ISSI International Team 150
February
1-4, 2010
International
Space Science Institute (ISSI)
Hallerstrasse 6
3012 BERNE - SWITZERLAND
PARTICIPANTS
C.HANUISE, Team Leader
G. BERTHET
E.
BLANC
J. BLECKI
M. FULLEKRUG
M. GODEFROY
F. GORDILLO-VAZQUEZ
F. LEFEUVRE
S. KLIMOV
J. MONTANYA
Y.
ORSOLINI
M. PARROT
E. SERAN
E. TURUNEN
AGENDA
|
01/02 |
C. Hanuise |
Organization of the meeting, outputs … |
|
|
E. Turunen |
Status of EISCAT_3D planning |
|
|
S. Klimov |
Status
of CHIBIS |
|
|
J.L. Pinçon |
Status
of TARANIS |
|
|
|
|
|
02/02 |
E. Blanc |
Associated ground-based measurements of infrasound
and atmospheric waves |
|
|
M. Fullekrug |
Radio
observations of sprites |
|
|
F. Gordillo-Vazquez |
Atmospheric chemistry driven by sprites |
|
|
J.A. Sauvaud |
Wave particle interactions leading to radiation belt
particle precipitation inside the atmosphere: Some Demeter results |
|
|
E. Turunen |
Report from the 2nd HEPPA(High-Energy Particle
Precipitation in the Atmosphere) workshop in Boulder |
|
|
M. Parrot |
A search of powerful whistlers recorded by DEMETER |
|
|
J. Blecki |
Strong electromagnetic ELF/VLF emissions observed by
DEMETER during thunderstorm over southern France on 8/10/2009 |
|
|
|
|
|
03/02 |
G. Berthet |
Stratospheric
chemistry and physics |
|
|
Y. Orsolini |
Satellite measurements of nitrogen family species |
|
|
E. Turunen |
Proposal for an extended atmospheric measurement
campaign at EISCAT: Next Solar Maximum |
|
|
E. Seran |
LDLEGO: electric measurements in the auroral
stratosphere during magnetospheric storms |
|
|
E. Blanc |
Projet ARISE (Atmospheric Research from InfraSound
monitoring in Europe) |
|
|
J.B. Renard |
COBRAT balloon campaigns associated with ASIM and
TARANIS |
|
|
M. Godefroy |
Emebedded, Light, Multi-Instrument Gondola (ELMIG)
for balloon measurements. Concept and examples of applications for
stratospheric observations in thunderstorm and auroral regions |
|
|
E. Seran / M.
Godefroy |
MEF-ATLEC of COBRAT/TARANIS project:
electric&magnetic measurements and 3D imaging of
stratospheric/tropospheric discharges |
|
|
|
Discussion on COBRAT (instruments, locations, …) and
on future studies of optical emissions from TLEs (possible IR and UV
emissions from space) |
|
|
S. Klimov |
RUSALKA
experiment |
|
|
|
|
|
04/02 |
J. Montanya |
Presentation of UPC lightning detection group |
|
|
E. Turunen |
Preliminary plans of Dr Annika Seppala ISSI team |
|
|
|
Discussion on various cooperative projects (TEA-ESF,
…) |
|
C. Hanuise |
Conclusions of the meeting – Next meeting |
The main objectives of the second
team meeting were (1) to examine the theoretical and modeling studies of the
chemistry related to Transient Luminous Events (TLEs) in the atmosphere, and
(2) to define the ground-based or balloon instruments necessary to study the
TLEs in association with the various space missions. In particular, we have
reviewed the COBRAT long-duration balloon project and determined the set of
instruments that could be flown on these balloons.
As detailed in the attached agenda,
presentations have been made on:
- Status
of TARANIS and CHIBIS space missions,
- Space
observations of nitrogen family species,
- Atmospheric chemistry models,
- Atmospheric
effects of thunderstorms: infrasound, gravity waves,
- Radio detection of sprites,
- Waves
related to thunderstorm activities at ELF, VLF and HF,
- Development
of balloons and associated instrument,
- Various
activities related to TLEs in members’ institutions,
- Presentation
of Dr A. Seppäla ISSI team.
All presentations are available in a
protected area of the team ISSI website.
.
The team discussions led to a
successful definition of the COBRAT balloon project. The team agreed
unanimously to hold a third meeting, probably early in 2011. Several actions
have been defined, to be performed before this last team meeting.
Conclusions
The following conclusions, and
associated actions, were decided for the next team meeting:
·
As there is overlapping interest in both team, hold
the 3rd team meeting at the same time as Dr A. Seppäla team meeting,
if feasible. Dr E. Turunen belongs to both team and will take care of the
coordination.
·
Define priority scientific topics of interest for the
next meeting,
·
Final definition of COBRAT balloons and submission to
CNES for funding. Study the possibility of making infra-red observations (never
made before) and that are of large interest to compare with model predictions.
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