Structure of magnetic fields in NOAA active regions 0486 and 0501 and in the associated interplanetary ejecta

Details Structure of magnetic fields in NOAA active regions 0486 and 0501 and in the associated interplanetary ejecta Structure of magnetic fields in NOAA active regions 0486 and 0501 and in the associated interplanetary ejecta

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005spwea...308c02y&link_type=abstract

Space Weather, Volume 3, Issue 8, CiteID S08C02

Astronomy and Astrophysics

Astrophysics

20

Interplanetary Physics: Coronal Mass Ejections (7513), Interplanetary Physics: Interplanetary Magnetic Fields, Solar Physics, Astrophysics, And Astronomy: Magnetic Fields, Space Weather: Forecasting (2722), Space Weather: Magnetic Storms (2788)

Scientific paper

Spectacular burst of solar activity in October-November 2003, when large solar spots and intense solar flares dominated the solar surface for many consecutive days, caused intense geomagnetic storms. In this paper we analyze solar and interplanetary magnetic fields associated with the storms in October-November 2003. We used space- and ground-based data in order to compare the orientations of the magnetic fields on the solar surface and at 1 AU as well as to estimate parameters of geomagnetic storms during this violent period of geomagnetic activity. Our study further supports earlier reports on the correlation between the coronal mass ejection speed and the strength of the magnetic field in an interplanetary ejecta. A good correspondence was also found between directions of the helical magnetic fields in interplanetary ejecta and in the source active regions. These findings are quite significant in terms of their potential to predict the severity of geomagnetic activity 1-2 days in advance, immediately after an Earth directed solar eruption.

Affiliated with

Also associated with

No associations

Rating

Structure of magnetic fields in NOAA active regions 0486 and 0501 and in the associated interplanetary ejecta does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Structure of magnetic fields in NOAA active regions 0486 and 0501 and in the associated interplanetary ejecta, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Structure of magnetic fields in NOAA active regions 0486 and 0501 and in the associated interplanetary ejecta will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-803233