| Issue |
EAS Publications Series
Volume 14, 2005
Dome C Astronomy and Astrophysics Meeting
|
|
|---|---|---|
| Page(s) | 269 - 274 | |
| DOI | https://doi.org/10.1051/eas:2005042 | |
| Published online | 05 January 2006 | |
M. Giard, F. Casoli and F. Paletou (eds)
EAS Publications Series, 14 (2005) 269-274
Diagnostic of the Solar Atmosphere through Two Level Doppler and Magnetic Measurements
1
Dipartimento di Fisica, Universita degli Studi di Roma “La
Sapienza”, Piazzale Aldo Moro2, 00185 Roma, Italy;
2
Maui Scientific Research Center,
University of New Mexico, 590 Lipoa Parkway, Suite 262, Kihei, HI
96753, USA
3
Oceanit Inc., 590 Lipoa Parkway, Suite 264, Kihei, HI 96753, USA
Corresponding author: alessandro.cacciani@roma1.infn.it
This contribution describes our solar project at the Antarctic sites of Baia Terranova, South Pole and Dome-C. The project is based on a multi-level helioseismology analysis, aimed to study, for the first time, the local properties of the solar atmosphere. In addition, we plan to detect the presence of Alfvèn waves in and around the active regions, as an energy transfer vehicle from sunspots towards the corona. The technology used is the well known compact, stable, relatively unexpensive and still improving MOF (Magneto-Optical Filter).
© EAS, EDP Sciences, 2005