NAU Harvester System
Auroral activity in connection with structure of the heliospheric magnetic field
Вісник астрономічної школи
View Archive Info| Field | Value | |
| Title |
Auroral activity in connection with structure of the heliospheric magnetic field
|
|
| Creator |
Reshetnik V.M.
Dziubenko M.I. |
|
| Date |
2004
|
|
| Source |
Astronomical School’s Report, 2004, Volume 5, Issue 1-2, P. 79-87
2411-6602 |
|
| Identifier |
http://astro.nau.edu.ua/papers/AstSR_2004_Vol_5_Iss_1_P_79.pdf
10.18372/2411-6602.05.1079 |
|
| Language |
uk
|
|
| Description |
Variations of polar flux in northern and southern ovals and integral precipitation intensity were analyzed in connection with changes of the heliospheric magnetic field near the Earth. It is shown that polar flux increases when the magnetic field has Bz <0 and By <0, and when the magnitude of the interplanetary magnetic field increases. The seasonal variation of auroral precipitation intensity is observed also aurora activity is maximal during equinoxes and minimal during solstices. The dependence of the auroral precipitation on IMF orientation has a strong asymmetry in heliographic inertial coordinates (HGI) which amount to 50 per cent. Auroral intensity is maximum when the magnetic field is situated at the first quadrant of HGI coordinates.
|
|
| Publisher |
National Aviation University
|
|
| Format |
application/pdf
|
|