Plasma and Magnetic Fields in the Heliosphere at the Growth Phase of Solar Cycle 23: Comparison with Previous Cycles

Details Plasma and Magnetic Fields in the Heliosphere at the Growth Phase of Solar Cycle 23: Comparison with Previous Cycles Plasma and Magnetic Fields in the Heliosphere at the Growth Phase of Solar Cycle 23: Comparison with Previous Cycles

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001sosyr..35..238v&link_type=abstract

Solar System Research, v. 35, Issue 3, p. 238-242 (2001).

Physics

Scientific paper

The average values of the parameters of the solar wind and the interplanetary magnetic field at the Earth's orbit are calculated by using the results of direct measurements performed in the current and three previous solar cycles. Individual and general features of each cycle are analyzed by the method of superposition of epochs and hysteresis curves. The similarity in trends of solar cycles 23 and 20 at their growth phase is revealed. This gives additional reason to expect that the current solar cycle as a whole will be weaker than the two previous cycles.

Affiliated with

Also associated with

No associations

Rating

Plasma and Magnetic Fields in the Heliosphere at the Growth Phase of Solar Cycle 23: Comparison with Previous Cycles 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 Plasma and Magnetic Fields in the Heliosphere at the Growth Phase of Solar Cycle 23: Comparison with Previous Cycles, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Plasma and Magnetic Fields in the Heliosphere at the Growth Phase of Solar Cycle 23: Comparison with Previous Cycles will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-948495