Search Publications

Magnetic turbulence in the cusp region: 3D spectra and vortex cascades
DOI: 10.1134/S0016793213060133 Bibcode: 2013Ge&Ae..53..733R

Romanov, S. A.

Cluster satellite measurements that were carried out in the region of the altitudinal cusp in the Earth's magnetosphere and adjacent regions were processed to yield the dynamic pattern of the 3D spectra of magnetic field oscillations in the space of wave vectors, with wave numbers ranging from 0.002 to 0.5 rad/km. The anisotropic properties of spa…

2013 Geomagnetism and Aeronomy
Cluster 1
On the possibility of coupling satellite and ground-based optical measurements in the region of pulsating auroras
DOI: 10.1134/S001679321007008X Bibcode: 2010Ge&Ae..50..873S

Safargaleev, V. V.; Shibaeva, D. N.; Sergienko, T. I. +1 more

The possibility of comparing in detail CLUSTER satellite data with data on pulsating spots registered with a TV camera at the Lovozero Observatory when the satellite crossed the magnetospheric region related to the camera's field of view is discussed. The satellite ionospheric projections were calculated using the T89, T96, and T01 models. It was …

2010 Geomagnetism and Aeronomy
Cluster 2
New method for separating K- and F-corona brightness based on LASCO/SOHO data
DOI: 10.1134/S0016793209070020 Bibcode: 2009Ge&Ae..49..830F

Fainshtein, V. G.

A relatively simple (in technology) method for separating K- and F-corona brightness based on LASCO data, which makes it possible to obtain the latitude distribution of this brightness in the field of view of the LASCO C2 and C3 coronographs at any instant for which white light corona images are available, has been proposed. It has been estimated …

2009 Geomagnetism and Aeronomy
SOHO 3
Correlation between the parameters of coronal mass ejections and features of their propagation in the corona with the large-scale structure of the solar magnetic field
DOI: 10.1134/S001679320908009X Bibcode: 2009Ge&Ae..49.1096I

Ivanov, E. V.; Fainshtein, V. G.; Rudenko, G. V.

Correlation between the parameters of coronal mass ejections (CMEs) that are detected on the LASCO coronographs and are associated with eruptive prominences and the distances of CME axes from the coronal streamer belt has been analyzed. The deviations of CME trajectories from the radial direction have been investigated.

2009 Geomagnetism and Aeronomy
SOHO 2
Space projections on solar-terrestrial physics
DOI: 10.1134/S0016793209080209 Bibcode: 2009Ge&Ae..49.1137K

Zelenyi, L. M.; Kuznetsov, V. D.

An overview of the current status of research in the field of solar-terrestrial physics conducted by space agencies of various countries is given. The main results of current (Ulysses, SOHO, TRACE, RHESSI, Hinode, and STEREO) and completed (Coronas-F and others) missions as well as the scientific goals and objectives of space projects being prepar…

2009 Geomagnetism and Aeronomy
Ulysses 2
Ejection and descent of matter in the solar atmosphere
DOI: 10.1134/S0016793209080088 Bibcode: 2009Ge&Ae..49.1093D

Divlekeev, M. I.

The descent and ejection of matter in the solar atmosphere observed in the CaII 8498-Å line have been studied. In the NOAA active region no. 10 792 on July 30, 2005 before the flare, the dense cold gas cloud descended with a ray velocity of ∼8 km/s and then ascended in the impulsive phase. The plasma ascended with an acceleration reaching 0.4 km/s…

2009 Geomagnetism and Aeronomy
SOHO 0