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CoSTePA Correlated Solar-Terrestrial Polar Activities. E. Amata M. Candidi (1) , M.F. Marcucci (1) , S. Massetti (1) , P. Francia (3) , U. Villante (3). (1) Istituto di Fisica dello Spazio Interplanetario (IFSI), INAF, Rome, Italy
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Correlated Solar-TerrestrialPolar Activities
M. Candidi(1), M.F. Marcucci(1), S. Massetti(1),
P. Francia(3), U. Villante(3)
(1)Istituto di Fisica dello Spazio Interplanetario (IFSI), INAF, Rome, Italy
(3)Dipartimento di Fisica, Università dell’Aquila, l’Aquila, Italy
The study of the polar and auroral ionosphere and the related ground based measurements (radars, magnetometers, all sky cameras, riometers) is essential to achieve a better understanding of Sun-Earth relations
CoSTePA aims at:
- the installation (by January 2008) of two SuperDARN radars at Dome C, to complete the southern hemisphere SuperDARN MLT coverage of the auroral Ionosphere;
- the coordinated study of data from such radars, the italian all-sky camera at Terra Nova Bay, the italian ground magnetometers at Terra Nova Bay and Dome C, the two italian northern hemishere all sky cameras of Ny Alesund and Daneborg;
- the development of an italian national web portal with two main objectives:
1) support the data exchange in the national community, 2) provide an
education and outreach tool towards the public at large.
SuperDARN, All Sky Camera and ground magnetometer data are all relevant to both themes hereafter dealt with. Some examples are detailed, one per theme.
IPY theme 3.
The completion of the SuperDARN Southern hemisphere network will allow a better description of the auroral and polar ionospheric convection, aiming at the real time nowcasting of the cross polar cap potential.
IPY theme 5.
Entry mechanisms of upstream waves in the magnetosphere or/and local generation and propagation of ULF waves.
Monitoring of the position and extension of the cusp (seasonal, solar wind related effects).
Extension of magnetospheric substorms into the polar cap.
- IFSI participation to the 2 Dome C radars (PI’s: E. Amata & J.-P. Villain).
and the AURORA all sky camera (with ENEA) at MZS
The French- Italian Concordia base at DOME C (DMC)
CGM lat: 89°S; MLT=UT-08:55
The University of L’Aquila runs high resolution triaxial search-coil magnetometers with 1s sampling at Dome C and MZS.
The Italian Mario Zucchelli Station
at Terra Nova Bay (TNB)
CGM lat: 80°S; MLT=UT-08:11
The geomagnetic storm of October 2003 (maximum K index=9) as recorded by L’Aquila (AQU) and Mario Zucchelli Station (TNB) observatories.
For the same storm the panel on the left shows the arrival of two simultaneous wave packets at AQU and TNB related to the global oscillation modes of the magnetospheric cavity.
power in the Pc3-4 range during November 16-22, 2003
the power detected at TNB peaks around noon, when the station approaches the cusp, and does not appear at DMC, in the deep polar cap;
both DMC and TNB observations show a general trend for a power decrease with decreasing solar wind speed.
similar power enhancements appear at both stations (the cusp shifts at lower latitudes and also TNB stays in the deep cap);
enhancements correspond to solar wind density peaks.
De Lauretis et al., JGR, 2005
Geographic (dotted lines) and Corrected Geo-Magnetic CGM (solid lines) coordinates
Geographic (black) and Corrected Geo-Magnetic CGM (red) coordinates
December 19, 2002: a double cusp observed by ITACA2 interpreted through SuperDARN data
But, there is already an all sky camera (IFSI & ENEA) at MZS...
... And IFSI is constructing (for the end of 2007) the two SuperDARN radars at Dome C.
MZS magnetometers, riometers,
Ionosonde, GPS, All sky camera.
A significant scientific contribution can be provided by the italian community to
ICESTAR and IPY.