Published by the STCE - this issue : 19 May 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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Dear Colleagues
Dear interested ESWW14 Fair Participants
We invite you to participate with a fair stand at the ESWW14, the 14th European Space Weather Week to be held in Ostend, Belgium on 2017. As in the past, this year's ESWW will include a Wednesday Space Weather fair, where users and service providers will have the opportunity to interact in an informal working environment. The fair is an opportunity for academics, scientists, and companies, non-academics, clients, and service providers to profile their activities and learn what there is to know in the field of Space Weather. A science cafe follows the fair.
The fair event will be held on Wednesday Nov 29, 17:00 - 18:30
Information for stand holders: http://www.stce.be/esww14/program/infofair.php
Check here to request a stand: http://www.stce.be/esww14/registration.php
A Wednesday booth is included in a full week conference fee.
We are looking forward for your fair contribution.
Mauro Messerotti and Petra Vanlommel, on behalf of the ESWW PC
Solar flare activity remained very low 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 372):
http://proba2.oma.be/swap/data/mpg/movies/weekly_movies/weekly_movie_2017_05_08.mp4
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:
http://proba2.oma.be/swap/data/mpg/movies/
During this week solar activity was extremely low with no C-class, and even B-class flares, reported.
The only wide CME observed this week was faint and slow partial halo CME, with projected speed of about 140 km/s and angular width of about 170 degree, observed on May 13. The CME, first seen in the SOHO LASCO C2 field of view at about 22:00 UT, seem to be associated with the faint filament eruption from the southern solar hemisphere. The bulk of the CME mass was directed southward of the Sun-Earth line, and only the glancing blow from the associated CME-driven shock wave might be expected.
Elongated equatorial coronal hole, with the extent to the both southern and northern hemisphere, reached central meridian in the morning of May 12.
During the whole week the Earth was inside a slow solar wind fluctuating between 300 and 440 km/s. The interplanetary magnetic field magnitude had values between 2 and 12 nT.
At about 16:00 UT on May 09, a sudden change of the phi angle, simultaneously with the interplanetary magnetic field magnitude increase (from about 3nT to the value of 8nT) was observed, indicating the crossing of the sector boundary.
On the last day of the week, May 14 at about 10 UT, the increase of the interplanetary magnetic field magnitude (with oscillations of the Bz component of the interplanetary magnetic field) was observed simultaneously with the decrease of density and slow increase of the solar wind speed and temperature. All this indicate arrival of the fast solar wind associated with the elongated equatorial coronal hole.
The geomagnetic conditions were quiet to unsettled during the whole week.
The Monday SIDC space weather briefing:
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.
See http://stce.be/newsletter/GNSS_final.pdf for some more explanations ; for detailed information, see http://gnss.be/ionosphere_tutorial.php
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.
Website: https://iswi2017.bc.edu/
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
Website: http://www.ursi2017.org
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'.
Website:
http://iapso-iamas-iaga2017.com/index.php
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.
Website: http://wrmiss.org/
Start : 2017-11-06 - End : 2017-11-10
Jean-Louis Steinbeg has been one of the major pioneers in
radioastronomy. Co-founder of the Nançay 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".
Website:
https://jlsworkshop.sciencesconf.org/
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.
Website:
http://www.stce.be/esww14/