Published by the STCE - this issue : 17 Jun 2016. 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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An event to look forward for the Space Weather Community is the annual European Space Weather Week, now in it's 13th edition.
Space Weather does have an impact on our society which is a network of industries and economy intertwined with science and space weather services. At ESWW13 we try to make the perfect cocktail of people and knowledge that makes us Space Weather proof and strengtens our safety net. Cheers!
Check the poster on http://www.stce.be/esww13/
The 2016 edition of the STCE annual meeting led us along Roof Top Science, Cosmic Rays, 10years STCE Happy Birthday cake and a launch to Wuthering Heights.
An impression of a successful day
or check http://www.stce.be/sites/default/files/field/image/Annualmeeting_lr.gif
Solar flare activity fluctuated between very low and 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 324).
http://proba2.oma.be/swap/data/mpg/movies/weekly_movies/weekly_movie_2016_06_06.mp4
Details about some of this week's events, can be found further below.
An eruption was observed by SWAP on the east limb of the Sun on 2016Jun10 at 03:25 UT
Find a movie of the events here (SWAP movie)
http://proba2.oma.be/swap/data/mpg/movies/20160610_swap_movie.mp4
An eruption was observed by SWAP on the east limb of the Sun on 2016Jun11 at 22:26 UT
Find a movie of the events here (SWAP movie)
http://proba2.oma.be/swap/data/mpg/movies/20160611_swap_movie.mp4
The week started with a spotless Sun and the GOES X ray background at B1 level. Beta region NOAA AR 2552 appeared on Wednesday June 8 and was the source of all 4 C flares later this week.
Following the passage of a coronal hole high speed stream in the weekend before, Kp reached one interval of minor geomagnetic storm (Kp=6) on Monday June 6. A sector boundary crossing (SBC) from negative to positive was observed in ACE data at 11:23 UT on June 10. From around 20h UT onwards, a high speed stream associated with a positive coronal hole (CH) gradually increased solar wind speeds from 360 km/s to a maximum of about 600 km/s.
The magnitude of the Interplanetary Magnetic Field (IMF) rose from about 4 to 14 nT. The geomagnetic response did not exceed active levels.
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 : 2016-06-27 - End : 2016-07-01
Website:
http://www.issibern.ch/program/workshops.html
Start : 2016-10-24 - End : 2016-10-28
This event brings together solar, heliospheric, magnetospheric,
and ionospheric communities to discuss the current state and future
challenges in global modelling of the entire space weather chain.
Major developments in forecasting space weather, and understanding
the effects of solar eruptions requires increased communication and
collaboration of these often rather distinct communities. We
welcome submissions from these modelling communities and also
synergetic studies utilising both observations and numerical
models.
Website:
https://pnst.ias.u-psud.fr/sites/pnst/files/global_modelling_space_weather_oct2016.pdf
Start : 2016-11-14 - End : 2016-11-18
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/esww13/
Start : 2017-04-03 - End : 2017-04-06
This event will be hosted by the Instituto de Astrofisica de
Andalucia - CSIC. Please mind that on April 7th the 20th SWT
meeting will take place at the same venue.
Website: Unkown
Presentation given at the Cosmic Rays workshop
Check https://events.oma.be/indico/event/10/
http://www.spaceweather.eu/en/repository/show?id=602
Presentation given at the Cosmic Rays workshop
check https://events.oma.be/indico/event/10/
http://www.spaceweather.eu/en/repository/show?id=603
Presentation given at the Cosmic Rays workshop
check https://events.oma.be/indico/event/10/
http://www.spaceweather.eu/en/repository/show?id=604
Presentation given at the Cosmic Rays workshop
check https://events.oma.be/indico/event/10/
http://www.spaceweather.eu/en/repository/show?id=605
Presentation given at the Cosmic Rays workshop
check https://events.oma.be/indico/event/10/
http://www.spaceweather.eu/en/repository/show?id=606
Presentation given at the Cosmic Rays workshop
check https://events.oma.be/indico/event/10/
http://www.spaceweather.eu/en/repository/show?id=607