from scientific exchange with existing research groups at the Institute and from a vibrant scientific atmosphere. The necessary administrative support will be provided.

The institute is located in Göttingen, Germany, a lively and scenic university town, in a well-equipped new building on the northern campus of the University, in the immediate vicinity of the Institute for Astrophysics of the University.

Applicants must hold a Ph.D. in physics, astrophysics or a closely related field. They should have an outstanding research record including the publication of significant research papers. The establishment of a competitive research program and application for third party funds are expected. The primary criterion for selection will be the proven ability to independently conduct internationally recognized research of high quality.

The position is aimed at talented junior scientists. Ideally, applicants should have obtained their doctorate a maximum of seven years ago, although exceptions are possible.

Applications including a CV, a publication list, a description of past research activities and a research plan for the group should be sent to pds@mps.mpg.de. In addition, applicants should arrange to have three letters of reference sent separately to Sami K. Solanki (solanki-office@mps.mpg.de). Review of applications will begin January 15, 2015 and continue until the position is filled.

The Max Planck Society is aiming to increase the percentage of women on its scientific staff and strongly encourages applications from qualified women. The Max Planck Society is also committed to employ more handicapped individuals and especially encourages them to apply.

For further information please contact Sami. K. Solanki (solanki@mps.mpg.de) or Johannes Stecker (stecker@mps.mpg.de).


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Postdoctoral position in Particle Acceleration High Energy Astrophysics
Vahe Petrosian
11 Nov 2014

The Physics Department at Stanford University invites applications for a post-doctoral position in Professor Petrosian’s research group.  This appointment is for two or three years and will be reviewed annually.  Starting date could be as early as January 1, 2015.

Professor Petrosian’s primary research area is in high energy astrophysics more specifically, in particle acceleration in astrophysical sources such as solar flares, accretion disks and jets, and the interstellar and intra-cluster mediums. More information can be found at physics.stanford.edu/people/faculty/petrosian/group and past publications can be viewed by clicking on ADS and astro-ph.

Successful applicants are expected to pursue research in areas related to the current research in the group with initial focus on particle acceleration in solar flares using existing codes and data from RHESSI, Fermi and as well as ground based observations. The successful applicant will be encouraged to be involved with other research activities of Kavli Institute of Particle Physics and Cosmology (KIPAC) a joint institute of the Departments of Physics and SLAC at Stanford University.  Further information about KIPAC is available at kipac.stanford.edu/kipac/

Applicants should have, or be in the process of completing, a Ph.D. in Astronomy or Physics and should possess a strong research background.  Review of applications will begin at end of December 2014 and continue until the position is filled.  Inquiries may be addressed to Prof. Petrosian (vahep@stanford.edu). 

Applicants should provide a statement of research interests, a CV, and three letters of reference. This information should be sent to Dana Volponi (volponi2@stanford.edu).


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George Ellery Hale Postdoctoral Fellowship Position in Solar Physics at the University of Colorado Boulder
Molly Hand
12 Nov 2014

George Ellery Hale Postdoctoral Fellowship Position in Solar Physics at the University of Colorado Boulder

The University of Colorado Boulder is seeking applicants for the George Ellery Hale Postdoctoral Fellowship in Solar and Space Physics.  The University of Colorado and surrounding institutions provide a rich environment within which to conduct solar research, and this two-year research fellowship accompanies the relocation of the National Solar Observatory (NSO) headquarters to Boulder.

Of particular interest are postdoctoral candidates who are interested in theoretical and computational studies of dynamics within solar and stellar interiors, photospheres, and atmospheres (chromospheres and coronae).  Boulder is an internationally recognized center for studying convection, turbulence, radiative magnetohydrodynamics, and the dynamo amplification of magnetic fields in the Sun.  The successful candidate will have access to extensive computational resources and existing modern, highly parallel astrophysical fluid dynamics codes, and could be involved in the creation of next generation codes for studying solar fluid dynamics. Connections between such modeling activities efforts and the observational capabilities of NSO’s Daniel K Inouye Solar Telescope (DKIST, formerly ATST) and/or Integrated Synoptic Program (NISP) will enhance an application, and the successful candidate is encouraged to forge those connections while in Boulder.

The successful candidate will also have the opportunity play a prominent role in the new George Ellery Hale collaborative graduate education program, which aims to offer solar physics course work and summer professional development to students enrolled in graduate programs at the University of Colorado, University of Hawaii, and the New Jersey Institute of Technology via telepresence technology.  The successful candidate will have the opportunity to work closely with the program to develop capability and facilitate learning in this distributed environment. Thus candidates with a strong interest and experience in teaching and learning methodologies, in addition to those more focused on solar physics research goals, are encouraged to apply.

Applicants should submit a curriculum vitae, a list of publications, a description of research and teaching interests, and the names and contact information for three references.  These materials should be submitted electronically to: www.jobsatcu.com, posting #RF01913.

For more information please contact Prof. Benjamin Brown, Search Committee Chair, bpbrown@colorado.edu.  Review of the applications will begin 1 December 2015 and continue until the position is filled.  The University of Colorado is an Equal Opportunity Employer.

The University of Colorado offers a full benefits package. Information on University benefits programs, including eligibility, is located at www.cu.edu/employee-services/benefits


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Meeting Announcements

Studentships Available for 2015 TESS Meeting
Gordon Emslie
03 Nov 2014

The Solar Physics Division is pleased to announce the availability of funds to support student participation in its next annual meeting, to be held as part of the Triennial Earth-Sun Summit from April 26 – May 1, 2015 in Indianapolis, IN – see aas.org/meetings/tess2015

More detailed information on how to apply for studentship awards, and on the associated obligations (e.g., presenting a paper at the meeting), can be found at spd.aas.org/studentships.html

Note: Because the abstract submission opens very early (November 14, 2014) and closes in late January, applications for studentships are being sought much earlier this year!  Applications are due by December 10, 2014}; awardees will be notified by January 5, 2015, giving time to submit an abstract by the abstract deadline.

Please feel free to distribute this notice to any individuals who may not be on the SolarNews mailing list but who nevertheless may be interested in this opportunity.

Advisors please note: the SPD strongly encourages applications for partial support, with the remainder of the necessary funds coming from other (e.g., grant, university) sources.  Note especially the requirement (see website) that the supporting advisor letter include “an evaluation of the student’s financial requirements for attending the meeting and the extent to which partial support from other sources is available.”  Ideally, such a statement should also detail amounts for airfare, hotel, etc.  Applications that simply state “any support that can be provided will be greatly appreciated” (or similar words) are discouraged.

The SPD Student Committee (Gordon Emslie, Matthias Rempel, Kathy Reeves)


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Approaching abstract deadline for RAS Discussion Meeting on the Dynamical Chromosphere
Ailsa Prise
13 Nov 2014

The Dynamical Chromosphere and its Role in Energy Transfer through the Solar Atmosphere: Results from IRIS

The abstract deadline is approaching for this RAS Specialist Discussion Meeting, being held on 9th January 2015.

This meeting will bring together researchers to discuss new results from IRIS: linking IRIS observations with those in the photosphere and corona, and using theory and simulations to advance our understanding of the energy transfer between these layers. Invited talks will be given by Bart De Pontieu (Lockheed Martin Solar & Astrophysics Laboratory) and Mats Carlsson (University of Oslo). Further details can be found at: www.ucl.ac.uk/mssl/solar/ras-chromosphere/

Please send your title and abstract to ailsa.prise.11@ucl.ac.uk by Monday 1st December.

Organisers:
Louise Harra (MSSL, UCL), Alan Hood (University of St. Andrews), Ailsa Prise (MSSL, UCL)


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First Announcement: Coimbra Solar Physics Meeting "Ground based Solar Observations in the Space Instrumentation Era", 5 – 9 October 2015, University of Coimbra, Coimbra, Portugal
Ivan Dorotovic
13 Nov 2014

The Sun and its activity affect the entire heliosphere, including the Earth. Solar activity includes flares, coronal mass ejections (CMEs), eruptive prominences and filaments, outbursts at various spatial scales, sunspots, and plages. All these phenomena are driven by the magnetic field. Although these phenomena appear at time scales from seconds to months, the long-term variation of the magnetic field during the 11-year solar cycle modulates their frequency and space weather impact. Coronal phenomena are driven by the dynamo-generated fields that show large-scale organization.

Solar magnetic fields can be investigated from ground and space. Ground based observations of solar magnetic fields using polarimetry has a long history, contributing to the understanding of long-term behaviour of the Sun. Spectropolarimetric observations in FUV and EUV lines can only be made from space; they represent virgin territory and they are urgently needed for exploring the magnetic activity of the upper chromosphere and transition region.

This CSPM-2015 scientific meeting will cover various aspects of solar dynamic and magnetic phenomena which are observed over the entire electromagnetic spectrum: white-light, Hα, Ca II, and radio from ground and in a variety of other wavelengths (UV and EUV, and X-rays) from space. Emphasis will also be placed on instrumentation, observing techniques, solar image processing techniques, as well as theory and modelling through detailed radiative transfer in increasingly realistic MHD models. The long-term (cyclic) evolution of solar magnetism and its consequence for the solar atmosphere, eruptive phenomena, solar irradiation variations, and space weather, will be in focus. Here, special attention will be devoted to the long-term observations made in Coimbra and also to the results of the SPRING / SOLARNET and SCOSTEP VarSITI studies. In particular, the weak solar activity during the current solar maximum will be discussed. Finally, since this meeting is organised around the 90th anniversary of performing the first spectroheliographic observations in Coimbra, a session will be specially dedicated to new solar instruments (both ground-based and space-borne) that will give access to unexplored solar atmospheric features and dynamic phenomena over the coming years.

Scientific Organizing Committee:
J. Aboudarham (France), F. Clette (Belgium), I. Dorotovic (Slovakia/Portugal), C. Fischer (Germany), L. Fletcher (UK), N. Gopalswamy (USA), A. Kucera (Slovakia), D. Maia (Portugal), M. Sobotka (Czech Republic), Y. Suematsu (Japan), M. Temmer (Austria), J. Trujillo Bueno (Tenerife, Spain), G. Tsiropoula (Greece), B. Vrsnak (Croatia)

For further information please visit www.mat.uc.pt/~cspm2015 .


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EGU session - ST1.4/PS5.5: Preconditioning of interplanetary space
Manuela Temmer
14 Nov 2014

We would like to raise your interest to the following session at the EGU 2015, 12 – 17 April in Vienna, Austria.

ST1.4/PS5.5: Preconditioning of interplanetary space – a Space Weather parameter
For more details see: meetingorganizer.copernicus.org/EGU2015/session/18234
Benoit Lavraud accepted to give a solicited talk on the topic.

Deadlines:
28 November 2014 - Deadline for Support Applications
07 January 2015, 13:00 CET - Deadline for Receipt of Abstracts

Looking forward meeting you in Vienna!
Manuela Temmer
(also on behalf of my co-conveners Tibor Török, Jie Zhang, Volker Bothmer).


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Judges Needed for Student Presentations at AGU --- Please Help!
Brian Welsch
14 Nov 2014

Almost 200 student papers in SPA sessions were entered in the Outstanding Student Paper Awards program for the upcoming Fall AGU meeting, an increase of 20% over last year.

Please help us make sure every student gets evaluated fairly by volunteering to judge!  You can provide students with valuable feedback via presentation scores and comments regarding their scientific research.  Students are grateful to hear from scientists in their field,  and are eager to learn from you!

All three SPA subsections (SA, SH, SM) need judges, but the need is especially acute for SM sections.

Judges typically evaluate three papers. Sign-Up is Easy:

* Use your AGU member login to the OSPA system, ospa.agu.org/ospa/
* Judges must be AGU members and cannot be students
* Click on “Find Presentations” at right
* Search by session, paper title, keyword, or presentation type (oral, poster); you can’t judge students from your institution.
* You can add/remove presentations until the Meeting starts, but are then responsible for ensuring that they are judged.

You will be notified if any presentations that you signed up to judge are moved / cancelled.

Score sheets can be edited up until 11:59pm EST on Tuesday, 23 December.

Thank you for your help—the students very much appreciate it and are looking forward to hearing from you!

Sincerely,

Brian Welsch, Elizabeth Mitchell, and Allan Weatherwax, SPA-OSPA committee
Kara Smedley Rodean, Program Manager - Student Member Initiatives


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EGU2015- Opportunities for Students & Young Scientists
Claire Foullon
14 Nov 2014

Dear Colleagues,

There are several opportunities for students and young scientists planning to participate in EGU General Assembly 2015, 12 - 17 April, Vienna, Austria:

OUTSTANDING STUDENT POSTER (OSP) AWARD PROGRAM.
The Solar-Terrestrial Sciences (ST) Program Group takes part in the OSP program, whereby undergraduate and PhD students can register to have their posters take part. Abstract Submission Deadline: 7 January 2015. Full information on eligibility is at www.egu.eu/awards-medals/union-osp-award/

FINANCIAL SUPPORT FOR YOUNG SCIENTISTS.
Support Application Deadline: 28 November 2014. Full information on eligibility is at www.egu2015.eu/support_and_distinction.html

MORE FOR YOUNG SCIENTISTS.
Our ST Young Scientist (YS) Representative, Beate K. Humberset, is there to make the link between the EGU and the young scientist community. Get involved with your ST Division or with the Union & sessions, short courses and meetings of special interest at the Assembly, to follow at www.egu.eu/young-scientists/at-the-assembly/sessions/

All the very best,

Claire Foullon
(OSP coordinator ST)

Norma B. Crosby
(Division President ST)

Solar-Terrestrial Sciences Division: www.egu.eu/st/
EGU2015 Meeting Web Site: egu2015.eu/
EGU2015 ST programme: meetingorganizer.copernicus.org/EGU2015/sessionprogramme/ST


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Editor's Note

2014 SolarNews Instructions
Yuhong Fan
15 Jan 2014
`

SolarNews is normally distributed on the first and fifteenth of each month. Please send in your submissions by midnight the day before.

The SPD Web site can be found at spd.aas.org. The HTML version of SolarNews can be found at spd.aas.org/SolarNews/archive/news.html or solarnews.nso.edu. It contains in-line hyperlinks to all the Web sites and e-mail addresses mentioned in this issue. Archived back issues can be retrieved at solarnews.nso.edu.

SolarNews submissions can be in plain text or HTML markup. Submissions should be made via the submission webform at solarnews.aas.org/

Please try to keep meeting and workshop announcements to no more than one page (fewer than 60 lines of typed text with 72 characters per line), with a Web address for further information.

If you wish to subscribe, unsubscribe from SolarNews, get a password reminder, or change your subscription, go to:
mailman.ucar.edu/mailman/listinfo/solarnews

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