Mica: The mirror coronagraph for Argentina

Space Science Reviews

Volumn 87, Issue 1-2, 1999, Pages 307-310

  Stenborg, G ^a   Schwenn, R ^a   Srivastava, N ^a   Inhester, B ^a   Podlipnik, B ^a   Rovira, M ^b   Francile, C ^c  

^a MAX PLANCK INSTITUT FÜR SONNENSYSTEMFORSCHUNG   (Germany)

^b INSTITUTO DE ASTRONOMÍA Y FÍSICA DEL ESPACIO   (Argentina)

^c Observ Astron Félix Aguilar   (Argentina)

Author keywords

Corona; Coronagraph

Indexed keywords

EID: 0038905094     PISSN: 00386308     EISSN: None     Source Type: Journal    
DOI: 10.1023/a:1005141727375     Document Type: Article

References (5)

1. Brueckner, G. E., et al.: 1995, 'The Large Angle Spectroscopic Coronagraph (LASCO),' Solar Phys., 162, 357.
2. Epple, A., and Schwenn, R.: 1995, 'PICO: A Mirror Coronagraph on Pic Du Midi,' Proc. 15th National Solar Observatory/Sacramento Peak Summer Workshop, 1, 233.
3. Epple, A.: 1997, 'Erdgebundene Beobachtungen der Sonnenkorona mit einem Spiegelkoronographen,' Ph.D. Thesis, Göttingen University, Germany, pp. 42-47.
4. Newkirk G., and Bohlin, D.: 1963, 'Reduction of Scattered Light in the Coronagraph,' Appl. Opt., 2, 131.
5. Schwenn, R., et al.: 1997, 'First View of the Extended Green-Line Emission Corona at Solar Activity Minimum using the LASCO-C1 Coronagraph on SOHO,' Solar Phys., 175, 667.