Published by the STCE - this issue : 18 Aug 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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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 385):
http://proba2.oma.be/swap/data/mpg/movies/weekly_movies/weekly_movie_2017_08_07.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/
Over the past week solar activity has been very low. No significant flares have been recorded.
No Earth directed Coronal Mass Ejections (CMEs) have been detected.
The greater than 10MeV proton flux remained at background levels.
The solar wind speed decreased from around 600 km/s at the beginning of the week to around 350 km/s in the middle of the week before slowly increasing again to around 700 km/s at the end of the week.
Check the graph below showing the solar wind speed measured by the spacecraft DSCOVR at the L1 point.
The total magnetic field strength (Bt) fluctuated between 5 and 10 nT. The Bz component fluctuated around 0 nT but was mainly positive.
Check the graph below showing Bt and Bz measured by the spacecraft DSCOVR at the L1 point.
Geomagnetic conditions ranged between Kp index 0-3 (NOAA) and local K index 0-3 (Dourbes).
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 : 2017-08-19 - 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/