Dear Colleagues,
Here are a few items which have come to our attention since the last Newsletter.
You can find this news also at the UKSP website:
http://www.uksolphys.org/news/last-15-days/
or the newsletter in full in our JISCMail archive:
http://www.jiscmail.ac.uk/uksp
Richard ([log in to unmask])
Mihalis ([log in to unmask])
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General News/UKSP Business:
European Solar Physics Division (ESPD) – 2019 PhD Thesis and Early Career Researcher Prizes: First Call for Nominations
SOLARNET Access Time – First Call for Proposals 2019
GREGOR/VTT – Call for Observing Proposals 2019A (Apr 28 – Aug 1)
Astronomy Guidelines – 2019
Invitation to join Whole Heliosphere and Planetary Interactions campaigns
Nuggets:
Two new RHESSI Science Nuggets
Meetings/Workshops/Summer Schools:
Save the Date: “Scintillating Science: Cutting-Edge Science Achieved Through the Observations of Radio Scintillation” Workshop
Deadline for NAM session proposals is 7th January
RAS Discussion meeting (G) – 8th March 2019 from 10:30 at the RAS Lecture Theatre, Burlington House, London
EGU call for abstracts: ST4.5 Prediction of Solar Flares and Eruptions
China-Europe Solar Physics Meeting – Second announcement
EWASS – Session on Coronal Mass Ejections, observations and models
AOGS2019 ST20 Solar Flare Forecasting Using Machine Learning
Jobs/Studentships:
NCAR Advanced Study Program (ASP) and High Altitude Observatory (HAO: Boulder, Colorado) – Postdoc Positions, Application Deadline January 4, 2019
Istituto Ricerche Solari Locarno (IRSOL, Locarno Monti, Switzerland) – Postdoctoral Contract: SOLARNET2 Project
PhD position in Solar Physics available at Northumbria University
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General News/UKSP Business:
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European Solar Physics Division (ESPD) – 2019 PhD Thesis and Early Career Researcher Prizes: First Call for Nominations
from Richard Morton [December 15, 2018]
Deadline: February 15th, 2019
Since 2017, the European Solar Physics Division (ESPD) of the European Physical Society (EPS) awards two prizes yearly: the ESPD PhD Thesis Prize and the ESPD Early Career Researcher (Postdoc) Prize. These prizes are nomination-based. The deadline for nomination is February 15th, 2019.
The 2019 ESPD PhD Thesis Prize will be awarded to a young researcher whose PhD thesis/viva was defended in 2018.
The 2019 ESPD Early Career Prize will be awarded to a young researcher whose PhD was awadered after 01/012015 (with possible extension).
Further information about eligibility, documents to be included in the nomination package, and submission process for each prize can be found on the ESPD prizes webpage: www.eps.org/members/group_content_view.asp?group=85203&id=641304
Étienne Pariat for the ESPD Prize Committee
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SOLARNET Access Time – First Call for Proposals 2019
from Richard Morton [December 15, 2018]
Proposals are hereby invited under the SOLARNET Trans-National Access Programme for observing time at the solar telescopes GREGOR, SST, THEMIS, and VTT. This call also includes observing time in the International Time Program (ITP).
Proposals will be handled by the EAST TAC, a common European time allocation committee installed by the European Association for Solar Telescopes. Typically, successful proposals will be awarded with 10 observing days. SOLARNET campaigns also get travel grants for going to the telescope. In 2019, the SST will provide some of its time in service mode, thus not requiring visits by the investigators. Certain criteria of eligibility related to the nationalities of the applicants exist. If in doubt, ask. New users of the facilities are encouraged to apply.
Data acquired in the SOLARNET Access Programme will become public one year after being delivered to the PI.
Information on instrumentation and proposal details are available at the telescope web pages:
GREGOR
SST
THEMIS
VTT
Proposals can be made for each individual telescope or for a combination of them. All applications will be assumed to be for both SOLARNET and ITP when possible. All proposals should be sent via email to [log in to unmask] and must be received by January 20, 2019.
Disclaimer: SOLARNET is expected to be funded by the European Union’s Horizon 2020 research and innovation programme under grant agreement No. 824135. The awarding of SOLARNET observing time is contingent on the signing process that is currently underway.
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GREGOR/VTT – Call for Observing Proposals 2019A (Apr 28 – Aug 1)
from Richard Morton [December 15, 2018]
GREGOR is a 1.5 meter on-axis solar telescope at the Observatorio del Teide in Tenerife operated in PI mode. VTT is a coelostat with a 70 cm main mirror, also operated in PI mode. We invite proposals for observing campaigns at GREGOR and/or VTT in 2019, with a submission deadline of January 18, 2019, 23 UT. Both telescopes will operate with 2 observing seasons in 2019 and the available instrumentation differs in both seasons. This call is for the first season, another call may be expected in May.
Instrumentation available for the first season is:
GREGOR:
GRIS IFU (image slicer) at wavelengths 1.0–1.3 or 1.5–1.8 microns. This instrument can record spatial and spectral information simultaneously in a FOV of 6”x3”. Simultaneous H-alpha and continuum slitjaw images are available.
Fast context imaging in any wavelength below 900 nm (below 480 nm if using GFPI) if a suitable filter is available or provided by the observers.
Imaging spectroscopy (no polarimetry) with GFPI at wavelengths below 860 nm. This instrument is available only in collaboration with AIP and please contact them before proposal submission.
Please see our website for the current capabilities and restrictions.
VTT:
The chromospheric grating for spectroscopy in up to 3 spectral regions simultaneously
Own instrument setups
There are different quotas for observing time in 2019A:
KIS: 24 days. Eligibility: Any researcher with no restriction on institute/nationality can apply for observing time if at least one collaborator from KIS is included in the proposal.
– Spanish time: 16 days. Eligibility: No restriction on institute/nationality.
CCI time: 8 days. Application via EAST TAC. Eligibility: Anybody apart from the operators of the telescope.
SOLARNET (see separate call, send proposals to [log in to unmask] Deadline 20 January): 20 days. Eligibility: The PI and the majority of the users must work at institutions which are outside the country(ies), which operate the telescope (Germany, Spain). Travel and lodging grants are available for up to 2 people.
The remaining time is reserved for partners.
The proposal form for KIS time and more information on the instrumentation can be found here:
www.leibniz-kis.de/en/observatories/gregor/observing-with-gregor/
www.leibniz-kis.de/en/observatories/vtt/observing-with-vtt/
and on the “Scientific instruments” page. Proposal submission for SOLARNET and Spanish time is announced in separate calls.
For questions, please contact L. Kleint (KIS and GREGOR/VTT SOLARNET time; [log in to unmask]) or E. Khomenko (Spanish time; [log in to unmask])
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Astronomy Guidelines – 2019
from Sian Giles [December 14, 2018]
Dear Colleagues
This note is to advise that the closing date for the 2019 Astronomy Grant Round is 6th February 2019. Submissions are accepted from 1st December 2018.
The Astronomy Guidelines for Applicants have been revised and can be found at:
http://www.stfc.ac.uk/research/astronomy-and-space-science/astronomy-space-science-programme/astronomy-research-grants/
Applicants are strongly advised to read the guidelines in detail and contact the office with any queries.
Key points or revisions from the 2018 guidelines have been highlighted in yellow within the document and summarised briefly below for information:
– The structure of proposals – Please ensure the project case for support includes a clearly defined lead applicant and clearly defined roles for all PDRAs, Technicians and Applicants requesting funding.
– The AGP will consider projects as presented, if an Applicant chooses to propose a project with more than one PDRA they should be aware the panel will not recommend partial funding of the project (e.g. for only one PDRA of the two requested, it will either recommend funding or not funding the request).
– Page Limits – All pages (including references) must be written in standard Arial 11pt (or an equivalent regular sans serif universal font). Please note our preferred font is Arial 11pt.
– Facilities Table – this replaces the Je-S facilities section previously used, please see the revised guidance and template on page 8. This should be submitted as part of the case for support.
– Applicant Time – For projects requiring the management of a PDRA the AGP would expect the lead Applicant to request a minimum of 15%FTE support. In projects where two or more applicants have been requested at the same level of FTE a project lead must nonetheless be identified.
New groups submitting their first consolidated grant proposal or those considering a consortium grant submission are advised to inform the Office.
If you have any queries please contact the AGP Programme Manager ([log in to unmask])
http://www.stfc.ac.uk/research/astronomy-and-space-science/astronomy-space-science-programme/astronomy-research-grants/
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Invitation to join Whole Heliosphere and Planetary Interactions campaigns
from Mario M. Bisi [December 14, 2018]
From Sarah Gibson (HAO/NCAR):
It’s solar minimum. In the tradition of Whole Sun Month (1996) and Whole Heliosphere Interval (2008), it’s time for Whole Heliosphere & Planetary Interactions (2019) – WHPI!
Goal? A coordinated observing and modeling effort to characterize the three-dimensional interconnected solar-heliospheric-planetary system. By focussing on specific solar rotations near solar minimum, structures and activity can be unambiguously traced throughout the heliosphere and into planetary space environments.
When? 3 target intervals:
Jul 2019 – Solar eclipse
Sep 2019 – Parker Solar Probe at perihelion
Dec 2019 – Parker Solar Probe Venus flyby
Who? Everyone is welcome – it’s a grassroots effort. Sign up – we will have telecons and workshops to coordinate analyses.
See https://whpi.hao.ucar.edu/ for further details.
https://whpi.hao.ucar.edu/
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Nuggets:
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Two new RHESSI Science Nuggets
from Hugh Hudson [December 6, 2018]
No. 340, “The flight of FOXSI-3”, by Lindsay Glesener and Noriyuki Narukage: single-photon counting and direct imaging across hard and soft energies.
No. 339, “Stellar Flares and Starspots”, by Lauren Doyle: stellar flares don’t spatially coincide with their giant spots.
See http://sprg.ssl.berkeley.edu/~tohban/wiki/index.php/RHESSI_Science_Nuggets
listing the current series, 2008-present, and
http://sprg.ssl.berkeley.edu/~tohban/nuggets/
for the original series, 2005-2008.
We publish these at roughly two-week intervals and welcome contributions,
which should be related, at least loosely, to RHESSI science.
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Meetings/Workshops/Summer Schools:
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Save the Date: “Scintillating Science: Cutting-Edge Science Achieved Through the Observations of Radio Scintillation” Workshop
from Mario M. Bisi [December 14, 2018]
Dear Colleagues.
We would like you to save the dates and draw your attention to our upcoming “Scintillating Science: Cutting-Edge Science Achieved Through the Observations of Radio Scintillation” focussed/specialist workshop which will be held in Hermanus (near Cape Town), South Africa, the week of 15th July 2019. The workshop will cover all aspects of scintillation from the science (including all the domains in which it can be applied, e.g. ionosphere, heliosphere, interstellar) through to engineering concepts/requirements including all aspects of its theory/modelling. Further details will follow early in 2019.
Enjoy the Holidays and see you in 2019!
Best wishes,
Mario M. Bisi (UKRI STFC RAL Space – SOC Co-Chair)
Mike Kosch (SANSA/Lancaster University – SOC Co-Chair/LOC Chair)
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Deadline for NAM session proposals is 7th January
from Anthony Yeates [December 13, 2018]
This is a reminder that the deadline for submitting NAM 2019 parallel session proposals is soon: on 7th Jan 2019. We still have plenty of room for more solar sessions, as well as joint sessions with MIST or other areas of astronomy.
If you have any questions about the science programme, including opportunities for cross-discipline sessions, please contact the SOC at [log in to unmask]
Proposals should be submitted here: https://nam2019.org/session-submission
Best wishes,
Anthony Yeates (on behalf of the SOC and organisers)
https://nam2019.org/session-submission
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RAS Discussion meeting (G) – 8th March 2019 from 10:30 at the RAS Lecture Theatre, Burlington House, London
from Richard Morton [December 12, 2018]
Transitioning Research and Instrument Expertise in Heliophysics into Space Weather Monitoring Capabilities at L1 and L5
The UK has a world-class heliophysics programme in terms of both research and the underpinning instrumentation; this is illustrated by scientific missions such as SOHO, Cluster, STEREO and Solar Orbiter. Investment in these missions has resulted in major advances in our understanding of the physics of our solar system. This experience is crucial for understanding the “space weather” effects of solar-generated activity on human technology and health. Since the UK Government placed extreme space weather on the Risk Register of Civil Emergencies in 2011, the UK has been at the forefront of endeavours to develop an effective approach to space weather mitigation. This includes: establishment of the Space Environment Impact Expert Group to advise Government; formation of the UK Met Office Space Weather Operations Centre; engagement with ESA’s SSA Space Weather programme. The aim of the latter is to launch an operational space weather monitoring mission to the L5 Lagrange point, in conjunction with a US mission to L1. To this end, Phase A/B1 studies of the L5 spacecraft and payload are underway. Both the remote-sensing and in-situ instrument package studies (and one of the parallel system studies) are being led by the UK. It is, hence, timely to assess how best to coordinate the complementary research and operational aspects of the UK’s heliophysics programme. This discussion meeting is aimed at the transitioning of research and instrumental expertise acquired from our recent and on-going space science missions into operational space weather capabilities.
We invite contributions (both oral and posters) from the community. Please send a title and brief abstract to one of the organisers by February 15th.
Details of the meeting can be found at https://ras.ac.uk/events-and-meetings/ras-meetings/transitioning-research-and-instrument-expertise-heliophysics-space. The meeting starts at 10:30 and finishes at 15:30.
Organisers:
Professor Richard A Harrison1, Dr Jackie A Davies1 and Dr Jonny Rae2
1. STFC RAL Space, Harwell Campus, Didcot, Oxfordshire OX11 0QX
2. Mullard Space Science Laboratory, Holbury St Mary, Dorking, Surrey
E-mail – [log in to unmask]
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EGU call for abstracts: ST4.5 Prediction of Solar Flares and Eruptions
from robertus erdelyi [December 11, 2018]
Dear Colleagues,
We would like to draw your attention and invite you to consider submitting an abstract to session ST4.5 in the Space Weather and Space Climate programme group to be held at the EGU General Assembly 2019, April 7–12, in Vienna
Abstract submission: https://meetingorganizer.copernicus.org/EGU2019/abstractsubmission/31920
The abstract deadline is 10 January 2019, 13:00 CET.
ST4.5 Prediction of Solar Flares and Eruptions: Observations, Theory and Modeling
Session details:
The session is intended as a discussion forum for reviewing and improving our current understanding of solar flare occurrence mechanisms and the prediction of flares and eruptions in both observational and modeling settings. In particular, this session will discuss, first, the apparent paradigm shift from simple flare and eruption prediction methods to interdisciplinary, multi-parameter investigations enabled by artificial intelligence (AI) and, second, the current and future synergies between academic and operational sectors in the framework of research to operations (R2O). Solar eruptions cause space weather phenomena that can affect space environment and sometimes impact our infrastructure, causing disruptions to our societal fabric. Prediction of solar flares and eruptions is essential to increase the lead time and the accuracy of space weather forecasts. Synergies are crucial for establishing operational prediction models and for effectively evaluating and validating these models. Such collaborative approaches are motivated by observational advances enabled by space missions (SDO, STEREO, SOHO, Hinode, RHESSI, GOES, Parker Solar Probe, and Solar Orbiter in the near future, etc.), empirical human forecasting for decades, statistical methods, advances in machine- and deep-learning techniques, big-data handling, as well as realistic, data-driven numerical simulations. We solicit contributions on solar flare and eruption prediction, including operational human forecasting, statistical models, AI investigations and state-of-the-art forecast models enabled by numerical simulations, aiming toward future operations. Abstracts on data and performance verification, validation and benchmarking are also welcome.
We look forward to receiving your contributions and thank you very much for your attention.
Sincerely yours, session conveners,
Mamoru Ishii,
Manolis Georgoulis ,
KD Leka,
Naoto Nishizuka
https://www.egu2019.eu
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China-Europe Solar Physics Meeting – Second announcement
from Eduard Kontar [December 6, 2018]
Second announcement
2nd China-Europe Solar Physics Meeting (CESPM)
Advances in Solar and Heliospheric Physics
Hvar, Croatia, May 6 – 10, 2019
http://oh.geof.unizg.hr/CESPM2019
CESPM 2019 meeting is open to colleagues from all countries.
CESPM 2019 is the second meeting between Chinese and European solar physicists and aims to further strengthen the collaboration between European and Chinese scientists, in particular among the young scientists.
The registration for CESPM 2019 is now open and you can register and pay the registration fee by using the on-line form: http://oh.geof.unizg.hr/index.php/en/meetings/cespm2019/registration
The abstract submission form is also available on-line (until 15 January 2019): http://oh.geof.unizg.hr/index.php/en/meetings/cespm2019/abstract
We would like to remind you of important CESPM 2019 deadlines:
Deadline for abstract submission: 15 January 2019 Deadline for early registration: 15 February 2019
Deadline for late abstract submission (poster only): 31 March 2018
We strongly encourage all participants to reserve the accommodation for CESPM 2019 early enough. Although early May is not the main touristic season in Hvar, prices and availability of certain type of accommodation can change. Suncani hvar hotels offer all CESPM 2019 participants accommodation in the hotels Amfora and Pharos with reduced prices (discount code is CESPM2019). All reservations at Amfora and Pharos hotels can be cancelled up to 8 days before the start of reservation and 100% of your payment will be returned to you. More information about the accommodation and link to hotel reservation are given at the bottom of webpage: http://oh.geof.unizg.hr/index.php/en/meetings/cespm2019/travel
http://oh.geof.unizg.hr/CESPM2019
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EWASS – Session on Coronal Mass Ejections, observations and models
from Paolo Pagano [December 5, 2018]
Dear Colleagues,
The European Week of Astronomy and Space Science (24 – 28 June 2019, Lyon) will host a Special Session on “Combining Observations with Models to Derive Coronal Mass Ejections Properties: Where We Stand and What’s Next”
The registration is open and the deadline for abstract submission is March, 3rd 2019.
https://eas.unige.ch/EWASS2019/session.jsp?id=SS20
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AOGS2019 ST20 Solar Flare Forecasting Using Machine Learning
from robertus erdelyi [December 3, 2018]
Dear Colleagues,
We would like to draw your attention to Session ST20: Solar Flare Forecasting Using Machine Learning, of the 16th Annual Meeting of the Asia-Oceania Geosciences Society (AOGS), 28 Jul – 02 Aug, 2019, Singapore.
Please note that the deadline for Abstract Submission is 12 Feb 2019. Submission can be made at:
http://www.asiaoceania.org/aogs2019/public.asp?page=abstract.htm
ST20 Session Description:
Solar flares, one of the most powerful and energetic explosions in our Solar System, are often caused by very abrupt and sudden changes of magnetic field configuration in the Sun’s atmosphere. These violent solar activities could be potentially catastrophic to our satellites, ground-based infrastructure, and even threat the health and life of humans. Therefore, solar flare forecasting has drawn considerable attentions from scientists to governments in recent years.
Besides the physical models of solar flare forecasting, there are more and more successful large data-driven models developed on the basis of machine learning methods. Along with the rise of big data, the advantages and potentials of date-driven models became increasingly relevant. This session solicits presentations focusing on a wide variety of solar flare forecasting models, especially those about data-driven models. We particularly encourage submissions on addressing recent results of solar flare forecasting based on machine learning techniques. We would also welcome submissions addressing the design and operation of numerical forecasting of solar flares, delivering a cutting-edge, more reliable, accurate and near-real time automated solar flare forecasting.
Conveners:
Long Xu (NAOC, China), [log in to unmask]
Robertus Erdelyi (U of Sheffield, UKi), [log in to unmask]
Xin Huang (NAOC, China), [log in to unmask]
http://www.asiaoceania.org/aogs2019/public.asp?page=abstract.htm
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Jobs/Studentships:
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NCAR Advanced Study Program (ASP) and High Altitude Observatory (HAO: Boulder, Colorado) – Postdoc Positions, Application Deadline January 4, 2019
from Richard Morton [December 15, 2018]
The Advanced Study Program (ASP) Postdoctoral Fellowship is an excellent opportunity to conduct independent research at the National Center for Atmospheric Research (NCAR). Early career Ph.D. scientists interested in theoretical, experimental and observational studies of the Sun and Earth’s upper atmosphere are encouraged to apply to the ASP and select the High Altitude Observatory (HAO) as the preferred NCAR unit.
Successful applicants will pursue research, in collaboration with members of NCAR and HAO scientific staff, on a wide range of topics, including study of the Earth’s ionosphere, thermosphere, and magnetosphere; observations and simulations of coronal mass ejections; spectro-polarimetric observations and their interpretation using HAO instrumentation and data inversion tools; probing solar magnetism through observations and modeling; and instrument development.
Postdoctoral fellows are appointed for a maximum of two years, typically beginning in October 2019; some flexibility is possible on the specific times of arrival and departure. Fellowships must begin by January 31, 2020.
The application deadline is January 4, 2019.
See www2.hao.ucar.edu/ for further detail about HAO, and see the ASP website for complete application details: www.asp.ucar.edu/postdocs/prospective-applicants Contact Caitlyn Erdesz ([log in to unmask]) or Matthias Rempel ([log in to unmask]) for further information.
ASP Postdoctoral Fellowships in HAO will be granted on the basis of proven scientific ability and relevance to HAO research programs. Applications are accepted through NCAR ASP (www.asp.ucar.edu). Applicants should specify HAO as the preferred NCAR unit to be considered for ASP fellowships within HAO. Offers will be made no later than April 2019.
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Istituto Ricerche Solari Locarno (IRSOL, Locarno Monti, Switzerland) – Postdoctoral Contract: SOLARNET2 Project
from Richard Morton [December 15, 2018]
The Istituto Ricerche Solari Locarno (IRSOL, Locarno Monti, Switzerland) is currently accepting applications for a postdoctoral position within the project “Measurement for absolute high precision polarimetry” financed by the H2020 project SOLARNET-2.
The aim of the project is to develop a technology that allows to improve the measurement accuracy of the absolute value of polarization signals in high-precision solar spectro-polarimetric observations. A prototype instrument has been developed at IRSOL, which combines a low frequency modulation, effected by rotating a retarder located in front of the telescope, and a high frequency modulation carried out by a high-sensitivity polarimeter located after the telescope. This technology will be developed at IRSOL and will subsequently be tested on larger telescopes such as GREGOR.
The possibility of measuring the absolute value of the polarization with a much higher precision than ever before would represent a major breakthrough in the field of solar spectro-polarimetry, especially regarding the measurement of spectral line polarization.
The IRSOL post-doc successful applicant is expected to lead the project according to the goals of SOLARNET-2 in close interaction with IRSOL staff.
The contract is expected to begin in May 2019 (exact date to be negotiated); it is a two year position with the possibility of applying for renewal.
The announcement, with the information on how to apply, can be found at www.irsol.ch/jobs/
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PhD position in Solar Physics available at Northumbria University
from Richard Morton [December 5, 2018]
The Solar Physics Group at Northumbria University undertakes research in stellar and solar physics, and magnetohydrodynamic phenomenon, specialising in both observations and modelling of plasmas.
We are currently advertising a PhD position in Solar Physics to work with Dr Richard Morton on MHD waves in the Sun’s atmosphere, with the topic of the PhD focusing on the question – ‘Can a stars internal oscillations power their coronae?’. For further details on the project contact Richard ([log in to unmask]) or see:
https://www.findaphd.com/phds/project/can-a-stars-internal-oscillations-power-their-coronae-advert-reference-rdf19-ee-mpee-morton/?p103811
The PhD is a fully funded 3-year position with stipend, and is open to applicants from any country. It is expected that applicants have at least a degree in Mathematics or Physics at the time the position starts and a record of academic excellence. Experience in solar physics research, numerical modelling or astronomical observations would be highly beneficial.
The deadline for applications is Friday 25 January 2019 with an expected start date of 1 October 2019.
https://www.findaphd.com/phds/project/can-a-stars-internal-oscillations-power-their-coronae-advert-reference-rdf19-ee-mpee-morton/?p103811
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