SOLARNET FACTS

Status of the program at ESA: SOLARNET recommended for a SMART - ESA Technology Mission. Read the SolarNews announcement of Eric Priest following the ESA Tenerife Symposium, 'A CROSSROADS for EUROPEAN SOLAR and HELIOSPHERIC PHYSICS: RECENT ACHIEVE-MENTS and FUTURE MISSION OPPORTUNITIES', 23-27 March 1998

News

Download (proc_Tenerife98.pdf [642 KB]) or read (proc_Tenerife98/proc_Tenerife.htm) our last paper giving detailed information - 23 pages proceeding of the Tenerife meeting,23-27 March 1998, ESA SP-417 - on the program, the instrument and focal instrumentation (the 'subtractive double monochromator, image reconstruction, etc.). A poster paper (proc_Tenerife98_demo.pdf [423 KB] concentrates more on concrete laboratory demonstration work.


Science Objectives

They are two-fold: 

Solar

  • Understand plasma processes: current sheets, reconnection, "blinkers", double layers, Alvenic waves heating, plasmoid formation, electrodynamics coupling
  • Untangle magnetohydrodynamic configurations: coronal loops, prominences, chromospheric spicules, sunspots, photospheric flux tubes
  • Probe radiation hydrodynamics: granulation, acoustic heating, shock formation and dissipation
  • Determine fine scale structure activity: evolution of magnetic patterns, flux emergence and disappearance
  • Discover the mechanisms of eruptive phenomena and instabilities: flares, micro-flares, "disparition brusques" of prominences, surges, coronal bullets, ephemeral active region

Planetary

  • Atmosphere of the giant planets: Jupiter (balance between solar and auroral energy), Saturn (auroral UV emission)
  • Magnetospheric activity of Mercury
  • Monitoring UV contrasts and Albedo of Venus atmosphere
  • Contribution to the study of minor bodies (comets, asteroids) by images in FUV and UV (over 3 years, up to 40 asteroids will be seen with a size larger than 75 mas)

Mission Description

SOLARNET on PROTEUS

Measurement Strategy

Technology Requirements

Status

 

Spatial and Spectral Possible Characteristics of SOLARNET Focal Plan Instrumentation

Wavelength
Field-of-view
Detectors
Spatial resolu-
Spectral
range (nm)
(arcsec)
Pixels
Type
tion (arcsec)
resolution (nm)

FUV: 117 - 200

130 - 300

40 x 40

60 x 60

2048 x 2048
ICCD
0.025 - 0.04

0.04 - 0.1

0.002

~ 20

UV: 280 - 400

60 x 60
2048 x 2048
ICCD
0.06 - 0.08
0.01

(0.001*)

* This could be achieved by an extra filtering (Fabry Perot).

 

SOLARNET Resources Summary

Mass

160 kg (including 20% margin)

Telemetry

400 kbits/s average
(4 Mbits/s at maximum rate)

Envelope

Ø110 x 150 cm3
(3 x Ø35 cm telescopes)

Primary pointing accuracy

± 0.5°

Primary pointing stability

± 0.03°/s

Internal Active pointing stability

< 12 mas

Internal phase control

< l/8 (at Lyman a, 120 nm)

Field-of-view

1.2° (Sun viewing)

Power

60 watts (peak: 75 watts)

Mission duration

2 nominal (and up to 6 years)

More on SOLARNET

See also, for more completness, our last paper detailing the program, design, focal instrument, image reconstruction, etc.

Science Team

Luc Damé (Chair)
Service d'Aéronomie du CNRS
BP 3, F-91371, Verrières-le-Buisson Cedex, France
Tel.: [33] 1 64474328
Fax: [33] 1 69202999
e-mail: luc.dame@aerov.jussieu.fr
Michel Hersé
Service d'Aéronomie du CNRS
BP 3, F-91371, Verrières-le-Buisson Cedex, France
Tel.: [33] 1 64474280
Fax: [33] 1 69202999
e-mail: michel.herse@aerov.jussieu.fr
Pierre Cugnon
Observatoire Royal de Belgique
3 Avenue Circulaire, B-1180 Bruxelles, Belgique
Tel.: [32] 2 3730276
Fax: [32] 2 3730224
e-mai: Pierre.Cugnon@ksb-orb.oma.be
Anny-Chantal Levasseur-Regourd
Service d'Aéronomie du CNRS
BP 3, F-91371, Verrières-le-Buisson Cedex, France
Tel.: [33] 1 64474293
Fax: [33] 1 69202999
e-mail: aclr@aerov.jussieu.fr
André Preumont
Dépt. de Génie Mécanique et Robotique
Université Libre de Belgique
Av. F.D. Roosevelt, B-1050, Bruxelles, Belgique
Tel.: [32] 2 6504663
Fax: [32] 2 6504660
e-mai: apreumon@ulb.ac.be
Thomas Widemann
Service d'Aéronomie du CNRS
BP 3, F-91371, Verrières-le-Buisson Cedex, France
Tel.: [33] 1 64474256
Fax: [33] 1 69202999
e-mail: thomas.widemann@aerov.jussieu.fr
Sami K. Solanki
Institut Für Astronomie, ETH-Zentrum,
CH-8092, Zürich, Switzerland
Tel.: 41] 1 6323810
Fax: [41] 1 6321205
e-mail: solanki@astro.phys.ethz.ch
Francesco Angrilli
CISAS - Universita di Padova
Via Gradenigo 6A, I-35100, Padova, Italy
Tel.: [39] 49 8276790
Fax: [39] 49 8276785
e-mail: Angrilli@mail.dim.unipd.it
Philippe Lemaire
Institut d'Astrophysique Spatiale
Université Paris XI, Bât. 121,
F-91405, Orsay Cedex, France
Tel.: [33] 1 69858622
Fax: [33] 1 69858675
e-mail: lemaire@iaslab.ias.fr
Gianandrea Bianchini (Instrument Scientist)
CISAS - Universita di Padova
Via Gradenigo 6A, I-35100, Padova, Italy
Tel.: [39] 49 8276808
Fax: [39] 49 8276785
e-mail: mecca01@ipdunivx.unipd.it
Renée Prangé
Institut d'Astrophysique Spatiale
Université Paris XI, Bât. 121,
F-91405, Orsay Cedex, France
Tel.: [33] 1 69858581
Fax: [33] 1 69858675
e-mail: Prange@iaslab.ias.fr
Roberto Ragazzoni
Osservatorio Astronomico di Padova
vicolo dell'Osservatorio, 5
I-35122, Padova, Italy
Tel.: [39] 49 8070268
Fax: [39] 49 8293416
e-mail: ragazzoni@astrpd.pd.astro.it
Brigitte Schmieder
DASOP, Observatoire de Paris
5 Place Jules Janssen
F-92195, Meudon Cedex, France
Tel.: [33] 1 45077817
Fax: [33] 1 45077959
e-mail: schmieder@obspm.fr
R Kariyappa
Indian Institute of Astrophysics,
Koramangala, Bangalore 560034, India
Tel.: [91] 80 5530672
Fax: [91] 80 5534043
e-mail: rkari@iiap.ernet.in
Philippe Zarka
DESPA, Observatoire de Paris
5 Place Jules Janssen
F-92195, Meudon Cedex, France
Tel.: [33] 1 45077819
Fax: [33] 1 45072806
e-mail: zarka@obspm.fr


Web Page: Luc Damé

Last Updated Friday, March 19, 1999