Published by the STCE - this issue : 20 Dec 2012. 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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With 2012 nearing its end, it may be a good time to have a quick review of some of the more spectacular events that the Sun produced this year. Though Solar Cycle 24 (SC24) certainly has been weak so far, solar activity was quite interesting at times with the Sun producing some truly amazing events.
A chronological list of 12 of these events can be found underneath. Using Helioviewer and JHelioviewer, a movie at http://www.youtube.com/watch?v=aO5IZSyYTEM was created containing a few clips of each event. Usually, SDO-images (http://sdo.gsfc.nasa.gov/ ) were used, occasionally supplemented with imagery from STEREO (http://stereo.gsfc.nasa.gov/ ) , PROBA2 (http://proba2.oma.be/ ) , SOHO (http://sohowww.nascom.nasa.gov/ ) and GOES/SXI (http://www.swpc.noaa.gov/sxi/index.html ).
As this concerns punctual events on the Sun, one will not find here clips from the total solar eclipse, the Venus transit, or the ongoing magnetic reversal at the Sun's poles. Even then, it was still quite hard to pick these 12 events from all other eruptions, so no attempt was being made to rank them in another way. We leave it up to the reader to determine which is the fairest of them all.
Merry Christmas and a Happy New Year!
The week was not especially exciting if it concerns flaring activity. The background X-ray radiation stayed at the bottom of the B-level. 3 C-flares occurred. On Dec 10 and 11, NOAA AR 1630 (N19W24) did the flaring honours including a C5.5 flare on Dec 10. On Dec 12, the flare torch was passed to NOAA AR 1629, a neighbouring active region, resulting in a C5.7 flare. A newly emerged sunspot group Catania 47 - NOAA active region 1632, trailing AR 1630 and 1629, wrapped up with a third, moderate C1.2-flare.
On Dec 10, a filament from behind the east limb erupted. CACTus sent out a Halo CME alert but it was catalogued as back-sided.
A filament in the SW quadrant of the solar disk erupted late Dec 13-early Dec 14. Images from SDO/AIA 193 and 304 show that the eruption started on Dec 13, 22UT. The lower part, i.e. higher latitude and farther from the west limb, of the filament erupted first. By Dec 14, 3UT the part of the filament situated near the west limb had also erupted.
The solar wind speed stayed below 350 km/s until Dec 15. From that moment, the speed increased slowly reaching 430 km/s on Dec 16.
Solar Activity
It was - again - a very calm week on the Sun. 7 C-level flares were recorded during the whole 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.
Despite the low level of flaring activity, several interesting events occurred. A movie with this week’s filament/prominence activities can be found here: http://proba2.oma.be/swap/data/mpg/movies/campaign_movies/2012_12_10_00_00_19_2012_12_16_22_52_55_SWAP_174__AIA_304-hq%282%29.mp4.
Some of them are presented below:
C5.7 flare eruption ‘on disk’, eruption on the NNW limb, followed by an eruption on the SE limb (the latter is not visible on this picture, but see movie here: http://proba2.oma.be/swap/data/mpg/movies/campaign_movies/20121212_3Consecutive_Eruptions_swap_diff.mp4)
A movie of the above event can be found here: http://proba2.oma.be/swap/data/mpg/movies/campaign_movies/2012_12_13_23_00_31_2012_12_14_04_58_43_SWAP_174__AIA_304-hq.mp4.
Barely visible with SWAP, a large filaprom erupted on Dec 14, around 08:00, North East quadrant. It was quite spectacular in AIA/304 (see helioviewer.org)
European Space Weather Landscape: Current Perspectives and Requirements for the Future
http://www.spaceweather.eu/en/repository/show?id=340
European Space Weather Landscape: Current Perspectives and Requirements for the Future
http://www.spaceweather.eu/en/repository/show?id=341
European Space Weather Landscape: Current Perspectives and Requirements for the Future
http://www.spaceweather.eu/en/repository/show?id=342
European Space Weather Landscape: Current Perspectives and Requirements for the Future
http://www.spaceweather.eu/en/repository/show?id=343
European Space Weather Landscape: Current Perspectives and Requirements for the Future
http://www.spaceweather.eu/en/repository/show?id=344
European Space Weather Landscape: Current Perspectives and Requirements for the Future
http://www.spaceweather.eu/en/repository/show?id=345
European Space Weather Landscape: Current Perspectives and Requirements for the Future
http://www.spaceweather.eu/en/repository/show?id=346
European Space Weather Landscape: Current Perspectives and Requirements for the Future
http://www.spaceweather.eu/en/repository/show?id=347
European Space Weather Landscape: Current Perspectives and Requirements for the Future
http://www.spaceweather.eu/en/repository/show?id=348
Innovations and Key Challenges in Space Weather Science
http://www.spaceweather.eu/en/repository/show?id=349
Innovations and Key Challenges in Space Weather Science
http://www.spaceweather.eu/en/repository/show?id=350
Innovations and Key Challenges in Space Weather Science
http://www.spaceweather.eu/en/repository/show?id=351
Innovations and Key Challenges in Space Weather Science
http://www.spaceweather.eu/en/repository/show?id=352
Innovations and Key Challenges in Space Weather Science
http://www.spaceweather.eu/en/repository/show?id=353
Innovations and Key Challenges in Space Weather Science
http://www.spaceweather.eu/en/repository/show?id=354
Innovations and Key Challenges in Space Weather Science
http://www.spaceweather.eu/en/repository/show?id=355
Innovations and Key Challenges in Space Weather Science
http://www.spaceweather.eu/en/repository/show?id=356
Innovations and Key Challenges in Space Weather Science
http://www.spaceweather.eu/en/repository/show?id=357
Solar Variability Effects on Climate
http://www.spaceweather.eu/en/repository/show?id=358
Solar Variability Effects on Climate
http://www.spaceweather.eu/en/repository/show?id=359
Solar Variability Effects on Climate
http://www.spaceweather.eu/en/repository/show?id=360
Solar Variability Effects on Climate
http://www.spaceweather.eu/en/repository/show?id=361
Solar Variability Effects on Climate
http://www.spaceweather.eu/en/repository/show?id=362
Solar Variability Effects on Climate
http://www.spaceweather.eu/en/repository/show?id=363
Solar Variability Effects on Climate
http://www.spaceweather.eu/en/repository/show?id=364
Coupled Space Weather Modelling
http://www.spaceweather.eu/en/repository/show?id=365
Coupled Space Weather Modelling
http://www.spaceweather.eu/en/repository/show?id=366
Coupled Space Weather Modelling
http://www.spaceweather.eu/en/repository/show?id=367
Coupled Space Weather Modelling
http://www.spaceweather.eu/en/repository/show?id=368
Coupled Space Weather Modelling
http://www.spaceweather.eu/en/repository/show?id=369
Coupled Space Weather Modelling
http://www.spaceweather.eu/en/repository/show?id=370
Coupled Space Weather Modelling
http://www.spaceweather.eu/en/repository/show?id=371
Coupled Space Weather Modelling
http://www.spaceweather.eu/en/repository/show?id=372
Coupled Space Weather Modelling
http://www.spaceweather.eu/en/repository/show?id=373
Spacecraft Operations and Space Weather
http://www.spaceweather.eu/en/repository/show?id=374
Spacecraft Operations and Space Weather
http://www.spaceweather.eu/en/repository/show?id=375
Spacecraft Operations and Space Weather
http://www.spaceweather.eu/en/repository/show?id=376
Spacecraft Operations and Space Weather
http://www.spaceweather.eu/en/repository/show?id=377
Spacecraft Operations and Space Weather
http://www.spaceweather.eu/en/repository/show?id=378
Spacecraft Operations and Space Weather
http://www.spaceweather.eu/en/repository/show?id=379
Space Weather in the Solar System
http://www.spaceweather.eu/en/repository/show?id=381
Space Weather in the Solar System
http://www.spaceweather.eu/en/repository/show?id=382
Space Weather in the Solar System
http://www.spaceweather.eu/en/repository/show?id=383
Space Weather in the Solar System
http://www.spaceweather.eu/en/repository/show?id=384
Space Weather in the Solar System
http://www.spaceweather.eu/en/repository/show?id=385
Space Weather in the Solar System
http://www.spaceweather.eu/en/repository/show?id=386
Space Weather in the Solar System
http://www.spaceweather.eu/en/repository/show?id=387
COST ES0803 Final Results
http://www.spaceweather.eu/en/repository/show?id=388
COST ES0803 Final Results
http://www.spaceweather.eu/en/repository/show?id=389
COST ES0803 Final Results
http://www.spaceweather.eu/en/repository/show?id=390
COST ES0803 Final Results
http://www.spaceweather.eu/en/repository/show?id=391
COST ES0803 Final Results
http://www.spaceweather.eu/en/repository/show?id=392
COST ES0803 Final Results
http://www.spaceweather.eu/en/repository/show?id=393
COST ES0803 Final Results
http://www.spaceweather.eu/en/repository/show?id=394
COST ES0803 Final Results
http://www.spaceweather.eu/en/repository/show?id=395
COST ES0803 Final Results
http://www.spaceweather.eu/en/repository/show?id=396
Spacecraft Operations and Space Weather
http://www.spaceweather.eu/en/repository/show?id=397
ESWW9 Splinter wrap up
http://www.spaceweather.eu/en/repository/show?id=398
Presentation given at the conference 'Solar and Heliospheric influences on the geospace', Bucharest, Romania in the session 'Education, dissemination, outreach'
http://www.spaceweather.eu/en/repository/show?id=399
A presentation given for the members of the public observatory 'Armand Pien', Gent: 60 participants.
http://www.spaceweather.eu/en/repository/show?id=400
On October 27, this Dutch presentation was given about Solar Cycle 24 for a group of amateur astronomers, namely the Workgroup Sun of the VVS and the NVWS, 20 people.
http://www.spaceweather.eu/en/repository/show?id=401
http://www.spaceweather.eu/en/repository/show?id=402
Start : 2013-01-14 - End : 2013-01-16
SWIFF (Space Weather Integrated Forecasting Framework), a
project funded by the European Commission through the Framework
Program 7, aims to develop mathematical models and computational
methods especially designed to handle the multiple physics and the
multiple scales characteristic of space weather phenomena (for more
information see
). SWIFF Project reaches two years on
January 31, 2013. Hence, the aim of the Conference will be to
review the progress in those two years and plan for the next last
year of activity.
http://www.swiff.eu/
Meeting Registration - DEADLINE EXTENDED until December 30:
deadlines for meeting registration and abstract submission are now
extended until December 30, 2012!
Registration Fee is €140.00, including: access
to all sessions, coffee breaks, and the Social Dinner. The Social
Activity (visit to the Egyptian Museum) and lunches are not
included in the fee. We kindly ask you to pay the registration fee
via the on-line form as soon as possible. Late (on-site)
registrations and payments will also be accepted (via credit card
only), but we kindly ask you to make the fee payment before the
deadline of December 30. Official receipts of Registration Fee
payments will be provided at the Meeting desk.
During the registration, we ask you to preliminary state if you
intend to participate also to the Social Activity and/or to the
Social Dinner, just to have a first idea of the total number of
people. Payment for the Social Activity (approximately
€12, depending on the final number of
participants) will be required on-site (by cash only). Receipts
will be provided.
For any further information please contact the Scientific
Organizing Committee ( swiff2_soc@oato.inaf.it) or the Local
Organizing Committee ( swiff2_loc@oato.inaf.it).
Website:
http://swiff2.oato.inaf.it/
Start : 2013-01-14 - End : 2013-01-17
The Atacama Large Millimeter/submillimeter Array (ALMA), an
international partnership of Europe, North America and East Asia in
cooperation with the Republic of Chile, is the largest astronomical
project in existence.
The workshop aims to bring together the ALMA-minded solar
community to discuss solar observational issues with ALMA, solar
science and planned observations with ALMA, and the planning of
solar ALMA observations.
Th workshop is hosted by Astronomy & Astrophysics Group,
and will take place in School of Physics and Astronomy, University
of Glasgow, Room 323, Kelvin Building.
Website:
http://www.astro.gla.ac.uk/~eduard/solarALMA/
Start : 2013-02-04 - End : 2013-02-08
Helioseismology provides tools for imaging structures and mass
flows below the solar surface, and is becoming an essential
technique for understanding the dynamics of solar activities and
developing physics-based forecasts of the solar cycle, emerging
active regions and energy release events. A better understanding is
needed to unravel the effects of the complex interactions of solar
oscillations with the turbulent magnetized plasma
on global and local helioseismology
diagnostics. These effects are particularly challenging in regions
of strong magnetic fields. Numerical simulations of solar MHD waves
and turbulent dynamics give important insights into the complicated
wave and turbulence physics, and provide synthetic data for
verification and validation of helioseismology methods and
results.
The goals of this workshop are to discuss and stimulate further
development of helioseismology methods, solar interior models, and
realistic numerical simulations. These goals are particularly
important for analysis of the continuous data flow from the Solar
Dynamics Observatory, development and verification of
helioseismology methods, and for theoretical interpretation of
observations and inversion results.
Website:
http://sun.stanford.edu/LWS2013/
Start : 2013-02-11 - End : 2013-02-15
More information follows later.
Website:
http://www.spaceclimate.fi/
Start : 2013-02-28 - End : 2013-02-28
On February 28th, 2013 the AFFECTS team organises an
international user workshop at the Royal Observatory of Belgium in
Brussels.
At the workshop there will be a demonstration of all AFFECTS
space weather
products:
* Near real time dimming and EIT
wave detection
* 3D CME
analysis tool
* Coronal analysis tool
* CME
& solar wind
arrival and impact forecast
tool
* Flare, CME
, geomagnetic, auroral, ionospheric
forecasts & alerts
* Forecast of perturbed TEC
* Solar activity and space weather
timelines viewer
To register, please send an e-mail incl. your full name,
institution, e-mail and (institutional) address to
.
Dörte Dannemann
Website:
http://www.affects-fp7.eu/news-events/user-ws/
Start : 2013-03-04 - End : 2013-03-06
Geant4 Space Users' Workshop -G4SUW- is focused on new
results on space radiation interaction with components, sensors and
shielding analysis, as well as on Geant4-based tools and
developments applicable to space missions.
The Geant4 particle transport toolkit is jointly developed by a
world-wide collaboration and is intended for a wide range of
applications in HEP, medical field, and space physics and
engineering. In recent years, space and astrophysics has become a
significant user category, with applications ranging from
instrument and detector response verification to space radiation
shielding optimization, component effects, support of scientific
studies, and analysis of biological effects.
Main topics for next G4SUW will include:
* Single Event Effects (SEE) simulation.Geant4-TCAD
coupling.
* Microdosimetry.
* Planetary exploration applications.
* Space electronics and science detectors.
* Simulation of astronaut radiation hazards.
* Interfaces and tools to space environment analysis tools such
as SPENVIS.
* Cosmic ray magnetospheric propagation analysis.
* Large-scale simulations requiring event biasing and/or GRID
capabilities.
* General shielding optimization applications.
Website:
http://www.inta.es/g4suw2013/index.html
Start : 2013-04-07 - End : 2013-04-12
The EGU General Assembly 2013 will bring together geoscientists
from all over the world into one meeting covering all disciplines
of the Earth, Planetary and Space Sciences. Especially for young
scientists, it is the aim of the EGU to provide a forum where they
can present their work and discuss their ideas with experts in all
fields of geosciences. The EGU is looking forward to cordially
welcoming you in Vienna.
Website:
http://www.egu2013.eu/home.html
Start : 2013-04-08 - End : 2013-04-12
The most recent solar minimum, solar cycle 23-24 minimum, was
unusually long (266 spotless days in 2008, the most since 1913),
and the magnetic field at the solar poles was approximately 40%
weaker than the last cycle; and unusually complex (the solar wind
was characterized by a warped
heliospheric current sheet, HCS, and fast-wind
streams at low latitudes: the
fast-wind
threads the ecliptic
more commonly in 2008 than 1996.)
This complexity resulted in many effects observed from Sun to
Earth, with many observations indicating unusual conditions on the
Sun, in the heliosphere
, and in the magnetosphere
, ionosphere
, and upper atmosphere of the
Earth.
This remarkable set of conditions provide the scientific
community with an exceptional opportunity to assess the nature and
structure of a very quiet Sun, and an upper atmosphere relatively
devoid of solar influences, helping to provide a better
understanding of the relative roles of solar activity and internal
variability in the dynamics of the Earth's upper atmosphere and
ionosphere
. Such an understanding requires a
multidisciplinary approach.
The main goal of the conference is to bring together the solar,
heliospheric, magnetospheric, upper atmosphere, and ionospheric
communities to debate and discuss interdisciplinary work and reach
a better understanding of the nature and structure of a very quiet
Sun, and of an upper atmosphere relatively devoid of solar
influences, and in doing so, to help clarify the role of solar
activity in the dynamics and variability of the Earth's upper
atmosphere and ionosphere
relative to the internal
variations.
Website:
http://chapman.agu.org/solarminimum/
Start : 2013-05-06 - End : 2013-05-10
In the last 50 years, helioseismology has made significant
contributions to the knowledge of the Sun's interior physics
and has led the way to asteroseismology. We have now reached an era
where more sophisticated questions are being asked to understand
the subtle properties of the Sun and other stars due to the
synoptic and high-resolution observations available from BISON,
GONG and space missions such as SOHO
, SDO, CoRot and Kepler.
On this occasion, a workshop on the theme of '50 years of the
seismology of the Sun and stars' is being organized to reflect the
progress that has been made as well as to focus on future goals. We
plan to bring together helio- and asteroseismologists, theorists
and observers in a journey that will take us from the interior of
the Sun and its magnetism towards the structure of distant stars
and activity cycles.
Website:
http://www.nso.edu/workshops/2013
Start : 2013-06-23 - End : 2013-06-29
The 2013 ILWS Science Workshop will take place June 23-29, 2013
in Irkutsk, Russia and will be hosted by the Institute of
Solar-Terrestrial Physics of the Russian Academy of Sciences
Website:
http://en.iszf.irk.ru/ILWS_2013
Start : 2013-07-12 - End : 2013-07-19
Applications are invited for the 2013 Heliophysics Summer
School, which will be held in beautiful Boulder, Colorado. We are
seeking students and undergraduate level teachers and instructors
to join us this coming summer for a unique professional experience.
Students and teachers will learn about the exciting science of
heliophysics as a broad, coherent discipline that reaches in space
from the Earth's troposphere to the depths of the Sun, and in
time from the formation of the solar system to the distant future.
At the same time, a goal of the Summer School is for the group of
instructors to develop materials from Heliophysics that can be
applied in their classes.
The Heliophysics Summer School focuses on the physics of space
weather events that start at the Sun and influence atmospheres,
ionospheres and magnetospheres throughout the solar system. The
solar system offers a wide variety of conditions under which the
interaction of bodies with a plasma environment can be studied:
there are planets with and without large-scale magnetic fields and
associated magnetospheres; planetary atmospheres display a variety
of thicknesses and compositions; satellites of the giant planets
reveal how interactions occur with subsonic and sub-Alfvenic flows
whereas the solar wind interacts with supersonic and super-Alfvenic
impacts.
Encompassed under a general title of comparative magnetospheres
are processes occurring on a range of scales from the solar wind
interacting with comets to the interstellar medium interacting with
the heliosphere. The school will address not only the physics of
all these various environments but will also go into the
technologies by which these various environments are being
observed. The program is complemented with considerations of the
societal impacts of space weather that affects satellites near
Earth and elsewhere in the solar system.
The school will be based on lectures, laboratories, and
recitations from world experts, and will draw material from the
three textbooks Heliophysics I-III, published by Cambridge
University Press.
Several teachers along with about 35 students will be selected
through a competitive process organized by the UCAR Visiting
Scientist Programs. The school lasts for eight days, and each
participant receives full travel support for airline tickets,
lodging and per diem costs.
Website:
http://www.vsp.ucar.edu/Heliophysics/
Start : 2013-07-16 - End : 2013-07-25
The Summer School Alpbach enjoys 36 years of tradition in
providing in-depth teaching on different topics of space science
& technology, featuring lectures and concentrated working
sessions on mission studies in self-organised working groups. 60
young highly qualified European science and engineering students
converge annually for stimulating 10 days of work in the Austrian
Alps. 4 teams compete to design a space mission judged by a jury of
experts. Students learn how to approach the design of a satellite
mission and explore new and startling ideas supported by experts.
The Summer School 2013 will focus on Space Weather
.
The purpose of the Summer School is to foster the practical
application of knowledge derived from lectures, to develop
organisational and team-work skills and to encourage creativity.
Teams will compete to design the best project, judged by an
independent jury. The teams themselves are responsible for the
selection of the subject of the project and for the team structure
and working methods.
Website:
http://www.summerschoolalpbach.at/
Start : 2013-09-09 - End : 2013-09-14
We gain information about the universe through analysis of the
spectra from celestial objects. However, while the intensity
spectrum represents a scalar quantity but electromagnetic radiation
occurs in the form of transverse waves, the polarized spectrum
provides us with a 4-vector, the Stokes vector. The increased
amount of information space opens new windows to the universe, in
particular for the exploration of magnetic fields. It is well
recognized that the magnetic field is a primary agent responsible
for structuring and the source of all variability on intermediate
time scales, which manifests itself in all forms of solar and
stellar activity.
It is therefore not surprising that every year there are many
scientific meetings organized with the objective of studying the
role of magnetic fields in cosmic objects. What is largely missing
in these meetings is however an in-depth investigation of the
fundamental aspects of how magnetic fields can be determined by the
means of spectro-polarimetry, our main gateway to cosmic magnetism.
The primary aim of our series of Workshops is to address these
fundamental aspects, with less emphasis on the morphological and
physical properties of cosmic magnetic fields.
Website: http://spw7.ynao.ac.cn/
Start : 2013-11-18 - End : 2013-11-22
The 10th Edition of the European Space Weather
Week will take place on 18-22nd
November 2013 in Belgium. The venue will be confirmed early next
year, but mark your calendars now for the 10th Anniversary of this
growing European event.
The ESWW will again adopt the central aim of bringing together
the diverse groups in Europe working on different aspects of Space
Weather
. This includes but isn't
limited to the scientific community, the engineering community,
applications developers, service providers and service end users.
The meeting organisation will again be coordinated by the Belgian
Solar-Terrestrial Centre of Excellence (STCE), ESA
and the Space Weather
Working Team. The local
organisation will be done by the STCE.
Website: not yet available
Start : 2014-08-02 - End : 2014-08-10
The 40th COSPAR Scientific Assembly will be held in Moscow,
Russia from 2 - 10 August 2014. This Assembly is open to all bona
fide scientists.
Website:
http://www.cospar-assembly.org/