The Electronic Newsletter of the
Solar Physics Division
American Astronomical Society
Volume 2016 Number 16
Aimee Norton, Editor
15 August 2016
- CESRA New Highlights
- SDO/HMI Magnetograms – New Synoptic Data Products
- SunPy 0.7 Released
- UKSP Nuggets of 2016 so far
- The Joint Next Generation Solar Physics Mission’s Science Objectives Team (NGSPM-SOT)
- Employment Opportunities
- Postdoctoral Position in the SOLAR-C Project Office at the National Astronomical Observatory of Japan
- Editor’s Notes
CESRA New Highlights
02 Aug 2016
Solar radio science highlight was just published: “Observation of a Quasi-periodic Pulsation in Hard X-Ray, Radio, and Extreme-ultraviolet Wavelengths”, by Pankaj Kumar, Valery M. Nakariakov and Kyung-Suk Cho. cesra.net/?p=646
The Highlight of Solar Radio Physics or CESRA Nugget allows you to publish fresh research to keep CESRA community informed and up-to-date. These are short communications written in the language accessible to a non-expert in the specific area.
SDO/HMI Magnetograms – New Synoptic Data Products
03 August 2016
The NSO Integrated Synoptic Program (NISP) is pleased to announce the availability of new synoptic data products based on SDO/HMI data. These include both pseudo-radial flux maps derived from the longitudinal HMI m_720s magnetograms and 3-component (radial, poloidal, toroidal) vector flux maps derived from the vector HMI b_720s magnetograms. Two versions of the vector component maps reflect different options for the disambiguation of the quiet-sun (‘random’ and ‘radial-acute’). This dataset covers the period May 2010 – January 2016, is described in the NSO Technical Report NSO/NISP-2016-002 (arxiv.org/abs/1605.03500), and can be accessed from the NISP/SOLIS project website (solis.nso.edu) or directly via ftp (solis.nso.edu/HMI/).
SunPy 0.7 Released
08 Aug 2016
The SunPy project is pleased to announce the latest release of the SunPy library. This release is the result of 10 months of work by 27 people. Installation instructions can be found here. The highlights of this release are:
- The new subpackage
sunpy.coordinatesenabling the transformation between Helioprojective, Heliocentric and Heliographic coordinate systems. It also makes it easy to calculate and convert co-ordinates from different viewpoints such as SDO and STEREO.
- A code gallery demonstrating common solar physics tasks using SunPy.
Mapwhich make it easier to overplot rectangles and contours on Map plots.
- Support for data masking in
- Python 3.4 and 3.5 support. We recommend that all new users install Python 3 and that existing users consider upgrading as soon as possible.
The full list of changes and bug fixes can be found here.
If you have questions about using Python for solar physics or want to get involved with the project see our help page for ways to get involved with the community.
UKSP Nuggets of 2016 so far
11 Aug 2016
UKSP nuggets are monthly short articles highlighting solar physics research in the UK: www.uksolphys.org/uksp-nuggets/
70. Magnetic Flux Cancellation in Ellerman Bombs by Aaron Reid & Mihalis Mathioudakis (QUB)
A nice CRISP view of small scale flux cancellation in Ellerman bombs
69. Low-Coronal Sources of “Stealth” Coronal Mass Ejections by Nathalia Alzate & Huw Morgan (Aberystwyth University)
Image processing reveals the Not-So-Stealthy Sun.
68. Random bursty perturbations leading to wave-like characteristics in the corona by Ding Yuan and Robert W. Walsh (UCLan), Jiangtao Su (NAOC), Fangran Jiao (Shandong University)
Do coronal oscillations imply a periodic driver?
67. Solar Physics with SunPy by Stuart Mumford & Andrew Leonard (Sheffield & on behalf of SunPy)
The future of solar physics data analysis?
66. Evidence for similar processes occurring in stellar superflares and solar flares by Chloe Pugh, Valery Nakariakov & Anne-Marie Broomhall (Warwick)
Solar-like behaviour in stellar super flare lightcurves
65. EUV irradiances across a solar cycle by Giulio Del Zanna (Cambridge)
SOHO’s CDS spectrometer can be used to study the Sun’s impact on the Earth
64. 3D Electron Density Distributions in the Solar Corona during Solar Minimum by Judith de Patoul and Claire Foullon (Exeter) and Pete Riley (Predictive Science)
A new tomographic method promises better solar wind models
The Joint Next Generation Solar Physics Mission’s Science Objectives Team (NGSPM-SOT)
11 Aug 2016
The joint Next Generation Solar Physics Mission’s Science Objectives Team (NGSPM-SOT) has been formed based on the agreement among NASA, JAXA and ESA for the study of a possible multilateral solar physics mission concept. The objectives of this NGSPM-SOT are to a) develop the science goals for NGSPM, b) assess how these scientific goals are aligned with JAXA, ESA and NASA agency priorities, c) assess the required measurements necessary to meet the science goals, d) assess the top-level observational (mission design) strategy for the NGSP mission to accomplish the scientific goals, e) identify the minimum performance for the mission systems, and f) deliver a science report that supports the generation of documents suitable for input into any future joint Announcement of Opportunity or Call for Missions. The final report will be delivered to the agencies in summer next year.
The team members consist of 4 NASA appointed members (David McKenzie, Ted Tarbell, John Raymond, Sara Gibson), 4 ESA appointed members (Louis R. Bellot Rubio, Mats Carlsson, Lyndsay Fletcher, Sami Solanki) and 4 JAXA appointed members (Kiyoshi Ichimoto, Kanya Kusano, Hirohisa Hara, Toshifumi Shimizu). Shimizu chairs the team. All the members are points of contacts with the worldwide community; they will engage with the community, and collect ideas to build up the best optimized science goals and mission design options.
The team has started to review the Solar-C science objectives and will develop the revised set of science goals for the next generation solar physics in a couple of months. At the Solar-C science meeting in Nagoya, Japan on September 10 (attached to Hinode-10, hinode.stelab.nagoya-u.ac.jp/Hinode10/), the team will introduce its activity so far to the participants of the meeting. To develop the best science goals, the meeting will be a good opportunity to get feedback from the community.
Postdoctoral Position in the SOLAR-C Project Office at the National Astronomical Observatory of Japan
04 Aug 2016
The National Astronomical Observatory invites applications for a postdoctoral position in the SOLAR-C Project Office. The Project Office is executing the research and development activity for the future space solar physics mission in cooperation with ISAS/JAXA. (1) Research topics on the sounding-rocket experiment CLASP (Chromospheric Lyman-Alpha Spectro-Polarimeter: hinode.nao.ac.jp/KakenS/index_e.shtml) and on a balloon-borne experiment Sunrise-3 (the research and payload development on the CLASP-2 and Sunrise-3 ). (2) Research topics in association with the future satellite project SOLAR-C: (hinode.nao.ac.jp/SOLAR-C/index_e.html : the research and development of the SOLAR-C science payload, research on the methodology to derive magnetic fields from expected polarimetric data, etc.)
The position is available from 1 November 2016 (starting date negotiable) and is offered for three years. For the detail, please visit the following website: www.nao.ac.jp/en/job-vacancy.html
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