• No results found

Operational Directorate 4 "Solar Physics and Space Weather"

N/A
N/A
Protected

Academic year: 2021

Share "Operational Directorate 4 "Solar Physics and Space Weather""

Copied!
29
0
0

Bezig met laden.... (Bekijk nu de volledige tekst)

Hele tekst

(1)

David Berghmans


Head Of Scientific Service

Operational Directorate 4


(2)

http://sidc.be/aboutSIDC

Mission Statement

1. Research: to increase our

understanding of the

Sun

and

its influence on the solar system.

2. Observations: to have a full

understanding of the complete

data acquisition and calibration

process.

3. Services: to have an active,

leading role in European space

weather services

(3)

Thematics

1. Ground-based telescopes 2. Solar Radio Physics

3. Space based instruments 4. Advanced technology

5. Data Processing

(4)

Thematics

1. Ground-based telescopes 2. Solar Radio Physics

3. Space based instruments 4. Advanced technology

5. Data Processing

6. Space Weather services

TYPICAL SETUP:


structurally supported by an STCE funding line 


managed by a contractual scientist


encouraged to grow through project money

(5)

Thematics

1. Ground-based telescopes 2. Solar Radio Physics

3. Space based instruments 4. Advanced technology

5. Data Processing

6. Space Weather services

TYPICAL SETUP:


structurally supported by an STCE funding line 


managed by a contractual scientist


encouraged to grow through project money

F

u

n

d

a

m

e

n

ta

l

R

e

s

e

a

rc

h

D

is

s

e

m

in

a

ti

o

n

(6)

Thematics

since 1950s

since 1981

1. Ground-based telescopes 2. Solar Radio Physics

3. Space based instruments 4. Advanced technology

5. Data Processing

(7)

Thematics

SOHO/EIT since 1995

PROBA2 since 2009

1. Ground-based telescopes

2. Solar Radio Physics

3. Space based instruments 4. Advanced technology

5. Data Processing

(8)

Thematics

since 2002

1. Ground-based telescopes 2. Solar Radio Physics

3. Space based instruments 4. Advanced technology

5. Data Processing

(9)

Thematics

since 2000

since 2006

since 2010

• daily space weather forecast • weekly review of activity

European Space 
 Weather Week ESA
 Space
 Situational
 Awareness 1. Ground-based telescopes

2. Solar Radio Physics

3. Space based instruments 4. Advanced technology

5. Data Processing

(10)

ESA Space Situational Awareness

+

instrument prototype projects

+

modelling efforts

(11)

statistics on personnel,

budgets, performance

(12)

Thematics

1. Ground-based telescopes 


& long term monitoring

2. Solar Radio Physics

3. Space based instruments

4. Advanced technology

5. Data Processing, incl

visualisation

6. Space Weather services,


incl. dissimenation

Technical staff space researcher Other scientist IT specialist 3 3 0 0 1 2 1 0 1 10 4 1 0 1 2 0 2 1 0 4 2 3 2 0

(13)

43 people

9 technical staff

20 space

researchers

5 IT specialist

9 other scientists

~25 FTE researchers of which 1 PhD student (KULeuven)

~ 12 nationalities, most < 45 years

12%

21%

47% 21%

(14)

ESA, H2020,

IUAP brain.be

PRODEX STCE ROB

technical staff 1 0 2 6 scientific staff 12 11 8 2+(1)

30%

26%

23%

21%

financing: 2016

TOTAL

43 people,

of which 2

permanent

scientists

(15)

ESA, H2020,

IUAP brain.be

PRODEX STCE ROB

technical staff 1 0 2 6 scientific staff 12 11 8 2+(1) evolution ? increased competition, end of IUAP, brain.be less research, more technical mission preparation erosion erosion

financing: 2016

TOTAL

43 people,

of which 2

permanent

scientists

30%

26%

23%

21%

(16)

0 10 20 30 40 2003 2004 2005 2006 2007 2008 2009 2010 2011 2012 2013 2014 2015

research papers in international refereed journals

OPPY rule

(17)

Message # per year # clients

fast space weather alerts 150 950

daily space weather forecast 365 709

weekly reviews 52 507

monthly sunspot index bulletin 12 684

(18)

Scientific Production: data set collection

USET telescopes

Humain radiospectrographs

International Sunspot Index

(19)
(20)

S PA C E R E S E A R C H

P R E S E N T E D B Y A N D R E I Z H U K O V

O D 4 “ S O L A R P H Y S I C S A N D S PA C E W E A T H E R ”

(21)

I N V O LV E M E N T I N S O L A R S PA C E M I S S I O N S ( 1 ) (funded by PRODEX and STCE)

Sour

ces of t

he CME mass

(Zhukov & Auchè

re 2004) Thermal structur e of act ive regions (Reale et al. 2007) SOHO Hinode CME stat ist ics over t he solar cycle ( Robbr echt et al. 2009) Mul ti-component out flows in cor onal dimmings (Dol la & Zhukov 2011)

(22)

I N V O LV E M E N T I N S O L A R S PA C E M I S S I O N S ( 2 ) (funded by PRODEX and STCE)

3D structur

e of

“EIT waves” (Zhukov 2011)

Giant and hot post-erupt

ive

loops

(W

est & Seaton 2014)

STEREO SDO 3D r econstruct ion of CMEs (Mierla et al. 2010) Supervised classificat ion of solar featur es (De V isscher et al. 2015)

(23)

P R O B A 2

OD4 has the PI-ship of the SWAP and

LYRA instruments funded by PRODEX.

PROBA2 Science Center (P2SC)

hosted by ROB operates the scientific payload. The development and

operations of the P2SC are funded by PRODEX, STCE, ESA D/SRE, and SSA.

A special issue of Solar Physics

dedicated to PROBA2 was published in 2013.

• Co-edited by the OD4 team

members.

• A number of papers were

co-authored by the OD4 researchers. Quasi-periodic pulsations in

flares (Dolla et al. 2012)

Large-scale coronal structure

(24)

P R E PA R AT I O N O F F U T U R E E S A

M I S S I O N S

Solar Orbiter (to be launched in October 2018)

• The mission will establish how the Sun creates

and controls the heliosphere.

• OD4 has the CoPI-ship of the Extreme Ultraviolet Imager (EUI) funded by PRODEX.

• The EUI PI-ship is now with CSL but will be transferred to OD4 after the launch.

PROBA-3 (to be launched in the end of 2019)

• The mission will have the best straylight rejection

ever achieved by a solar coronagraph, allowing us to observe structures very close to the solar limb.

• OD4 has the PI-ship of the ASPIICS coronagraph funded by PRODEX.

• CSL leads the industrial consortium that is

(25)

S PA C E T E C H N O L O G Y & C A L I B R AT I O N

L A B O R AT O R I E S ( S T C L @ S T C E )

Two complementary groups:

- STCE WP ROB A.5 : “Advanced Technology for Solar Observations” (led by Dr A. BenMoussa)

- STCE WP BISA A.4 : “Optics Laboratory facilities” (led by Dr D. Bolsée)

agree to join their efforts to support the design, development & calibration of instruments (from soft X-ray to IR).

Interdisciplinary team

Dr Ali BenMoussa (STCE, ROB) Dr David Bolsée (STCE, BISA) Dr Samuel Gissot (ROB) Dr Boris Giordanengo (ROB) Nuno Pereira (BISA)

More information:

http://www.stce.be/projects/WP/STCL.php http://bold.oma.be/

More specifically:

-1- High-quality calibration of space- and ground-based instruments • Pre-flight sub-system and end-to-end calibration,

• In-flight calibration systems and operations,

• Co-operation with European and international organizations for calibration/metrology standards,

-2- Design next generation of space-based instruments

• R&D in advanced technologies (e.g., wide bandgap detectors, CMOS active pixel sensor, UV LEDs, optical filters, FPGA, … ),

• Scientific data compression, processing, and exploitation,

• Instrument ageing effects: space-environment irradiation testing, lesson learned from past and present space missions, contamination/

cleanliness issues, modeling & simulation.

(26)
(27)

Ussual problems

high dependence on soft money

push towards applied research at the expensive of

services

(28)

collaborations with

universities

KULeuven, CmPA.


Joint PhDs, Provision of Numerical codes, joint

research projects

ULiege, CSL


(29)

• Of the 26 permanent scientists at ROB, only 2 are at OD4

while it is the biggest directorate. 2 permanent scientists is not sufficient to secure the management.

• A number of contractual scientists on semi-hard money

(STCE) take up management roles, despite lack of personal promotion possibilities.

• The permanent & contractual management together are

succesfull in attracting soft money for the other half of the group.

• The whole construction is sensitive to departure of

contractuals with key-roles


Referenties

GERELATEERDE DOCUMENTEN

In fact, a detailed study of the physics of the interaction between PAHs and high energy particles (ions and electrons) was still lacking, although PAHs are a key component of the

Benzene (C 6 H 6 ) is an aromatic hydrocarbon (not polycyclic since only one ring is present) and a fundamental unit of the Polycyclic Aromatic Hydro- carbons (PAHs) which are

Interstellar PAHs are often “associated” with dust grains because, on the one hand, they are formed as a by-product of the formation of carbonaceous dust, and on the other hand,

The calibration is based on observations of standard stars (Decin et al. The ends of each orders, where the noise increases significantly, were man- ually clipped. To obtain a good

The fractional destruction induced by nuclear excitation increases with the PAH size, while in case of electronic excitation and electron collisions is lower for higher N C values,

Because of the decrease of the dissociation probability when the PAH size increases, as expected, the electron and electronic rate constants are strongly suppressed, and both

As expected, when E min = 50 MeV/nucleon τ 0 is higher for all sizes, ions and E 0 , due to the fact that we include in the calculation only the cosmic rays with higher energies,

In Chapter 3 we use our models to estimate the lifetime of PAHs against collisions with ions and electrons having high velocities arising from the thermal and relative motions