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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 ObjectivesThey are two-fold: Solar
Planetary
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FUV: 117 - 200 130 - 300 |
60 x 60 |
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0.04 - 0.1 |
~ 20 |
UV: 280 - 400 |
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(0.001*) |
Mass |
160 kg (including 20% margin) |
Telemetry |
400 kbits/s average |
Envelope |
Ø110 x 150 cm3 |
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) |
See also, for more completness, our last paper detailing the program, design, focal instrument, image reconstruction, etc.
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 |
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Web Page: Luc Damé |
Last Updated Friday, March 19, 1999 |