|Published by the STCE - this issue : 11 Jul 2017.
The Solar-Terrestrial Centre of Excellence (STCE) is a collaborative network of the Belgian Institute for Space Aeronomy, the Royal Observatory of Belgium and the Royal Meteorological Institute of Belgium.
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What does a solar observer do on a quiet and sunny Sunday morning? Observing the Sun of course, in particular if one of the largest sunspot groups of the year (so far) is transiting the solar disk. According to the NOAA data (http://www.swpc.noaa.gov/products/solar-region-summary ), active region NOAA 2665 had a surface area of more than 4 times that of the Earth, and it was long enough (front-to-end) to fit 10 Earth's next to each other! The sunspot region was relatively compact, and was reported a naked eye object (using solar eclipse glasses of course: keep it safe!). The Mount Wilson Observatory (http://obs.astro.ucla.edu/images/cur_drw.jpg ) measured the magnetic field strength in the main spot to be more than 3500 times the intensity of the Earth's magnetic field. The region had produced several C-class flares during the early hours of 9 July, as well as 1 M-class ("medium") flare that peaked at 03:18UT.
The PROBA2 team welcomes research proposals for the eighth round of its Guest Investigator program for research based on SWAP and LYRA data analysis by scientists outside the SWAP and LYRA PI-teams. We encourage in particular young post-docs and PhD students to apply, although more senior guest investigators’ proposals are welcome also. In this round we anticipate funding for around five guest investigators or teams who will visit the PROBA2 Science Center at the Royal Observatory of Belgium, in Brussels, between September 2017 and May 2018.
Selected proposers will be invited to spend a few weeks with the PI teams to obtain expert knowledge on the instruments, to participate in the daily commanding of the SWAP and LYRA instruments according to the needs of their data analysis proposal, and to conduct their research.
Guest investigators may be reimbursed for travel, accommodation and living expenses up to a maximum of 5000 euro. Limited support to present the results at an international conference (during the visit at P2SC) can also be considered.
During the selection process, special consideration will be given to young scientists and PhD students, collaborative research teams with members from more than one research institute (funding above the 5000 euro level may be approved for such teams), and to proposals addressing research topics to which SWAP and LYRA are particularly well-suited.
More details about the application process can be found here:
http://proba2.oma.be/EighthGICall, or by emailing firstname.lastname@example.org
Deadline: Proposals must be received by 2017-Sep-24 (23:59 CET)
The PROBA2 team
The week started with active region NOAA 2664 rotating over the west limb. Shortly after, a small unnumbered active region about 15 degrees south of NOAA 2664 produced an M1.3 flare on July 3 peaking at 16:15 UT. See SDO/AIA303 image underneath, and http://www.stce.be/news/390/welcome.html for more info on this event.
Active region NOAA 2665 rotated into view on July 6. It grew quickly in size, number of sunspots and complexity (with beta-gamma magnetic field configuration). The region produced numerous C-class flares and one M1.3 flare peaking at 03:18 UT on July 9. See the other topics in this Newsletter for more information.
No Earth directed Coronal Mass Ejections (CMEs) were observed. Solar energetic protons remained at background levels over the week.
|LOC: approximate heliographic location||TYPE: radio burst type|
|XRAY: X-ray flare class||Cat: Catania sunspot group number|
|OP: optical flare class||NOAA: NOAA active region number|
|10CM: peak 10 cm radio flux|
Solar flare activity fluctuated between very low and moderate during the week.
In order to view the activity of this week in more detail, we suggest to go to the following website from which all the daily (normal and difference) movies can be accessed: http://proba2.oma.be/ssa
This page also lists the recorded flaring events.
A weekly overview movie can be found here (SWAP week 380):
Details about some of this week's events, can be found further below.
If any of the linked movies are unavailable they can be found in the P2SC movie repository here:
The first M-class flare of the week (M1.3) occurred on 2017-Jul-03. The flare and corresponding eruption can be seen on the western limb of the Sun at 16:14 UT in the SWAP image above.
Find a movie of the event here (SWAP movie):
The second M-class flare of the week, also classified as an M1.3, was from NOAA active region 2665 and occurred on 2017-Jul-09 in the south-eastern quadrant of the Sun, as shown in the SWAP image above at 03:36 UT.
Find a movie of the event here (SWAP movie):
The daily Estimated International Sunspot Number (EISN, red curve with shaded error) derived by a simplified method from real-time data from the worldwide SILSO network. It extends the official Sunspot Number from the full processing of the preceding month (green line). The plot shows the last 30 days (about one solar rotation). The horizontal blue line shows the current monthly average, while the green dots give the number of stations included in the calculation of the EISN for each day.
Geomagnetic conditions were quiet to unsettled until July 8 when the fast solar wind from a positive polarity equatorial coronal hole arrived at the Earth. It drove a shock that reached Earth at 23:27 UT on July 8, the speed reached 600 km/s on July 9 with the southward component of the interplanetary magnetic fields reaching -10 nT, with elevated density. Minor storm conditions were recorded both locally (K Dourbes = 5) and at planetary levels (Kp = 5) during July 9.
See the SIDC Space Weather Briefing for images and graphs.
The Space Weather Briefing presented by the forecaster on duty from 3 July till 9 July. It reflects in images and graphs what is written in the Solar and Geomagnetic Activity reports. A.wmv version can be found at http://stce.be/movies/SIDCbriefing-20170709.wmv
The figure shows the time evolution of the Vertical Total Electron Content (VTEC) (in red) during the last week at three locations:
a) in the northern part of Europe(N61°, 5°E)
b) above Brussels(N50.5°, 4.5°E)
c) in the southern part of Europe(N36°, 5°E)
This figure also shows (in grey) the normal ionospheric behaviour expected based on the median VTEC from the 15 previous days.
The VTEC is expressed in TECu (with TECu=10^16 electrons per square meter) and is directly related to the signal propagation delay due to the ionosphere (in figure: delay on GPS L1 frequency).
The Sun's radiation ionizes the Earth's upper atmosphere, the ionosphere, located from about 60km to 1000km above the Earth's surface.The ionization process in the ionosphere produces ions and free electrons. These electrons perturb the propagation of the GNSS (Global Navigation Satellite System) signals by inducing a so-called ionospheric delay.
Start : 2017-07-31 - End : 2017-08-04
This workshop marks the 10th anniversary of the International Heliophysical Year, which led to the genesis of the International Space Weather Initiative. It is organized jointly by the Office for Outer Space Affairs, the National Aeronautics and Space Administration (NASA) and Boston College to highlight the achievements made over the past ten years and to show-case the worldwide development of science, capacity building, and outreach.
The UN Workshops on ISWI have been aimed at providing a global forum for space weather experts from developed and developing countries, including representatives of the major instrument operators and data providers. In particular the Workshop will focus on recent advances made in scientific research by utilizing ISWI instrument data in conjunction with space mission data in adding significant new knowledge on space weather phenomena near Earth and interplanetary space.
The workshop will begin with a high level international forum on the economic and societal effects of extreme space weather. This forum will include keynote speakers from major international organizations followed by a panel session to discuss issues and policies for acknowledging space weather as a global challenge.
The workshop is also held in preparation for UNISPACE+50 in 2018, the 50th anniversary of the first UN Conference on the Exploration and Peaceful Uses of Outer Space (UNISPACE), held in Vienna in 1968. The three components of the Workshop will also help develop a coherent international policy towards an appropriate response to space weather.
Start : 2017-08-19 - End : 2017-08-26
For the thirty-second time since the inception of URSI, Radio Scientists from across the world will get together for the URSI General Assembly and Scientific Symposium. This triennial gathering will take place from 19th to 26th of August 2017, in Montreal, Canada. This conference is a unique opportunity to learn about recent advances in all fields of Radio Science, as covered by all ten URSI Commissions.
Among the different sessions, please note:
* 'Radio Science for Space Weather' Conveners: M. Messerotti, V. Pierrard
* 'Remote Sensing and Modeling of the Earth's Plasmasphere and Plasmapause' Conveners: A. M. Jorgensen, V. Pierrard, B. Heilig
The abstract deadline is 30 January 2017
Start : 2017-08-27 - End : 2017-09-01
The Joint IAPSO-IAMAS-IAGA Assembly, endorsed by the University of Cape Town and the South African Department of Science and Technology, will take place from 27 August to 1 September 2017 at the Cape Town International Convention Centre (CTICC). Several IAGA and IAMAS sessions are of Space Weather interests as well as the joint session 'Space Weather throughout the Solar System: Bringing Data and Models together'.
Start : 2017-09-05 - End : 2017-09-07
The Workshop on Radiation Monitoring for the International Space Station is an annual meeting to discuss the scientific definition of an adequate radiation monitoring package and its use by the scientific community on the ISS. Types of instruments and research topics need to be defined in order to optimise the radiation safety of the ISS crew.
Start : 2017-11-06 - End : 2017-11-10
Jean-Louis Steinbeg has been one of the major pioneers in radioastronomy. Co-founder of the NanÃ§ay Observatory, he has actively participated to, an inspired a large number of radio instruments on many international space missions. Jean-Louis Steinberg is the founder of the Space Radioastronomy laboratory of the Paris Observatory in 1963. Later on, this laboratory widened its science interests and became the DESPA (1971) and then the current LESIA (2002) which is one of the major space sciences laboratories in France. The aim of this workshop is to cover the science topics which Jean-Louis Steinberg has promoted during his career, focusing on Solar, Heliospheric & Magnetospheric radioastronomy & physics. This will be done by covering both observations from either ground facilities (NDA, RH, LOFAR, Artemis etc ...) or space missions (ISSEE, Ulysses, WIND, CLUSTER, STEREO, CASSINI, JUNO etc ...) and models/theories. A series of invited talks is also foreseen to cover the new developments in the discipline which may come with the future facilities such as Solar Orbiter, Solar Probe Plus, JUICE, JUNO, LOFAR+, SKA etc ....
This workshop will also be the opportunity to remember both the extraordinary personal & professional lifes of Jean-Louis Steinberg especially for new generation of scientists. At the occasion of this workshop it is also expected that the Building 16 (historical Space Sciences building) on the Meudon campus will be renamed "Building Jean-Louis Steinberg".
Start : 2017-11-27 - End : 2017-12-01
The ESWW is the main annual event in the European Space Weather calendar. It is the European forum for Space Weather as proven by the high attendance to the past editions. The agenda will be composed of plenary/parallel sessions, working meetings and dedicated events for service end-users. The ESWW will again adopt the central aim of bringing together the diverse groups in Europe working on different aspects of Space Weather.