In: Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 40, no. 1
J. Ambróz - K. Radziszewski - P. Rudawy - J. Rybák - K.j.h. Phillips
Detaily:
Rok, strany: 2010, 5 - 18
Kľúčové slová:
Sun, corona, coronal heating, instrumentation, fast imaging
URL originálneho zdroja: http://www.astro.sk/caosp/Eedition/Abstracts/2010/Vol_40/No_1/pp5-18_abstract.html
O článku:
Heating mechanisms of the solar corona will be investigated at the
high-altitude solar observatory Lomnicky Peak of the Astronomical Institute
of SAS (Slovakia) using its mid-size Lyot coronagraph and post-focal
instrument SECIS provided by Astronomical Institute of the University of
Wrocław (Poland). The data will be studied with respect to the energy
transport and release responsible for heating the solar corona to
temperatures of mega-Kelvins. In particular investigations will be focused
on detection of possible high-frequency MHD waves in the solar corona. The
scientific background of the project, technical details of the SECIS system
modified specially for the Lomnicky Peak coronagraph, and inspection of the
test data are described in the paper.
Ako citovať:
ISO 690:
Ambróz, J., Radziszewski, K., Rudawy, P., Rybák, J., Phillips, K. 2010. The SECIS instrument on the Lomnický Peak Observatory. In Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 40, no.1, pp. 5-18. 1335-1842.
APA:
Ambróz, J., Radziszewski, K., Rudawy, P., Rybák, J., Phillips, K. (2010). The SECIS instrument on the Lomnický Peak Observatory. Contributions of the Astronomical Observatory Skalnaté Pleso, 40(1), 5-18. 1335-1842.